Index: /trunk/Dwarf/Documents/Agreement/agreement-leo.tex =================================================================== --- /trunk/Dwarf/Documents/Agreement/agreement-leo.tex (revision 8596) +++ /trunk/Dwarf/Documents/Agreement/agreement-leo.tex (revision 8596) @@ -0,0 +1,40 @@ +\documentclass[a4paper]{newletter} +%\usepackage{german} + +\institute{Tuorla Observatory} +\name{Dr.\ Leo Takalo} +\street{V\"{a}is\"{a}l\"{a}ntie 20} +\city{FIN-21500 Piikki\"o} +\email{takalo@utu.fi} +%\tel{Tel: (0551) 39-50\,50} + +\place{Tuorla} +%\date{25. April 2000} + +\begin{document} +\begin{letter}{Universit\"{a}t Dortmund\\Prof.\ Dr. Wolfgang Rhode\\Otto-Hahn-Stra\ss e 4\\44227 Dortmund\\Saksa} + +\opening{Agreement} + +Dear Prof.\ Dr.\ Dr.\ Rhode, dear Prof.\ Dr.\ Mannheim, + +we plan to use the proposed air-Cherenkov telescope prototype system +DWARF on the MAGIC/ORM site on La Palma for the continuous monitoring +of strong blazars. Whenever possible, the monitoring effort at VHE +gamma rays will be complemented at optical and radio wavelengths using +the KVA optical telescope operated by the Tuorla group and the +Mets\"{a}hovi Radio Observatory. The ultimate goal of this program is +to obtain long-term lightcurves of strong blazars to determine their +flux variation power spectrum across a broad wavelength range. Thereby +we expect to achieve a major progress in understanding the mechanism +behind the variable non-thermal emission. The data rights of the +different telescope facilities remain proprietary to the operating +responsibles, but we intend to publish the results of joint campaigns +together on the basis of a consensus decision. + +\vspace{0.5cm} + +\closing{Signature} + +\end{letter} +\end{document} Index: /trunk/Dwarf/Documents/Agreement/agreement-merja.tex =================================================================== --- /trunk/Dwarf/Documents/Agreement/agreement-merja.tex (revision 8596) +++ /trunk/Dwarf/Documents/Agreement/agreement-merja.tex (revision 8596) @@ -0,0 +1,40 @@ +\documentclass[a4paper]{newletter} +%\usepackage{german} + +\institute{Mets\"{a}hovi Radio Observatory} +\name{Dr.\ Merja Tornikoski} +\street{Mets\"{a}hovintie 114} +\city{FIN-02540 Kylm\"{a}l\"{a}} +\email{merja.tornikoski@hut.fi} +%\tel{Tel: (0551) 39-50\,50} + +\place{Kylm\"{a}l\"{a}} +%\date{25. April 2000} + +\begin{document} +\begin{letter}{Universit\"{a}t Dortmund\\Prof.\ Dr. Wolfgang Rhode\\Otto-Hahn-Stra\ss e 4\\44227 Dortmund\\Saksa} + +\opening{Agreement} + +Dear Prof.\ Dr.\ Dr.\ Rhode, dear Prof.\ Dr.\ Mannheim, + +we plan to use the proposed air-Cherenkov telescope prototype system +DWARF on the MAGIC/ORM site on La Palma for the continuous monitoring +of strong blazars. Whenever possible, the monitoring effort at VHE +gamma rays will be complemented at optical and radio wavelengths using +the KVA optical telescope operated by the Tuorla group and the +Mets\"{a}hovi Radio Observatory. The ultimate goal of this program is +to obtain long-term lightcurves of strong blazars to determine their +flux variation power spectrum across a broad wavelength range. Thereby +we expect to achieve a major progress in understanding the mechanism +behind the variable non-thermal emission. The data rights of the +different telescope facilities remain proprietary to the operating +responsibles, but we intend to publish the results of joint campaigns +together on the basis of a consensus decision. + +\vspace{0.5cm} + +\closing{Signature} + +\end{letter} +\end{document} Index: /trunk/Dwarf/Documents/Agreement/agreement.tex =================================================================== --- /trunk/Dwarf/Documents/Agreement/agreement.tex (revision 8596) +++ /trunk/Dwarf/Documents/Agreement/agreement.tex (revision 8596) @@ -0,0 +1,39 @@ +\documentclass[a4paper]{newletter} +%\usepackage{german} + +\name{Tuorla Observatory,\\Dr.\ Leo Takalo} +\street{V\"{a}is\"{a}l\"{a}ntie 20} +\city{21500 Piikki\"o} +\email{takalo@utu.fi} +%\tel{Tel: (0551) 39-50\,50} + +\place{Tuorla} +%\date{25. April 2000} + +\begin{document} +\begin{letter}{Universit\"{a}t Dortmund\\Prof.\ Dr. Wolfgang Rhode\\Otto-Hahn-Stra\ss e 4\\44227 Dortmund\\Saksa} + +\opening{Agreement} + +Dear Prof.\ Dr.\ Dr.\ Rhode, dear Prof.\ Dr.\ Mannheim, + +we plan to use the proposed air-Cherenkov telescope prototype system +DWARF on the MAGIC/ORM site on La Palma for the continuous monitoring +of strong blazars. Whenever possible, the monitoring effort at VHE +gamma rays will be complemented at optical and radio wavelengths using +the KVA optical telescope operated by the Tuorla group and the +Mets\"{a}hovi Radio Observatory. The ultimate goal of this program is +to obtain long-term lightcurves of strong blazars to determine their +flux variation power spectrum across a broad wavelength range. Thereby +we expect to achieve a major progress in understanding the mechanism +behind the variable non-thermal emission. The data rights of the +different telescope facilities remain proprietary to the operating +responsibles, but we intend to publish the results of joint campaigns +together on the basis of a consensus decision. + +\vspace{0.5cm} + +\closing{Signature} + +\end{letter} +\end{document} Index: /trunk/Dwarf/Documents/Agreement/newletter.cls =================================================================== --- /trunk/Dwarf/Documents/Agreement/newletter.cls (revision 8596) +++ /trunk/Dwarf/Documents/Agreement/newletter.cls (revision 8596) @@ -0,0 +1,83 @@ +\NeedsTeXFormat{LaTeX2e} \ProvidesClass{newletter} + +\RequirePackage{ifthen} +\newboolean{@german} \setboolean{@german}{false} +\DeclareOption{german}{\setboolean{@german}{true}} + +\DeclareOption*{\PassOptionsToClass{\CurrentOption}{letter}} +\ProcessOptions +\LoadClass[a4paper]{letter} + +\newcommand{\@email}{} +\newcommand{\@institute}{} +\newcommand{\@street}{} +\newcommand{\@city}{} +\newcommand{\@tel}{} +\newcommand{\@foot}{} + +\newcommand{\email}[1]{\renewcommand{\@email}{#1}} +\newcommand{\institute}[1]{\renewcommand{\@institute}{#1}} +\newcommand{\street}[1]{\renewcommand{\@street}{#1}} +\newcommand{\city}[1]{\renewcommand{\@city}{#1}} +\newcommand{\tel}[1]{\renewcommand{\@tel}{#1}} +\newcommand{\foot}[1]{\renewcommand{\@foot}{#1}} + +\setlength{\textheight}{230mm} +\setlength{\textwidth}{162mm} +\setlength{\topmargin}{-50pt} +\setlength{\oddsidemargin}{0pt} +\setlength{\evensidemargin}{0pt} +\setlength{\headheight}{12pt} +\setlength{\headsep}{35pt} + +\newlength{\leftfield} \setlength{\leftfield}{118.5mm} +\newlength{\rightfield} \setlength{\rightfield}{42.5mm} + +\DeclareFixedFont{\xviisf}{OT1}{cmss}{m}{n}{24.88} +\DeclareFixedFont{\xsf}{OT1}{cmss}{m}{n}{10} +\DeclareFixedFont{\viiisf}{OT1}{cmss}{m}{n}{8} + +\newcommand{\@place}{} + +\renewcommand{\date}[1]{\def\@date{#1}} +\newcommand{\place}[1]{\renewcommand{\@place}{#1}} + +\renewcommand{\ps@firstpage}{ + \setlength{\headheight}{41pt} + \setlength{\headsep}{25pt} + \renewcommand{\@oddhead}{ + \parbox{\textwidth}{ + \raisebox{-6pt}{\parbox[t]{\leftfield}{ + \xviisf\@institute}} + \raisebox{4pt}{\parbox[t]{\rightfield}{ + \viiisf\baselineskip10pt\fromname\\\@street\\\@city}}\\[3pt] + \rule{\textwidth}{1pt}}} + \renewcommand{\@oddfoot}{ %\ifthenelse{ \equal{\@foot}{} }{}{ % + \raisebox{-10pt}[0pt]{ + \parbox{\textwidth}{ + \rule{\textwidth}{0.6pt}\\[2pt] + \mbox{}\hfill + \begin{tabular}[t]{p{5.5cm}}\@foot\end{tabular} }}} %}% + \renewcommand{\@evenhead}{} + \renewcommand{\@evenfoot}{}} + +\renewcommand{\opening}[1]{ + \thispagestyle{firstpage} + \vspace*{24pt} + \parbox[t]{\leftfield}{ + \underline{\footnotesize\itshape\@institute , \@street , \@city}\\ + \parbox[b][3.5cm][c]{\leftfield}{\begin{quote} + \bfseries\toname\\ \toaddress\end{quote}}} + \raisebox{15pt}{\parbox[t]{\rightfield}{ + \large\fromname\\ \@street\\ \@city\\ + \ifthenelse{\equal{\@tel}{}}{}{\@tel\\} \par + \normalsize\slshape + \ifthenelse{\equal{\@email}{}}{}{email: \sffamily\@email\\}}} + \par + \rule{\textwidth}{0.6pt} + \makebox[\leftfield][l]{#1} + \makebox[\rightfield][r]{ + \ifthenelse{\equal{\@place}{}}{M\"unchen, den}{\@place, } \@date} + \vspace{2\parskip}\par\nobreak} + +\renewcommand{\@texttop}{} Index: /trunk/Dwarf/Documents/ApplicationDFG/Makefile =================================================================== --- /trunk/Dwarf/Documents/ApplicationDFG/Makefile (revision 8596) +++ /trunk/Dwarf/Documents/ApplicationDFG/Makefile (revision 8596) @@ -0,0 +1,60 @@ +TARGET = kmwr_mb + +TARGETLIST = $(TARGET).pdf +INTERMEDIATES = $(TARGET).dvi + +all: $(TARGETLIST) + +OPT = -file-line-error-style -interaction=nonstopmode + +.SILENT: + +define run-latex + @echo " - Producing $@ from" $< + ! (latex $(OPT) $< | grep -E \.tex:[0-9]*:\ ) + bibtex --terse $(<:.tex=) + latex $(OPT) $< > /dev/null + latex $(OPT) $< > /dev/null + ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +# ! (latex $(OPT) $< | grep -E \.tex:[0-9]*:\ ) && \ +# bibtex --terse $(<:.tex=); \ +# cp icrc0974.bbl icrc0974.bbl~ && \ +# sed icrc0974.bbl~ -e 's/^\(.*\)\\url\(.*\)%/\1\\url\2/' > icrc0974.bbl && \ +# (latex $(OPT) $< > /dev/null) && \ +# (latex $(OPT) $< > /dev/null) && \ +# ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +# && \ +# ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +endef + +%.dvi: %.dtx + $(run-latex) + +%.dvi: %.tex + $(run-latex) + +%.ps: %.dvi + @echo " - Producing $@ from" $< + dvips -q $< $@~ && mv $@~ $@ + +%.pdf: %.dvi + @echo " - Producing $@ from" $< + dvipdf -q $< $@~ && mv $@~ $@ + +%: %.dvi + @echo " - Producing $@.pdf from" $< + dvipdf -q $< + +%.ps.gz: %.ps + @echo " - Producing booklet $@ from" $< + psbook -q $< | psnup -q -2 | pstops -q 2:0,1VH | gzip -c -9 > $@ + +%.bdf: %.ps.gz + @echo " - Producing booklet $@ from" $< + gzip -cd $< | ps2pdf - $@ + +clean: + @rm -f $(INTERMEDIATES) $(TARGETLIST) *.dvi *.aux *.blg *.lof *.log *.lot *.toc *.bbl *.bdf + +mrproper: clean + @rm -f *~ Index: /trunk/Dwarf/Documents/ApplicationDFG/application.bib =================================================================== --- /trunk/Dwarf/Documents/ApplicationDFG/application.bib (revision 8596) +++ /trunk/Dwarf/Documents/ApplicationDFG/application.bib (revision 8596) @@ -0,0 +1,2574 @@ +------------------------------------------------------------------------------ +Article (author, title, journal, year) + (volume, numbe,r pages, month, note) +Book (author/editor, title, publisher, year) + (volume/number, series, address, edition, month, note) +Conference (author, title, booktitle, year) + (editor, volume/number, organization, series, pages, publisher, address, month, note) +Inproceedings (author, title, booktitle, year) + (editor, volume/number, organization, series, pages, publisher, address, month, note) +Manual (title) + (author, organization, address, edition, month, year, note) +Masterthesis (author, title, school, year) + (address, month, note, type) +phdthesis (author, title, school, year) + (address, month, note, type) +unpublished (author, title, note) + (month, year) +misc () + (author, title, howpublished, month, year, note) +------------------------------------------------------------------------------ + +@MISC{www:fornaxa, key = {{www-01}}, title = {\url{http://www.nrao.edu/imagegallery/}}, year=2006, note={Credit: NRAO/AUI/NSF}} +@MISC{www:agnartist0, key = {{www-02}}, title = {\url{http://integral.esa.int/integ_pictures.html}}, year=2006} +@MISC{www:agnartist, key = {{www-03}}, title = {\url{http://www.spacetelescope.org/images/}}, year=2006, note={Credit: ESA/NASA, the AVO Project and Paolo Padovani}} +@MISC{www:compton, key = {{www-04}}, title = {\url{http://chandra.harvard.edu/resources/illustrations/xlightScatter.html}}, year=2006} +@MISC{www:shower, key = {{www-05}}, title = {\url{http://www.mpi-hd.mpg.de/hfm/CosmicRay/shower.png}}, year=2006} +@MISC{www:showerartist, key = {{www-06}}, title = {\url{http://abyss.uoregon.edu/~js/glossary/cosmic_rays.html}}, year=2006} +@MISC{www:mars, key = {{www-07}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/}}, year=2006} +@MISC{www:google, key = {{www-08}}, title = {\url{http://earth.google.com}}, year=2006} +@MISC{www:slalib, key = {{www-09}}, title = {\url{http://star-www.rl.ac.uk/star/docs/sun67.htx/sun67.html}}, year=2006} +@MISC{www:root, key = {{www-10}}, title = {\url{http://root.cern.ch}}, year=2006} +@MISC{www:htmldoc, key = {{www-11}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/htmldoc/}}, year=2006} +@MISC{www:mysql, key = {{www-12}}, title = {\url{http://www.mysql.com}}, year=2006} +@MISC{www:unified, key = {{www-13}}, title = {\url{http://chandra.harvard.edu/resources/illustrations/quasar.html}}, year=2006, note={Credit: NASA/CXC, Melissa Weiss}} +@MISC{www:asdc, key = {{www-14}}, title = {\url{http://www.asdc.asi.it/blazars/}}, year=2006} +@MISC{www:kva, key = {{www-15}}, title = {\url{http://tur3.tur.iac.es/}}, year=2006} +@MISC{www:integral, key = {{www-16}}, title = {\url{http://altamira.asu.cas.cz/iblwg/show.php?id=131}}, year=2006} +@MISC{www:ned, key = {{www-17}}, title = {\url{http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=1es1218+304}}, year=2006} + +%@MISC{www:BH1m, key = {{www-02}}, title = {\url{http://www.gsfc.nasa.gov/gsfc/spacesci/pictures/blackhole/BH1m.jpg}}, year=2006} +%@MISC{www:hillas, key = {{www-10}}, title = {\url{http://lpnhe-auger.in2p3.fr/slides/hillas.ps}}, year=2006} +%@MISC{www:agnartist2, key = {{www-03}}, title = {\url{http://upload.wikimedia.org/wikipedia/en/4/40/Galaxies_AGN_Inner-Structure-of.jpg}}, year=2006} + + +@BOOK{Peebles:1983, + author = {Peebles, Philip~James~Edwin}, + title = {Principles of Physical Cosmology}, + publisher = {Princton Series in Physics}, + year = 1983 +} + +@BOOK{Weekes:2003, + author = {Weekes, T.~C.}, + title = {Very high energy gamma-ray astronomy}, + series = {Astronomy and Astrophysics}, + publisher = {Institute of Physics Publishing}, + year = 2003 +} + +@BOOK{Rybicki:1979, + author = {{Rybicki}, George B. and {Lightman}, Alan P.}, + title = "Radiative Processes in Astrophysics", + publisher = { Wiley-Interscience }, + year = 1979 +} + +@BOOK{Begelman:1995, + author = {Begelman, M. and Rees, M.}, + title = "{Gravity's Fatal Attraction: Black Holes in the Universe}", + year = 1995, +publisher = {Scientific American Library} +} + +@BOOK{Mueller:2005, + author = {{M\"uller}, A.}, + title = "{Lexikon der Astrophysik}", + year = 2005, + month = sep, + url = {http://www.mpe.mpg.de/~amueller} +} + +@BOOK{Zensus:1987, + author = {{Pearson}, T.~J. and {Zensus}, J.~A.}, + year = 1987, + title = {Superluminal radio sources}, + publisher = {Cambridge University Press} +} + +@BOOK{Schlickeiser:2003, + author = {{Schlickeiser}, Reinhard}, + year = 2003, + title = {Cosmic Ray Astrophysics}, + publisher = {Springer} +} + +@BOOK{Landau:1971, + author = {{Landau}, L.~D. and {Lifshitz}, E.~M.}, + title = "{The classical theory of fields}", + publisher = {Course of theoretical physics - Pergamon International Library of Science, Technology, Engineering and Social Studies, Oxford: Pergamon Press, 1971, 3rd rev.~engl.~edition}, + year = 1971, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1971ctf..book.....L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@MANUAL{Corsika, + author = {{Heck}, D. and {Knapp}, J. and {Capdevielle}, J.~N. and {Schatz}, G. and {Thouw}, T.}, + year = 1998, + title = {{CORSIKA}: {A} {M}onte {C}arlo {C}ode to {S}imulate {E}xtensive {A}ir {S}howers}, +organization = {Forschungszentrum Karlsruhe, {R}eport {FZKA} 6019}, + note = {\url{http://www-ik.fzk.de/corsika/physics\_description/corsika\_phys.html}} +} + +@MANUAL{Breiman, + author = {Breiman, Leo}, + title = {Machine Learning 45(1), 5}, + year = 2001 +} + +@MASTERSTHESIS{Doro:Diploma, + author = {Doro, M.}, + title = {The Commissioning and Characterization of the Calibration System of the {MAGIC} Telescope}, + school = {Universit{\'a} di Padova}, + year = {2004}, + note = {\url{http://wwwmagic.mppmu.mpg.de/publications/theses/LaureaMDoro.ps.gz}} +} + +@MASTERSTHESIS{Stefan:Diploma, + author = {R\"ugamer, S.}, + title = {}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2006}, + note = {in preparation} +} + +@MASTERSTHESIS{Hoehne:Diploma, + author = {H\"ohne, D.}, + title = "{Beobachtung von HESS\,J1813-178 mit dem MAGIC-Teleskop}", + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + month = sep, + year = {2005}, +} + +@MASTERSTHESIS{Dorner:Diploma, + author = {Dorner, D.}, + title = {{S}ystem zum {A}usrichten und {N}achf\"uhren des {MAGIC}-{T}eleskops}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2003} +} + +@MASTERSTHESIS{Riegel:Diploma, + author = {Riegel, B.}, + title = {{S}ystematische {U}ntersuchung der {B}ildparameter f\"ur das {MAGIC}-{T}eleskop}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2005} +} + +@MASTERSTHESIS{Bretz:1999, + author = {Bretz, T.}, + title = {Magnetfeldeigenschaften des {S}pektrometers {HADES}}, + school = {Technische Universit{\"a}t M{\"u}nchen}, + year = {1999} +} + +%MASTERSTHESIS{Doro:2005, +% author = {Doro, Michele}, +% year = {2005} +% + +@MISC{Giommi:2006, + author = { Giommi, P. and others}, + year = 2006, + howpublished = {in preparation} +} + +@MISC{Giommi:2005, + author = { Giommi, P.}, + year = 2006, + howpublished = {private communication} +} + +@ARTICLE{Dondi:1995, + author = {{Dondi}, L. and {Ghisellini}, G.}, + title = "{Gamma-ray-loud blazars and beaming}", + journal = {\mnras}, + year = 1995, + month = apr, + volume = 273, + pages = {583-595}, + asdurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995MNRAS.273..583D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fermi:1954, + author = {{Fermi}, E.}, + title = "{Galactic Magnetic Fields and the Origin of Cosmic Radiation.}", + journal = {\apj}, + year = 1954, + month = jan, + volume = 119, + pages = {1-+}, + doi = {10.1086/145789}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1954ApJ...119....1F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fermi:1949, + author = {{Fermi}, E.}, + journal = {Phys.~Rev.}, + volume = 75, + pages = 1169, + year = {1949} +} + +@ARTICLE{Wentzel:1963, + author = {{Wentzel}, D.~G.}, + title = "{Fermi Acceleration of Charged Particles.}", + journal = {\apj}, + year = 1963, + month = jan, + volume = 137, + pages = {135-+}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1963ApJ...137..135W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@BOOK{Spitzer:1956, + author = {{Spitzer}, L.}, + title = "{Physics of Fully Ionized gases}", +publisher = {Interscience, New York }, + year = 1956, +} + +@ARTICLE{Einstein:1905, + author = {{Einstein}, A.}, + title = "{Zur Elektrodynamik bewegter K{\"o}rper}", + journal = {Annalen der Physik}, + year = 1905, + volume = 17, + pages = {891-921}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1905AnP....17..891E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Einstein:1916, + author = {{Einstein}, A.}, + title = "{Die Grundlage der allgemeinen Relativit{\"a}tstheorie}", + journal = {Annalen der Physik}, + year = 1916, + volume = 49, + pages = {769-822}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1916AnP....49..769E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Eddington:1935a, + author = {{Eddington}, A.~S.}, + title = "{On "relativistic degeneracy,"}", + journal = {\mnras}, + year = 1935, + month = jan, + volume = 95, + pages = {194-206}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1935MNRAS..95..194E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Rindler:1956, + author = {{Rindler}, W.}, + title = "{Visual horizons in world models}", + journal = {\mnras}, + year = 1956, + volume = 116, + pages = {662-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1956MNRAS.116..662R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}, +} + +@ARTICLE{Eddington:1935b, + author = {{Eddington}, A.~S.}, + title = "{Note on "relativistic degeneracy"}", + journal = {\mnras}, + year = 1935, + month = nov, + volume = 96, + pages = {20-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1935MNRAS..96...20E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Chandrasekhar:1931, + author = {{Chandrasekhar}, S.}, + title = "{The Maximum Mass of Ideal White Dwarfs}", + journal = {\apj}, + year = 1931, + month = jul, + volume = 74, + pages = {81-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1931ApJ....74...81C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Oppenheimer:1939, + author = {{Oppenheimer}, Julius Robert and {Snyder}, Hartland}, + title = {On continued gravitational contraction}, + journal = {Phys.~Rev.}, + volume = 56, + pages = 455, + year = {1939} +} + +@ARTICLE{Kerr:1963, + author = {{Kerr}, Roy Patrick}, + title = {Gravitational field of a spinning mass as an example of algebraically special metrics}, + journal = {\prl}, + volume = 11, + pages = 237, + year = {1963} +} + +@ARTICLE{Bolton:1971, + author = {{Bolton}, C.~T.}, + title = {Identification of {Cyg} {X}-1 with {HDE} 226868}, + journal = {\nat}, + year = 1972, + volume = 235, + pages = {271}, +} + +@ARTICLE{Shakura:1973, + author = {{Shakura}, N.~I. and {Sunyaev}, R.~A.}, + title = "{Black holes in binary systems. Observational appearance.}", + journal = {\aap}, + year = 1973, + volume = 24, + pages = {337-355}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1973A%26A....24..337S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hasinger:1998, + author = {{Hasinger}, G. and {Burg}, R. and {Giacconi}, R. and {Schmidt}, M. and + {Trumper}, J. and {Zamorani}, G.}, + title = "{The ROSAT Deep Survey. I. X-ray sources in the Lockman Field}", + journal = {\aap}, + year = 1998, + month = jan, + volume = 329, + pages = {482-494}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998A%26A...329..482H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{LyndenBell:1969, + author = {{Lynden-Bell}, D.}, + title = "{Galactic Nuclei as Collapsed Old Quasars}", + journal = {\nat}, + year = 1969, + volume = 223, + pages = {690-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1969Natur.223..690L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Georga:1988, + author = {{George}, I.~M. and {Warwick}, R.~S. and {Bromage}, G.~E.}, + title = "{X-ray and ultraviolet observations of Markarian 421}", + journal = {\mnras}, + year = 1988, + month = jun, + volume = 232, + pages = {793-808}, + adsurl = 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Modification of gamma-ray spectra}, + journal = {\aap}, + year = 2004, + month = jan, + volume = 413, + pages = {807-815}, + doi = {10.1051/0004-6361:20031542}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004A%26A...413..807K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kneiske:2002, + author = {{Kneiske}, T.~M. and {Mannheim}, K. and {Hartmann}, D.~H.}, + title = {Implications of cosmological gamma-ray absorption. {I}. {E}volution of the metagalactic radiation field}, + journal = {\aap}, + year = 2002, + month = apr, + volume = 386, + pages = {1-11}, + doi = {10.1051/0004-6361:20020211}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2002A%26A...386....1K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hernandez:2005, + author = {{Hern{\'a}ndez-Rey}, J.~J.}, + title = "{The Neutrino Telescope Antares}", + journal = {\apss}, + year = 2005, + month = jun, + volume = 297, + pages = {257-267}, + doi = {10.1007/s10509-005-7628-4}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005Ap%26SS.297..257H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Bretz:2003icrc, + author = {{Bretz}, T.}, + title = {The {MAGIC} {A}nalysis and {R}econstruction {S}oftware}, +booktitle = {$28^{th}$ International Cosmic Ray Conference}, + year = 2003, + month = Aug +} + +@INPROCEEDINGS{Bretz:2004gamma, + author = {{Bretz}, T.}, + title = {{MARS} - {R}oadmap to a standard analysis}, +booktitle = {$2^{nd}$ International Symposium on High Energy Gamma-Ray Astronomy}, + year = 2004, + month = Jul +} + +@INPROCEEDINGS{Bretz:2005paris, + author = {{Bretz}, T. and Dorner, D.}, + title = {{MARS} - {A} framework for a standard analysis}, +booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, + year = 2005, + month = Apr +} + +@INPROCEEDINGS{Dorner:2005paris, + author = {{Dorner}, D. and Bretz, T.}, + title = {A concept for data managment and processing}, +booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, + pages = {571-575}, + year = 2005, + month = Apr +} + +@INPROCEEDINGS{Bastieri:2005, + author = {Bastieri, D. and others}, + title = {The mirrors of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Dorner:2005icrc, + author = {Dorner, D. and Berger, K. and Bretz, T. and Gaug, M. and others}, + title = {Data Managment and Processing for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 175, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Beixeras:2005, + author = {Beixeras, C. and others}, + title = "{MAGIC II}", +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + volume = 5, + pages = {227}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Cortina:2005, + author = {Cortina, J. and others}, + title = {Technical performance of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Bretz:2005mars, + author = {Bretz, T.}, + title = {Standard Analysis for the {MAGIC} Telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + volume = 4, + year = 2005, + pages = 315, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Gaug:2005, + author = {Gaug, M. and Bartko, H. and Cortina, J. and Rico, J. and others}, + title = {Calibration of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Riegel:2005icrc, + author = {{Riegel}, B. and Bretz, T.}, + title = {A systematic study of the interdependance of the {IACT} image parameters}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 215, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Riegel:2005icrc2, + author = {{Riegel}, B. and Bretz, T. and Dorner, D. and Wagner, R.~M. and others}, + title = {A tracking monitor for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 219, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Goebel:2005, + author = {{Goebel}, F. and Mase, K. and Meyer, M. and Mirzoyan, R. and Shayduk, M. and Teshima, M. and others}, + title = {Absolute energy scale calibration of the {MAGIC} telescope using muon images}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Majumdar:2005icrc, + author = {{Majumdar}, P. and {Moralejo}, A. and {Bigongiari}, C. and {Blanch}, O. and {Sobczynska}, D.}, + title = {{M}onte {C}arlo simulation for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Meyer:2005icrc, + author = {{Meyer}, M. and Mannheim, K. and Bretz, T. and Dorner, D. and Riegel, B. and H\"ohne, D. and Berger, K. and others}, + title = {{MAGIC} observations of high-peaked {BL} {L}ac objects}, +booktitle = {$28^{th}$ International Cosmic Ray Conference}, + volume = 4, + pages = 335, + year = 2005, + month = Aug, + note = {astro-ph/0508273} +} + +@ARTICLE{Lessard:2001, + author = {{Lessard}, R.~W. and {Buckley}, J.~H. and {Connaughton}, V. and {Le Bohec}, S.}, + title = "{A new analysis method for reconstructing the arrival direction of TeV gamma rays using a single imaging atmospheric Cherenkov telescope}", + journal = {Astroparticle Physics}, + year = 2001, + month = mar, + volume = 15, + pages = {1-18}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001APh....15....1L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Urry:1995, + author = {{Urry}, C.~M. and {Padovani}, P.}, + title = "{Unified Schemes for Radio-Loud Active Galactic Nuclei}", + journal = {\pasp}, + year = 1995, + month = sep, + volume = 107, + pages = {803-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995PASP..107..803U&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Urry:2000, + author = {{Urry}, C.~M. and {Scarpa}, R. and {O'Dowd}, M. and {Falomo}, R. and + {Pesce}, J.~E. and {Treves}, A.}, + title = "{The Hubble Space Telescope Survey of BL Lacertae Objects. II. Host Galaxies}", + journal = {\apj}, + year = 2000, + month = apr, + volume = 532, + pages = {816-829}, + doi = {10.1086/308616}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000ApJ...532..816U&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Porter:1960, + author = {Hill, D.~A. and Porter, N.~A}, + title = "{Photography of \v{C}erenkov Light from Extensive Air Showers in the Atmosphere}", + month = aug, + year = 1960, + journal = {\nat}, + volume = 191, + pages = 690, + note = {Letters to Editor} +} + +@ARTICLE{Jelley:1963, + author = {{Jelley}, J.~V. and {Porter}, N.~A.}, + title = "{{\v C}erenkov Radiation from the Night Sky, and its Application to {$\gamma$}-Ray Astronomy}", + journal = {\qjras}, + year = 1963, + month = sep, + volume = 4, + pages = {275-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1963QJRAS...4..275J&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Padovani:1995, + author = {{Padovani}, P. and {Giommi}, P.}, + title = "{The connection between x-ray- and radio-selected BL Lacertae objects}", + journal = {\apj}, + year = 1995, + month = may, + volume = 444, + pages = {567-581}, + doi = {10.1086/175631}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...444..567P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Boella:1997, + author = {{Boella}, G. and {Butler}, R.~C. and {Perola}, G.~C. and {Piro}, L. and + {Scarsi}, L. and {Bleeker}, J.~A.~M.}, + title = "{BeppoSAX, the wide band mission for X-ray astronomy}", + journal = {\aaps}, + year = 1997, + month = apr, + volume = 122, + pages = {299-307}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997A%26AS..122..299B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Catanese:1999, + author = {{Catanese}, M. and {Weekes}, T.~C.}, + title = "{Very High Energy Gamma-Ray Astronomy}", + journal = {\pasp}, + year = 1999, + month = oct, + volume = 111, + pages = {1193-1222}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999PASP..111.1193C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Daum:1997, + author = {{Daum}, A. and others}, + title = "{First results on the performance of the HEGRA IACT array}", + journal = {Astroparticle Physics}, + year = 1997, + month = dec, + volume = 8, + pages = {1-2}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997APh.....8....1D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Aharonian:2004, + author = {{Aharonian}, F. and others}, + title = "{Observations of 54 Active Galactic Nuclei with the HEGRA system of Cherenkov telescopes}", + journal = {\aap}, + year = 2004, + month = jul, + volume = 421, + pages = {529-537}, + doi = {10.1051/0004-6361:20035764}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004A%26A...421..529A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Pohl:2000, + author = {{Pohl}, M. and {Schlickeiser}, R.}, + title = "{On the conversion of blast wave energy into radiation in active galactic nuclei and gamma-ray bursts}", + journal = {\aap}, + year = 2000, + month = feb, + volume = 354, + pages = {395-410}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000A%26A...354..395P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1993, + author = {{Mannheim}, K.}, + title = "{The proton blazar}", + journal = {\aap}, + year = 1993, + month = mar, + volume = 269, + pages = {67-76}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993A%26A...269...67M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# CHECK AGAIN! +@INPROCEEDINGS{Sikora:2001, + author = {{Sikora}, M.}, + title = "{Jets in Quasars}", +booktitle = {ASP Conf. Ser. 227: Blazar Demographics and Physics}, + year = 2001, + pages = {95-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ASPC..227...95S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sikora:1987, + author = {{Sikora}, M. and {Kirk}, J.~G. and {Begelman}, M.~C. and {Schneider}, P. + }, + title = "{Electron injection by relativistic protons in active galactic nuclei}", + journal = {\apjl}, + year = 1987, + month = sep, + volume = 320, + pages = {L81-L85}, + doi = {10.1086/184980}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987ApJ...320L..81S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# CHECK AGAIN +@ARTICLE{Burns:1982, + author = {{Burns}, M.~L. and {Lovelace}, R.~V.~E.}, + title = "{Theory of electron-positron showers in double radio sources}", + journal = {\apj}, + year = 1982, + month = nov, + volume = 262, + pages = {87-99}, + doi = {10.1086/160399}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...262...87B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Svensson:1987, + author = {{Svensson}, R.}, + title = "{Non-thermal pair production in compact X-ray sources - First-order Compton cascades is soft radiation fields}", + journal = {\mnras}, + year = 1987, + month = jul, + volume = 227, + pages = {403-451}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987MNRAS.227..403S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@BOOK{Berezinskii:1990, + author = {{Berezinskii}, V.~S. and {Bulanov}, S.~V. and {Dogiel}, V.~A. and + {Ptuskin}, V.~S.}, + title = "{Astrophysics of cosmic rays}", +publisher = {Amsterdam: North-Holland, 1990, edited by Ginzburg, V.L.}, +year = 1990, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1990acr..book.....B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1991, + author = {{Mannheim}, K. and {Biermann}, P.~L. and {Kruells}, W.~M.}, + title = "{A novel mechanism for nonthermal X-ray emission}", + journal = {\aap}, + year = 1991, + month = nov, + volume = 251, + pages = {723-731}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1991A%26A...251..723M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Mannheim:1997, + author = {{Mannheim}, K.}, + title = "{AGN Models: High-Energy Emission.}", +booktitle = {Very High Energy Phenomena in the Universe; Moriond Workshop}, + year = 1997, + pages = {17-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997vhep.conf...17M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1998, + author = {{Mannheim}, K.}, + title = "{Possible Production of High-Energy Gamma Rays from Proton Acceleration in the Extragalactic Radio Source Markarian 501}", + journal = {Science}, + year = 1998, + month = jan, + volume = 279, + pages = {684-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998Sci...279..684M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hauser:2001, + author = {{Hauser}, M.~G. and {Dwek}, E.}, + title = "{The Cosmic Infrared Background: Measurements and Implications}", + journal = {\araa}, + year = 2001, + volume = 39, + pages = {249-307}, + doi = {10.1146/annurev.astro.39.1.249}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ARA%26A..39..249H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# TO BE CHECKED! +@ARTICLE{Perlman:1998, + author = {{Perlman}, E.~S. and {Padovani}, P. and {Giommi}, P. and {Sambruna}, R. and + {Jones}, L.~R. and {Tzioumis}, A. and {Reynolds}, J.}, + title = "{The Deep X-Ray Radio Blazar Survey. I. Methods and First Results}", + journal = {\aj}, + year = 1998, + month = apr, + volume = 115, + pages = {1253-1294}, + doi = {10.1086/300283}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998AJ....115.1253P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Laurent-Muehleisen:1998, + author = {{Laurent-Muehleisen}, S.~A. and {Kollgaard}, R.~I. and {Feigelson}, E.~D. + }, + title = "{The Rosat-Green Bank Sample of Intermediate BL Lac Objects}", +booktitle = {ASP Conf. Ser. 144: IAU Colloq. 164: Radio Emission from Galactic and Extragalactic Compact Sources}, + year = 1998, + pages = {163-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998ASPC..144..163L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Caccianiga:1999, + author = {{Caccianiga}, A. and {Maccacaro}, T. and {Wolter}, A. and {della Ceca}, R. and + {Gioia}, I.~M.}, + title = "{The REX Survey: A Search for Radio-emitting X-Ray Sources}", + journal = {\apj}, + year = 1999, + month = mar, + volume = 513, + pages = {51-68}, + doi = {10.1086/306822}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999ApJ...513...51C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Caccianiga:2004, + author = {{Caccianiga}, A. and {March{\~a}}, M.~J.~M.}, + title = "{The CLASS blazar survey: testing the blazar sequence}", + journal = {\mnras}, + year = 2004, + month = mar, + volume = 348, + pages = {937-954}, + doi = {10.1111/j.1365-2966.2004.07415.x}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004MNRAS.348..937C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kellermann:1989, + author = {{Kellermann}, K.~I. and {Sramek}, R. and {Schmidt}, M. and {Shaffer}, D.~B. and + {Green}, R.}, + title = "{VLA observations of objects in the Palomar Bright Quasar Survey}", + journal = {\aj}, + year = 1989, + month = oct, + volume = 98, + pages = {1195-1207}, + doi = {10.1086/115207}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1989AJ.....98.1195K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Rowan:1977, + author = {{Rowan-Robinson}, M.}, + title = "{On the unity of activity in galaxies}", + journal = {\apj}, + year = 1977, + month = may, + volume = 213, + pages = {635-647}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1977ApJ...213..635R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lawrence:1982, + author = {{Lawrence}, A. and {Elvis}, M.}, + title = "{Obscuration and the various kinds of Seyfert galaxies}", + journal = {\apj}, + year = 1982, + month = may, + volume = 256, + pages = {410-426}, + doi = {10.1086/159918}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...256..410L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Giommi:1994, + author = {{Giommi}, P. and {Padovani}, P.}, + title = "{Bl-Lacertae Reunification}", + journal = {\mnras}, + year = 1994, + month = may, + volume = 268, + pages = {L51+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994MNRAS.268L..51G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Antonucci:1985, + author = {{Antonucci}, R.~R.~J. and {Ulvestad}, J.~S.}, + title = "{Extended radio emission and the nature of blazars}", + journal = {\apj}, + year = 1985, + month = jul, + volume = 294, + pages = {158-182}, + doi = {10.1086/163284}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ApJ...294..158A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fossati:1998, + author = {{Fossati}, G. and {Maraschi}, L. and {Celotti}, A. and {Comastri}, A. and + {Ghisellini}, G.}, + title = "{A unifying view of the spectral energy distributions of blazars}", + journal = {\mnras}, + year = 1998, + month = sep, + volume = 299, + pages = {433-448}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998MNRAS.299..433F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Aharonian:2000, + author = {{Aharonian}, F.}, + title = "{TeV gamma rays from BL Lac objects due to synchrotron radiation of extremely high energy protons}", + journal = {\na}, + year = 2000, + month = nov, + volume = 5, + pages = {377-395}, + doi = {10.1016/S1384-1076(00)00039-7}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000NewA....5..377A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Muecke:2003, + author = {{M{\"u}cke}, A. and {Protheroe}, R.~J. and {Engel}, R. and {Rachen}, J.~P. and + {Stanev}, T.}, + title = "{BL Lac objects in the synchrotron proton blazar model}", + journal = {Astroparticle Physics}, + year = 2003, + month = mar, + volume = 18, + pages = {593-613}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003APh....18..593M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Schlickeiser:2000, + author = {{Pohl}, M. and {Schlickeiser}, R.}, + title = "{On the conversion of blast wave energy into radiation in active galactic nuclei and gamma-ray bursts}", + journal = {\aap}, + year = 2000, + month = feb, + volume = 354, + pages = {395-410}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000A%26A...354..395P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lyutikov:2005, + author = {{Lyutikov}, M.}, + title = "{Composition of ultra-relativistic jets}", + journal = {American Astronomical Society Meeting Abstracts}, + year = 2005, + month = may, + volume = 206, + pages = {-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005AAS...206.3008L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sikora:2005, + author = {{Sikora}, M. and {Begelman}, M.~C. and {Madejski}, G.~M. and + {Lasota}, J.-P.}, + title = "{Are Quasar Jets Dominated by Poynting Flux?}", + journal = {\apj}, + year = 2005, + month = may, + volume = 625, + pages = {72-77}, + doi = 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(A79-30026 11-90) Pittsburgh, Pa., University of Pittsburgh, 1978, p. 328-341; Discussion, p. 341-347. NATO-supported research}, + year = 1978, + pages = {328-341}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1978bllo.conf..328B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Bradbury:1997, + author = {{Bradbury}, S.~M. and others}, + title = "{Detection of {$\gamma$}-rays above 1.5TeV from MKN 501.}", + journal = {\aap}, + year = 1997, + month = apr, + volume = 320, + pages = {L5-L8}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997A%26A...320L...5B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Browne:1983, + author = {{Browne}, I.~W.~A.}, + title = "{Is it possible to turn an elliptical radio galaxy into a BL Lac object?}", + journal = {\mnras}, + year = 1983, + month = jul, + volume = 204, + pages = {23P-27P}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1983MNRAS.204P..23B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Celotti:2003, + author = {{Celotti}, A.}, + title = "{On the energetics and composition of jets}", + journal = {\nar}, + year = 2003, + month = oct, + volume = 47, + pages = {525-528}, + doi = {10.1016/S1387-6473(03)00086-1}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003NewAR..47..525C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Wardle:1984, + author = {{Wardle}, J.~F.~C. and {Moore}, R.~L. and {Angel}, J.~R.~P.}, + title = "{The radio morphology of blazars and relationships to optical polarization and to normal radio galaxies}", + journal = {\apj}, + year = 1984, + month = apr, + volume = 279, + pages = {93-98}, + doi = {10.1086/161868}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1984ApJ...279...93W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lind:1985, + author = {{Lind}, K.~R. and {Blandford}, R.~D.}, + title = "{Semidynamical models of radio jets - Relativistic beaming and source counts}", + journal = {\apj}, + year = 1985, + month = aug, + volume = 295, + pages = {358-367}, + doi = {10.1086/163380}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ApJ...295..358L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Phinney:1986, + author = {{Phinney}}, + title = {Astrophysics of {A}ctive {G}alaxies and {QSO}s}, +publisher = {Oxford University Press}, + editor = {R.W.Miller}, + year = 1986, + page = 453, +} + +@ARTICLE{Fazio:1979, + author = {{Fazio}, G.~G. and {Stecker}, F.~W.}, + year = 1979, + volume = 226, + pages = {135-+}, + title = {Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin}, + journal = {\nat} +} + +@ARTICLE{Punch:1992, + author = {{Punch}, M. and others}, + title = "{Detection of TeV photons from the active galaxy Markarian 421}", + journal = {\nat}, + year = 1992, + month = aug, + volume = 358, + pages = {477-+}, + doi = {10.1038/358477a0}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992Natur.358..477P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fanaroff:1974, + author = {{Fanaroff}, B.~L. and {Riley}, J.~M.}, + title = "{The morphology of extragalactic radio sources of high and low luminosity}", + journal = {\mnras}, + year = 1974, + month = may, + volume = 167, + pages = {31P-36P}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1974MNRAS.167P..31F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Odell:1974, + author = {{Jones}, T.~W. and {O'dell}, S.~L. and {Stein}, W.~A.}, + title = "{Physics of Compact Nonthermal Sources. 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acceleration of charged particles at relativistic shock fronts}", + journal = {\apj}, + year = 1987, + month = apr, + volume = 315, + pages = {425-433}, + doi = {10.1086/165147}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987ApJ...315..425K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kirk:1998, + author = {{Kirk}, J.~G. and {Rieger}, F.~M. and {Mastichiadis}, A.}, + title = "{Particle acceleration and synchrotron emission in blazar jets}", + journal = {\aap}, + year = 1998, + month = may, + volume = 333, + pages = {452-458}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998A%26A...333..452K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lawrence:1987, + author = {{Lawrence}, A.}, + title = "{Classification of active galaxies and the prospect of a unified phenomenology}", + journal = {\pasp}, + year = 1987, + month = may, + volume = 99, + pages = {309-334}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987PASP...99..309L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Padovani:1993, + author = {{Padovani}, P.}, + title = "{The Radio Loud Fraction of QSOs and its Dependence on Magnitude and Redshift}", + journal = {\mnras}, + year = 1993, + month = jul, + volume = 263, + pages = {461-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993MNRAS.263..461P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{LaFranca:1994, + author = {{La Franca}, F. and {Gregorini}, L. and {Cristiani}, S. and + {de Ruiter}, H. and {Owen}, F.}, + title = "{Deep VLA observations of an optically selected sample of intermediate redshift QSOs and the optical luminosity function of the radio loud QSOs}", + journal = {\aj}, + year = 1994, + month = nov, + volume = 108, + pages = 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month = nov, + volume = 399, + pages = {L23-L26}, + doi = {10.1086/186597}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992ApJ...399L..23P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Pier:1993, + author = {{Pier}, E.~A. and {Krolik}, J.~H.}, + title = "{Infrared Spectra of Obscuring Dust Tori around Active Galactic Nuclei. 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Sci. {\bf 49} (2002) 2497. + +\bibitem{MC_timing_Indians} +V.~R. {Chitnis} and P.~N. {Bhat}, +\newblock {\em {Possible discrimination between gamma rays and hadrons using + {\v C}erenkov photon timing measurements}}, +\newblock Astroparticle Physics {\bf 15} (2001) 29. + +----------------------------------------------------------------------------------- + +@ARTICLE{Aharonian:2006 + author = {{Aharonian}, F. and others}, + title = "{The H.E.S.S.\ Survey of the Inner Galaxy in Very High Energy Gamma Rays}", + journal = {\apj}, + year = 2006, + month = jan, + volume = 636, + pages = {777-797}, + doi = {10.1086/498013}, + adsurl = {http://cdsads.u-strasbg.fr/abs/2006ApJ...636..777A}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Paneque:2004, + author = {{Paneque}, D. and {Gebauer}, H.~J. and {Lorenz}, E. and {Mirzoyan}, R. + }, + title = "{A method to enhance the sensitivity of photomultipliers for Air Cherenkov Telescopes by applying a lacquer that scatters light}", + journal = {Nuclear Instruments and Methods in Physics Research A}, + year = 2004, + month = feb, + volume = 518, + pages = {619-621}, + doi = {10.1016/j.nima.2003.11.101}, + adsurl = {http://cdsads.u-strasbg.fr/abs/2004NIMPA.518..619P}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} Index: /trunk/Dwarf/Documents/ApplicationDFG/application.tex =================================================================== --- /trunk/Dwarf/Documents/ApplicationDFG/application.tex (revision 8596) +++ /trunk/Dwarf/Documents/ApplicationDFG/application.tex (revision 8596) @@ -0,0 +1,1059 @@ +\documentclass[12pt,openbib]{article} +\usepackage{german,graphicx,amssymb,amsmath,wasysym,stmaryrd,times,a4wide,wrapfig,exscale,xspace,url,fancyhdr} +\usepackage[round]{natbib} + +%cleardoubleplain,liststotoc,bibtotoc,idxtotoc, + +%\documentclass[a4paper,12pt,oneside,german]{article} +%\usepackage[ansinew]{inputenc} + +\input library.def + +\frenchspacing + +\newcommand{\loi}{\large \textbf{LoI:}\normalsize} +\newcommand{\anmerk}[1]{ \marginpar + [{\parbox[t]{19.mm}{\footnotesize\sf {#1}} + \parbox[t]{2.mm}{\rule[-14.4mm]{1.mm}{17.mm}}}] + {\parbox[t]{2.mm}{\rule[-14.4mm]{1.mm}{17.mm}}\parbox[t]{17.mm}{ + \footnotesize \sf {#1} } } } + + +%\textwidth17cm +%\oddsidemargin-0.5cm +%\oddsidemargin-1.cm +%\textheight25cm +%\topmargin=-1.5cm + + +\begin{document} +\noindent + +{\LARGE{\bf +\begin{center} +Antrag auf Gew"ahrung einer Sachbeihilfe\\Proposal for a research project +\end{center} +}} + +\noindent {\it Das Inhaltsverzeichnis dient nur zur "Ubersicht und ist im eigentlichen Antrag nicht enthalten. \\ + +\ + +{\underline{\bf to do Liste}}\\ +\begin{itemize} + \item [1.6] Es muss sich jemand einen der Texte (oder ein Konglomerat daraus) aussuchen. + \item [2.1] ist inhaltlich (u.A.) um die (z.T. in deutsch) angegebenen Stichpunkte zu erg"anzen. + \item [2.2] ist noch (von Wolfgang und Karl?) zu schreiben. + \item [3.1] ist inhaltlich (u.A.) um die (z.T. in deutsch) angegebenen Stichpunkte zu erg"anzen. + \item [3.2] ist w"ortlich aus dem LoI kopiert und bedarf wom"oglich einer "Uberarbeitung im Sinne der Kapitel"uberschrift. + \item [4.x] sind sprachlich, inhaltlich und optisch zu "uberarbeiten. + \item [5.1] ist sprachlich (in deutsch lassen?) und inhaltlich (v.A. W"urzburg) zu "uberarbeiten. + \item [5.2] ist inhaltlich (u.A.) um die angegebenen Stichpunkte und Informationen aus W"urzburg zu erg"anzen. + \item [--] Plots und Bilder sind noch zu erg"anzen. + \item [--] Referenzen sind im ganzen Text noch zu erg"anzen. + \item [{\bf alles}] muss nat"urlich noch auf Orthographie und "`sprachliche Eleganz"' hin gegengelesen werden. +\end{itemize} +\newpage +} +\tableofcontents +\newpage +%%% + +{\LARGE{\bf +\begin{center} +Neuantrag auf Gew"ahrung einer Sachbeihilfe\\Proposal for a research project +\end{center} +}} + +\section{Allgemeine Angaben/General Information}\anmerk{Die Gliederung ist von der DFG vorgegeben} + +\subsection{Antragsteller/Applicants} +% IN CASE A PROJECT IS DISTRIBUTED BETWEEN SEVERAL INSTITUTES +% PLEASE GIVE AT LEAST ONE APPLICANT FOR EACH INSTITUTE; +% ALSO, IN THIS CASE, THE PROPOSAL MUST MAKE CLEAR WHICH +% RESOURCES GO TO WHERE, HOW THE WORK IS SPLIT, HOW THE INTERACTION +% SHALL PROCEED ETC. +{\bf Rhode, Wolfgang, Prof.~Dr.~Dr.}\\ +Universit"atsprofessor (C3)\\ +born Oct 17 1961, Nationality: German\\ +Institut f"ur Physik\\ +Lehrstuhl: Experimentelle Physik V (Astroteilchenphysik)\\ + +Dienstaddresse:\\ +Universit"at Dortmund\\ +D-44221 Dortmund\\ +\begin{tabular}{ll} +Phone:&+49\,(231)\,755-3550\\ +Fax:&+49\,(231)\,755-4547\\ +Email:&wolfgang.rhode@udo.edu\\ +\end{tabular} + +\noindent +Home address: Am Schilken 28, 58285 Gevelsberg (TELEFONNUMMER) + +\vskip0.3cm\noindent +{\bf Mannheim, Karl, Prof.~Dr.}\\ +Universit"atsprofessor (C4)\\ +born Jan 4 1960, Nationality: German\\ +Institut f"ur Theoretische Physik und Astrophysik\\ +Lehrstuhl f"ur Astronomie\\ + +Dienstaddresse:\\ +Julius-Maximilian-Universit"at W"urzburg\\ +D-97074 W"urzburg\\ +\begin{tabular}{ll} +Phone:&+49\,(931)\,888-5031\\ +Fax:&+49\,(931)\,888-4603\\ +Email:&mannhein@astro.uni-wuerzbueg.de\\ +\end{tabular} + +\noindent +Home address: Oswald-Kunzemann-Str. 12, 97299 Zell am Main (TELEFON) +%} + +\subsection{Thema/Topic} +Long-term VHE $\gamma$-ray monitoring of bright blazars with a dedicated Cherenkov telescope + +\subsection{Fachgebiet und Arbeitsrichtung\\Scientific discipline and field of work} +Astronomy and Astrophysics, Particle Astrophysics + +\subsection{Voraussichtliche Gesamtdauer/Scheduled duration in total} +3\,years + +\subsection{Antragszeitraum/Application period} +3\,years. Work on the project may and will begin immediately after the +funding. + +\clearpage + +\subsection{Zusammenfassung/Summary} +\anmerk{nicht mehr als 15 Zeilen oder max. 1600 Zeichen. + in 12pt sind 1600 Zeichen aber 19 Zeilen} + +Beantragt \citeauthor{Chandrasekhar:1931} wird die F"orderung eines +Luft-Cherenkov-Teleskops f"ur Langzeitbeobachtungen von Gamma-Quellen +im Energiebereich zwischen 500 GeV und 50 TeV (DWARF=Dedicated +multiWavelength Astroparticle Research Facility). Mit DWARF sollen zwei +Aufgaben bei der Beobachtung erf"ullt werden: 1. weitgehend +automatisierte Langzeitbeobachtungen von bekannten hochenergetischen +Quellen. Solche Beobachtungen stehen nicht auf dem Programm der im +Betrieb befindlichen Generation von Cherenkov-Teleskopen 2. +Multiwavelenght-Kampangen mit Photon-Detektoren in unterschiedlichen +Energiebreichen, insbesondere auch mit dem Neutrino-Teleskop IceCube. +F"ur den Aufbau von DWARF soll die bestehende Infrastruktur auf dem +Roque de los Muchachos auf der kanarischen Insel La Palma genutzt +werden. Dort befindet sich der zur Zeit ungenutzte Mount des +ehemaligen ``HEGRA-Cherenkov-Teleskops 3'' sowie eine zur Plazierung +der Elektronik geeignete H"utte samt elektrischer Versorgung bei dem +Teleskop. Zur Minimierung von Peronalkosten soll das Teleskop nach der +Aufbauphase weitestgehend robotisch "uber das Internet / einen Link +"uber den ESA-Satelltien XYZ betrieben werden. Die mit DWARF +vorgenommenen Messungen dienen der Kl"arung der Frage nach der +zeitlichen Variabilit"at der Gamma-Emissionen von Aktiven Galaxien und +den zugrundeliegenden Beschelunigungsmechanismen der kosmsichen +Strahlung.\\ + +\loi\\ +\textbf{Abstract:} We propose to set up a Cherenkov telescope with +low-cost but high performance design for robotic operation. The goal is +to achieve long-term monitoring of bright blazars which will unravel +the origin and nature of their variability. The telescope design is +based on a technological upgrade of one of the former telescopes of the +HEGRA collaboration on the Canarian Island La Palma (Spain). \\ + +\textbf{Introduction:} Since the termination of the HEGRA observations, +the succeeding experiments MAGIC and H.E.S.S.\ have impressively extended +the physical scope of gamma ray observations by detecting tens of +formerly unknown gamma ray sources and analyzing their energy spectra +and temporal behavior. This became possible by lowering the energy +threshold from 700 GeV to less than 100 GeV and increasing at the same +time the sensitivity by a factor of five.\\ To fully exploit the +discovery potential of the improved sensitivity, the discovery of new, +faint objects has become the major task for the new telescopes. A +diversity of astrophysical source types such as pulsar wind nebulae, +supernova remnants, microquasars, pulsars, radio galaxies, clusters of +galaxies, gamma ray bursts, and blazers can be studied with these +telescopes and limits their availability for monitoring purposes of +well-known bright sources.\\ There are strong reasons to make an effort +for the continuous monitoring of the few exceptionally bright blazars. +This can be achieved by operating a dedicated monitoring telescope of +the HEGRA-type, referred to in the following as DWARF (Dedicated +multiWavelength Agn Research Facility). The reasons are outlined in +detail below. + +\clearpage + +\section{Stand der Forschung, eigene Vorarbeiten\\State of the art, preliminary work by proposer} + +\subsection{Stand der Forschung/State of the art} + +\subsubsection{High energy gamma and neutrino sources} + +%============================================================ +%Der TeV-Photon-Astronomie ist es in den letzten Jahrzehnten gelungen, {\bf 14} +%extragalaktische und {\bf ???} galaktische Objekte am Himmel zu +%identifizieren. Hinzu kommt die Detektion von zwei diffusen Regionen in der +%Galaxie, die von H.E.S.S. {\bf ZITAT!} und Milagro {\bf ZITAT!!!} gesehen +%wurden. Die erste Quelle wurde im Jahr {\bf 19??} von {\bf HEGRA ???} +%beobachtet. Im Vergleich zu R\"ontgen-Messungen, die den Himmel nach Quellen +%abscannen k\"onnen und dementsprechend mehr als {\bf 1000 ???} Quellen +%katalogisiert haben {\bf ZITAT KATALOG XMM Newton/Chandra}, scheint diese +%Anzahl jedoch sehr niedrig. Ein Grund ist das kleine Sichtfeld, was +%Luft-Cherenkov Teleskope besitzen, ein weiterer, dass das TeV-Photon Signal weit entfernter Quellen +%($z>0.2$) vom extragalaktischen Hintegrundlicht absorbiert wird. +%Aufgrund der geringen Statistik an Quellen ist es zu diesem Zeitpunkt ist es notwendig, dass sich hochsensitive Instrumente +%prim"ar auf die Untersuchung neuer Objekte am TeV-Photon-Himmel konzentrieren +%und nicht auf die quantitative, permanente Beobachtung von schon bekannten +%Quellen. Selbst wenn eine Quelle "uber einen l"angeren Zeitraum beobachtet +%wurde, handelt es sich hier um einen Zeitraum von {\bf $<3$~Monaten ????}. In +%dieser Zeit fallen jedoch sowohl Schlechtwetter-Perioden wie auch Phasen mit +%starker Mond-Einstrahlung weg. Au{\ss}erdem muss beachtet werden, dass die +%Quelle nur eine geringe Anzahl an Stunden sichtbar am Himmel ist. + +The TeV photon astronomy succeeded in discovering {\bf 14} +extragalactic and {\bf ???} galactic objects at the sky during the past +decades. Additionally there are two diffuse regions within our galaxy +which have been detected by H.E.S.S.\ref{Aharonian:2006} and Milagro {\bf +ZITAT!!!} {\it Neues Millagro Papier mit 4+ Quellregionen: "TeV +Gamma-Ray Sources from a Survey of the Galactic Plane with Milagro" +Arxiv-Nr.: 0705.0707} The first source was discovered in the year +19{\bf??} by the {\bf HEGRA} collaboration {\it (War das nicht wer +anders, die zu allererst den Crab sahen?...ZITAT?)}. In comparison to +x-ray measurments, which are able to scan the entire sky for sources +and thus have cataloged more than {\bf 1000 ???} sources, this number +appears to be quite small. One reason for this is the small field of +view of imaging air cherenkov telesopes (IACTs), another reason the +absorption of the TeV photon signal of distant ($z>0.2$) sources due to +extragalactic background light (EBL). Due to this small statistic at +the moment it is of particular importance that instruments with high +sensitivity concentrate on the analysis of new objects in the TeV sky +and not on the quantitative, permanent observation of already known +sources. Even when a source was observed over a longer period of time +this does mean {\bf less than three month ???? {\it Viel l"anger sind +die Quellen am St"uck doch gar nicht sichtbar, oder? Sinnvoller w"are es +wom"oglich die wenigen Beobachtungsstunden in diesen X Monaten +hervorzuheben.}} But one has to take into account that during this time +also periods of bad weather and times with strong moon light can +significantly reduce observation time. Furthermore on has to consider +that the sources are visible in the sky for few hours only. {\it Kann +man das wirklich so sagen?} + +%Bei den bisher beobachteten galaktischen Objekten handelt es sich um +%Mikroquasare und Supernova \"Uberreste, die identifizierten extragalaktischen +%Objekte sind Aktive Galaxien (AGN). Die Objekte sind in Tabelle~\ref{tev_objects} +%aufgelistet {\bf TESHIMAS VORTRAG IN MADISON}. Bei den AGN handelt es sich um +%13 BLLacs und um eine FR-I Galaxie, M87. + +The so far observed galactic objects are microqasars and supernova +remnands (SNR). The identified extragalactic sources are active +galactic nuclei (AGN). The objects are listed in table~\ref{dummy} {\bf +TESHIMAS VORTRAG IN MADISON}. The AGN are 13 BLLacs and one FR-I +galaxy, M87. So High-peaked BL Lacertae objects are the prime source +population for studies with Cherenkov telescopes. It is obvious that +monitoring observations of strong blazars are orthogonal to the mission +of the larger Cherenkov telescopes with their discovery potential for +new sources (luminosity function, redshift distribution). + +\begin{table}[c] +\label{dummy} +\end{table} + +%Im Falle von hadronischer Teilchenbeschleunigung in den TeV Quellen, kann das +%TeV Signal von $\pi^0$-Zerf"allen herr"uhren. Die neutralen Pionen kommen +%von Delta-Resonanz Zerf"allen, die durch Proton-Photon Wechselwirkungen +%entstehen. Ein weiterer Kanal im Zerfall der Delta-Resonanz f"uhrt zur +%Produktion von geladenen Pionen und damit zur Produktion von Neutrinos in +%koinzidenz mit TeV Photonen. Daher sind TeV Quellen auch immer interessant +%f"ur Hochenergie-Neutrinoteleskope. + +In case of hadronic particle acceleration within the TeV emitters, the +TeV signal may arise from $\pi^0$-decays. These neutral pions are decay +products of of delta resonances, which are formed in proton-photon +interactions. Anther decay channel of the delta resonance leads to the +production of charged pions and thus to neutrino production, coincident +with the TeV photons mentioned before. Therefrom TeV sources are always +interesting objects for investigations with high energy neutrino +telescopes. + +%Die hohe Variabilit"at in der zeitlichen Entwicklung der AGN +%TeV-Photon-Spektren kann bisher noch nicht schl"ussig erkl"art +%werden +The strong variability in the temporal evolution of the AGN TeV photon +spectra cannot be explained conclusively yet, + +{\it .... blabla quantitative Untersuchungen, d.h. +Langzeituntersuchungen notwendig.} + +{\bf SENSITIVIT\"ATSPLOT}\\ +{\bf TABELLE QUELLEN}\\ +{\bf AGN Physik kann man nicht ohne die unteren Paragraphen erkl"aren}\\ +{\it Die Frage ist, ob man galaktische Quellen mit in die +Langzeit-Beobachtung nehmen will, dann mu"s man das einzeln +durchgehen. Ich bau die Argumentation gerade nur auf AGN auf:} + +\begin{itemize} +\item Welche Quellen wurden oberhalb von 1 TeV bislang beobachtet? +\item Welche Sensitivit"at braucht man? +\item Warum braucht man Langzeitbeobachtungen? +\item Warum stehen diese Beobachtungen nicht auf der Speisekarte der +gro"sen neuen Telekope? +\end{itemize} + +\paragraph{Physikalische Modelle} +Erkl"are die verschiedenen Szenarien: +\begin{itemize} +\item Inverse Compton +\item Proton Synchrotron +\item Pion decay +\end{itemize} + +Unterschiede darstellen: Pion bump ist nicht so Spitz; Inverse Compton: +wenn man den 2. bump erh"oht, erh"oht sich automatisch auch der +erste; oft widerspruch zu den Daten. Ich glaube, Proton Synchrotron hat +das Problem nicht so, und auch Pion Zerfall nat"urlich nicht. + +Au"serdem: Stand der Dinge, um die Variabilit"at zu erkl"aren + +\paragraph{Ergebnisse von Multiwavelangth-Kampangen} +{\it hier m"ussen die verschiedenen Szenarien - inverse Compton von +elektronen/ proton Synchrotron und Pion-Zerf"alle an Einzelf"allen +diskutiert werden. Es gibt Bsp., bei denen Inverse Compton sehr gut +klappt; dann gibt's welche, wo das gar nicht hinhaut. Einen Fall +gibt's, wo Integral-Daten "uberhaupt nicht ins Bild passen. Da gibts +z.B. ein Papier von Aharonian zu auf astro-ph - irgendwann aus den +letzten 3 Monaten.} + +Experimente erw"ahnen: EGRET, COMPTEL, Integral, H.E.S.S., MAGIC, wer +noch??? f"ur bisherige Spektren; GLAST zum F"ullen der L"ucke!!! + +Auch hier: Diskussion der Variabilit"at; ``Orphan Flares''... + +\paragraph{Die Photon-Neutrino-Verbindung} +BLABLA-\\ + +\textbf{The science case:} The variability of blazars, seen across the +entire electromagnetic spectrum, arises from the dynamics of +relativistic jets and the particle acceleration going on in them. The +jets are launched from the vicinity of accreting supermassive black +holes, and theoretical models predict variability arising from the +interplay between jet expansion, particle injection, acceleration and +cooling.\\ + +Long-term monitor observations of bright blazars are the key to obtain +a solid data base for variability investigations. + +\subsection{Eigene Vorarbeiten/Preliminary work by proposer} + +\subsubsection{Quellphysik} + +\subsubsection{Beteiligung an Experimenten} + +\paragraph{MAGIC} + +\paragraph{IceCube} + +\loi\\ + +The Dortmund group is IceCube member and working since years on +phenomenological calculations and data analysis of possible +coincidences between VHE-gamma and neutrino-emission. \\ + +The available automatic analysis package developed by the W"urzburg +group for MAGIC is modular and flexible, and can thus be used with +minor changes for the DWARF project.\\ + +Ring-Methode f"ur wobble-modus aus W"urzburg? + +Monte Carlo production and storage will take place at Universit"at +Dortmund Monte-Carlo-Erfahrung Dortmund $\to$ Marijkes Diplomarbeit + +A microcontroller based motion control unit (SPS) similar to the one of +the current MAGIC II drive system will be used.\\ +$\to$DriveSystem-Erfahrung W"urzburg + +To correct for axis misalignments and possible deformations of the +structure (e.g. bending of camera holding masts) a pointing correction +algorithm as used in the MAGIC tracking system will be applied. It is +calibrated by measurement of the reflection of bright guide stars on +the camera surface and ensures a pointing accuracy well below the pixel +diameter. \\ $\to$ Diplomarbeit Benjamin Riegel (W"urzburg) + +\section{Ziele und Arbeitsprogramm\\Goals and work schedule} + +\subsection{Ziele/Goals} + +%Der vorliegende Antrag zielt darauf, das ehemalige CT3 der +%HEGRA-Kollaboration auf dem Roque de los Muchachos mit verg"o"serter +%Speiegelfl"ache und neuer Kamera und Datennahme unter dem Namen DWARF +%wieder in Betrieb zu nehmen. Die Sensitivit"at dieses neuen Instrumentes +%wird damit im Energiebereich oberhalb von 500 GeV etwa der des ebenfalls +%stillgelegten Whipple-Teleskopes entsprechen. + +The present application aims at putting the former CT3 of the HEGRA +collaboration on the Roque de los Muchachos back into operation - with +an enlarged mirror surface and a new camera and data taking, under the +name of DWARF. The sensitivity above 500\,GeV of this new instrument +will thus correspond with the one of the also disused Whipple +telescope. + +%Der Aufbau des Teleskopes soll in dem Sinn modular erfolgen, dass Komponenten +%zuk"unftiger Teleskope (Spiegel, Kamera, DAQ) ggf. an diesem Aufbau getestet +%und optimiert werden k"onnen. + +\noindent The layout of the telescope shall be carried out modular in +such a sense that components of future telescopes (mirror, camera, DAQ) +can be tested and optimized at this bodywork. + +%Wissenschaftlich sollen folgende Punkte realisiert werden: +\noindent Scientifically the following aims shall be realized: + +\begin{itemize} +%\item[(1)] Langzeitbeobachtungen zeitlicher Variationen von TeV-Gamma-Ray-Quellen.\\ +\item[(1)] Long-term observations of temporal variations of TeV gamma +ray sources.\\ +An understanding of this variability will deepen our knowledge about + \begin{itemize} + \item the composition and generation of the jets, intimately connected +to the physics of the ergosphere of rapidly spinning black holes +embedded into the hot plasma from the accretion flow. + \item the plasma physics responsible for highly efficient particle +acceleration, bearing similarities to plasma physics of the interaction +between extremely intense laser beams and matter. + \item the orbital modulation of jets due to binary black holes +expected from galaxy merger models.\\ the search for signatures of +binary black hole systems from orbital modulation of VHE gamma ray +emission + \end{itemize} +Long-term monitor observations of bright blazars are the key to obtain +a solid data base for variability investigations. Assuming +conservatively the performance of a single HEGRA-type telescope, +long-term monitoring of at least the following blazars is possible: +Mrk421, Mrk501, 1ES 2344+514, 1ES 1959+650, H 1426+428, PKS 2155-304. +We emphasize that DWARF will run as a facility dedicated to these +targets only, providing a maximum observation time for the program. +\textbf{\textit{oder ist dieser Abschnitt doch besser in 3.2. +aufgehoben?!}} +\item[(2)] Coincident observations with gamma telescopes in different +energy ranges:\\ Flux variations will be determined and compared with +variability properties in other wavelength ranges. +\item[(3)] Coincident observations with the neutrino telescope +IceCube:\\ Hadronic emission processes and possible coincidences +between VHE-gamma and neutrino-emission will be studied. +\item [(5)] Furthermore, we seek to obtain know-how for the operation +of future networks of Cherenkov telescopes (e.g. a monitoring array +around the globe or CTA) or telescopes at inaccessible sites. +\end {itemize} + +\subsection{Arbeitsprogramm/Work schedule}\anmerk{3.2 soll etwa die +H"alfte des Antrages ausmachen} + +\loi\\ + +At least one of the proposed targets will be visible any time of the +year (see plot/appendix). For calibration purposes, some time will be +scheduled for observations of the Crab nebula, which is the brightest +known VHE emitter with constant flux.\\ + +In detail the following investigations are planned: +\begin{itemize} +\item As direct result of the measurements, the duty cycle, the +baseline emission, and the power spectrum of flux variations will be +determined and compared with variability properties in other wavelength +ranges. +\item The lightcurves will be interpreted using models for the +nonthermal emission from relativistically expanding plasma jets. In +particular models currently developed in the context of the Research +Training Group "Theoretical Astrophysics" in W"urzburg +(Graduiertenkolleg, GK1147) shall be used. Particle acceleration is +studied with hybrid MHD and particle-in-cell methods. +\item The black hole mass and accretion rate will be determined from +the emission models. Estimates of the black hole mass from emission +models, a possible orbital modulation, and the Magorrian relation +(relating the black hole mass with the stellar bulge mass of the host +galaxy) will be compared. +\item When flaring states will be discovered during the monitor +program, MAGIC will issue a Target of Opportunity observation to obtain +better time resolution (Letters of support?). Corresponding +Target-of-Opportunity (ToO) proposals to H.E.S.S.\ and Veritas are in +preparation. +\item Correlating the arrival times of neutrinos detected by the +neutrino telescope IceCube with simultaneous measurements of DWARF will +allow to test the hypothesis that flares in blazar jets are connected +to hadronic emission processes and thus to neutrino emission from these +sources. The investigation proposed here is complete for both, neutrino +and gamma observations, and can therefore lead to conclusive results. +\item The diffusive fluxes of escaping UHE cosmic rays obtained from +AUGER or flux limits of neutrinos from IceCube, respectively, will be +used to constrain models of UHE cosmic ray origin and large-scale +magnetic fields. +\item Multi-frequency observations together with the Mets"ahovi Radio +Observatory and the optical Tuorla Observatory are planned (Letters of +support appendix). The measurements will be correlated with INTEGRAL +and GLAST results, when available. X-ray monitoring using the SWIFT and +Suzaku facilities will be proposed. +\item The most ambitious scientific goal of this proposal is the search +for signatures of binary black hole systems from orbital modulation of +VHE gamma ray emission. In case of a confirmation of the present hints +in the temporal behaviour of Mrk501, gravitational wave templates could +be computed with high accuracy to establish their discovery with LISA +(PhD project at W"urzburg funded by the German LISA consortium). +\end{itemize} + +\textbf{The technical setup:} At the Observatorio de los Muchachos +(ORM), at the MAGIC site, the mount of the former HEGRA telescope CT3 +now owned by the MAGIC collaboration is still operational. One hut for +electronics close to the telescope is available. Additional space is +available in the MAGIC counting house. The MAGIC Memorandum of +Understanding allows for operating it as an auxiliary instrument, and +basic support from the shift crew of MAGIC is guaranteed, although +robotic operation is the primary goal. Robotic operation is necessary +to reduce costs and man power demands. Furthermore, we seek to obtain +know-how for the operation of future networks of Cherenkov telescopes +(e.g. a monitoring array around the globe or CTA) or telescopes at +inaccessible sites. From the experience with the construction and +operation of MAGIC or HEGRA, respectively, the proposing groups +consider the planned focused approach (small number of experienced +scientists) as optimal for achieving the project goals. The available +automatic analysis package developed by the W"urzburg group for MAGIC +is modular and flexible, and can thus be used with minor changes for +the DWARF project. Therefore construction, commissioning and operation +of a small scale Cherenkov telescope are best suitable for education +and training of students by experienced scientists. + +To complete the mount to a functional Cherenkov telescope within a +period of one year, the following steps are necessary: + +Camera: +For long-term observations stability of the camera is a major +criterion. To keep the systematic errors small good background +estimation is mandatory. The only possibility for a synchronous +determination of the background is the determination from the night-sky +observed in the same field-of-view with the same instrument. To achieve +this the observed position is moved out of the camera center which +allows the estimation of the background from positions symmetric with +respect to the camera center (so called wobble-mode). This observation +mode increases the sensitivity by a factor of two because spending +observation for dedicated background observations becomes obsolete, +which also ensures a better time coverage of the observed sources. +Having a camera large enough allowing more than one independent +position for background estimation increases sensitivity further by +better background statistics. This is the case if the source can be +shifted 0.6deg-0.7deg out of the camera center. A camera completely +containing shower images of events in the energy region of 1TeV-10TeV +should have a diameter in the order of 5 deg. To decrease the +dependence of the background measurement on the camera geometry, a +camera layout as symmetric as possible will be chosen. Consequently a +camera allowing for wobble-mode observations should be round and have a +diameter of 4.5deg-5.0deg. + +To achieve this requirements a 313 Pixel camera (see figure +\ref{camDWARF}) will been build based on the experience with HEGRA and +MAGIC. 19 mm diameter Photomultiplier Tubes (PM, EMI 4035) will be +bought, similar to the HEGRA type (EMI\,9083\,KFLA). With a 20$\%$ +improved quantum efficiency they ensure a granularity which is enough +to guarantee good results even below the energy threshold (flux peak +energy). Each individual pixel has to be equipped with a preamplifier, +an active high-voltage supply and control. The total expense for a +single pixel will be in the order of 600 EURO. + +If development of G-APDs (QE$\ge$50$\%$) will be fast enough, +respectively the price low enough, and their long term stability is +proven well in time, their usage will be considered. + +For a transition time one of the old HEGRA cameras might be borrowed +(see figure \ref{camCT3}). With a special coating (wavelength shifter) +its quantum efficiency might be improved by ~8$\%$\ref{Paneque:2004}. + +Camera support: +The camera chassis must be water tight. An automatic lid protecting the +PMs at day-time will be installed. For further protection a plexi-glass +window will be installed in the front of the camera. By over-coating +the window with an anti-reflex layer of magnesium-fluoride a gain in +transmission of 5$\%$ is expected. Each PM will be equipped with a +light-guide (Winston Cone) as developed by UC Davis and successfully in +operation in the MAGIC camera. (3000 EURO). The current design will be +improved by using a high reflectivity aluminized Mylar mirror-foil, +overcoated with a dialectical layer (SiO2 alternated with Niobium +Oxide), to reach a reflectivity in the order of 98$\%$. In total this +will gain ~15$\%$ in light-collection efficiency compared to the old +CT3 system. + +For this setup the camera holding has to be redesigned. (1500EURO?) + +An electric and optical shielding of the individual PMs is planned. + +The mechanical work is done at Universit"at Dortmund. + +Data acquisition: +For the data acquisition system a hardware readout based on an analog +ring buffer (Domino II/III), currently developed for the MAGIC II +readout, will be used. This technology allows sampling the pulses with +high frequencies and allows to readout several channels with a single +Flash-ADC resulting in low-costs. The low power consumption will allow +including the digitization near the signal source which makes an analog +signal transfer obsolete. The advantage is less pick-up noise and less +signal dispersion. By high sampling rates (0.5\,GHz-1.2\,GHz) additional +information about the pulse shape can be obtained. This increasing the +over-all sensitivity further, because the short integration time allows +for almost perfect suppression of noise due to night-sky background +photons. The estimated trigger- (readout-) rate of the telescope is +below 100\,Hz (HEGRA: $<$10\,Hz) which allows to use a low-cost industrial +solution for readout of the system like USB\,2.0. (30.000-45.000: +95-145/channel). + +As for the HEGRA telescopes a simple multiplicity trigger is enough, +but also a simple three-next-neighbors (closed package) could be +programmed. ($<$30.000: $<$100/channel). + +To guarantee a homogenous trigger setup over the whole camera the +individual pixel rates, dominated by night-sky noise, will be monitored +and kept constant. + +Additional data reduction and preprocessing in the readout hardware or +the readout computer is provided. Assuming conservatively storage of +raw-data at a readout rate of 30\,Hz the storage space needed is less +than 250\,GB/month or 3\,TB/year. This amount of data can easily be stored +and processed by the W"urzburg Datacenter (current online capacity +$>$20\,TB, offline capacity $>$30\,TB, $>$16\,CPUs). To archive the data +safely 25 tapes (LTO3 with 400\,GB each, $\sim$1000\,EURO) and a SATA +disk-array ($\sim$4000EURO) will be bought. + +On-site computing: +For on-site computing less than three standard PCs are needed +($\sim$8.000EURO). This includes readout and storage, preprocessing, +and telescope control. For safety reasons a firewall is mandatory. For +local storage and backup two RAID\,5 SATA disk arrays with less than one +Terabyte capacity each will fulfill the requirement ($\sim$4.000EURO). +The data will be transmitted as soon as possible after data taking via +Internet to the W"urzburg Datacenter. + +Monte Carlo production and storage will take place at Universit"at +Dortmund + +For the absolute time necessary for an accurate source tracking a GPS +clock will be bought. + +Mount and Drive: +The present mount is used. Only a smaller investment for safety, +corrosion protection, cable ducts, etc. is needed (7.500). + +For movement motors, shaft encoders and control electronics in the +order of 10.000 EURO have to be bought. The drive system should allow +for relatively fast repositioning for three reasons: 1) Fast movement +might be mandatory for future ToO observations. 2) Wobble-mode +observations will be done changing the wobble-position continuously +(each 20\,min) for symmetry reasons. 3) To ensure good time coverage of +more than one source visible at the same the observed source will be +changed in constant time intervals ($\sim$20\,min). Therefore three 150 +Watt servo motors are intended. A microcontroller based motion control +unit (SPS) similar to the one of the current MAGIC II drive system will +be used. For communication with the readout-system a standard Ethernet +connection based on the TCP/IP- and UDP-protocol is applied. + +Security: +An uninterruptible power-supply unit (UPS) with 5-10\,kW will be +installed to protect the equipment against power cuts and ensure a safe +telescope position at the time of sun-rise. ($<$2000EURO) + +Mirrors: +The existing mirrors are replaced by new plastic mirrors which are +currently developed by the group of Wolfgang Dr"oge. The cheap and +light-weight material has been formerly used for Winston cones flown in +balloon experiments. The mirrors are copied from a master, coated with +a reflecting and a protective material. Previous tests have given +promising results. By a change of the mirror geometry the mirror area +can be increased from 8.5\,m$^2$ to 13\,m$^2$ (see picture \ref{CT3} and +montage \ref{DWARF}); this includes an increase of $\sim$10$\%$ per +mirror by using a hexagonal layout. A further increase of the mirror +area would require a reconstruction of parts of the mount and will +therefore be considered only in later phase of the experiment. + +If the current development cannot be finished in time a re-machining of +the old glass mirrors (8.5\,m$^2$) is possible with high purity aluminum +and quartz coating. (Both cases: 30 mirrors, 10k, offer by L-Tec +$\lesssim$500 EURO / mirror *30 mirrors = 15.000 EURO without transfer) + +To keep track of the alignment, reflectivity and optical +quality of the individual mirrors, and the point-spread function of the +total mirror, during long-term observations the application of an +automatic mirror adjustment system, as developed by ETH Z"urich and +successfully operated on the MAGIC telescope, is intended. The system +will be provided by ETH Z"urich. (1.000 EURO/pannel) + +For a 3.5\,m diameter mirror the delay between an isochronous parabolic +mirror and a spherical mirror at the edge is in the order of 1ns (see +figure/appendix). For a sampling rate in the order of 1\,GHz a mirror +mounting with a parabolic shape in needed. Since their small size the +individual mirrors can still have a spherical shape. + +Telescope calibration: + +Tracking: To correct for axis misalignments and possible deformations +of the structure (e.g. bending of camera holding masts) a pointing +correction algorithm as used in the MAGIC tracking system will be +applied. It is calibrated by measurement of the reflection of bright +guide stars on the camera surface and ensures a pointing accuracy well +below the pixel diameter. Therefore a high sensitive low-cost video +camera, as already in operation for MAGIC I and II, (300 EURO camera, +300 EURO optics, 300 EURO housing) will be installed. + +PM Gain: For the calibration of the PM gain a calibration system as +used for the MAGIC telescope is build. (2000 EURO) + +Summarizing, the expenses for the telescope are dominated by the camera +and DAQ. The financial volume for the complete hardware inclusive +transport amounts roughly 400.000 EURO. + +\textbf{Future extensions:} The known duty cycle of 10\% +($\sim$1000h/year) for a Cherenkov telescope operated at La Palma +limits the time-coverage of the observations. Therefore we propose a +worldwide network of ($<$10) small scale Cherenkov telescopes to be +build in the future allowing 24\,h monitoring of the bright AGNs. Such a +system is so far completely unique in this energy range. In a first +stage of the project mounts of other former HEGRA telescopes could be +used operated at locations in Croatia, the United States and Mexico. +For an increased sensitivity and improved energy threshold the use of a +low-cost mount build by the company MERO for solar power generation is +proposed. The mount is based on the experiences with the MAGIC +telescope, also builds by MERO, and has a diameter in the order of +eight meters. Including support (concrete foundation, railways, etc) +the costs are below 100.000EURO + +\subsection{Biologisch, medizinische Experiment} +Untersuchungen an Mensch oder Tier, sowie gentechnische Experimente +werden nicht durchgef"uhrt. + +\newpage + +\begin{figure}[ht] +\centering{ +\includegraphics[width=12cm]{cam271.eps} +\caption{Schematic picture of the 313 pixel camera for DWARF with a field of view of 5$^\circ$.} +\label{camDWARF} +} +\end{figure} + +\begin{figure}[ht] +\centering{ +\includegraphics[width=10.5cm]{cam313.eps} +\caption{Schematic picture of the 271 pixel CT-3 camera with a field of view of 4.6$^\circ$.} +\label{camCT3} +} +\end{figure} + +\begin{figure}[ht] +\centering{ +\includegraphics[width=12cm]{cam313.eps} +\caption{Picture of the HEGRA CT-3 taken at a time when it was still in operation.} +\label{CT3} +} +\end{figure} + +\begin{figure}[ht] +\centering{ +\includegraphics[width=12cm]{cam313.eps} +\caption{Photo montage of DWARF as it will look alike after the mirror replacement.} +\label{DWARF} +} +\end{figure} + +\clearpage +\newpage + +\section{Beantragte Mittel/Funds requested} + +\subsection{Personalbedarf/Required staff} +%Wir beantragen die F"orderung von je einem Postdoc und Doktoranden in +%W"urzburg und Dortmund. +We request funding for two postdocs (BATIIa, 3y) and two Ph.D. students +(BATIIa/2, 3y), one in Dortmund and one in W"urzburg each. + +(im Antrag ist der qualifizierte Einsatz der studentischen Hilfskraefte +darzulegen, KEINE Betr"age angeben!) + +(Bezahlung ab wann?, Kurzer Abriss der Aufgaben, ggf. Namen) + +\anmerk{2 Institute x 3 Jahre x (1 +PD = 60.000 + 1 PhD = 30.000) = 2 x 250.000 = 500.000} + +%Von den Mitarbeitern sollen folgende Aufgaben erf"ullt werden: +The staff members shall fulfill the following tasks: + +\begin{itemize} + +\item Postdoc W"urzburg + +\item Doktorand W"urzbug + +\item Postdoc Dortmund + +\item Doktorand Dortmund + +\end{itemize} + +%Geeignete und ggf. interessierte Kandidaten f"ur Postdocstellen sind... +Suitable candidates interested in these positions are Dr. xxx, Dr. yyy, +Dipl.-Phys. zzz and Dipl.-Phys. www. + +\subsection{Wissenschaftliche Ger"ate/Scientific equipment} + +\begin{itemize} + +\item Camera: 313Pixel*650EURO/Pixel ~ 200.000EURO (204kEURO) + \begin{itemize} + \item Pixel: 650EURO/Pixel + \begin{itemize} + \item 300-350EUROEURO Photomultiplier (EMI 4051) + \item 50EURO Preamplifier + \item 200-250EURO HV control and support (EMI) + \end{itemize} + \item Winston Cones: 3000EURO (?) + \item Camera holding and chassis: 3000EURO(?) + \end{itemize} + +\item Data acquisition: 313channel*245EURO/channel ~ 77.000EURO + \begin{itemize} + \item 145 (95) EURO/channel Readout + \item 100EURO/channel Trigger + \end{itemize} + +\item Calibration System: 9.000EURO + \begin{itemize} + \item 2000EURO Absolute light calibration? + \item IPR control? + \item Weather station 500EURO + \item 1500EURO GPS clock + \item 5.000EURO CD Cameras + readout + \end{itemize} + +\item Mirrors: 15.000EURO + +\item On-site computing: 12.000EURO + \begin{itemize} + \item 3xPC: 8000EURO + \item SATA RAID 3TB: 4000EURO + \end{itemize} + +\item Computing: 4.000EURO + \begin{itemize} + \item 3TB SATA Disk space: 4000EURO(?) + \end{itemize} + +\item AMC: 1000EURO/pannel +\item UPS: 2000EURO +\item 7.500EURO Robotics + +\end{itemize} + +\subsection{Verbrauchsmaterial/Consumables} +Stromrechnung La Palma, wie hoch pro Jahr? + +\begin{itemize} + \item operation costs: 5000EURO/3years + \item 25 LTO3 Tapes: 1000EURO + \item 10.000EURO Consumables +\end{itemize} + +\subsection{Reisen/Travel expenses} +\begin{itemize} + \item 35.000EURO Travel and construction +\end{itemize} + +\subsection{Publikationskosten/Publication costs} +%keine +none + +\subsection {Sonstige Kosten} +%keine\\ +\begin{itemize} + \item 5.000EURO transport and storage container + \item Dismantling (0, will be covered by proposing institutes) + \item 15.000EURO Transport +\end{itemize} + +\section{Voraussetzungen f"ur die Durchf"uhrung des Vorhabens\\Preconditions for carrying out the project} +%Vor Durchf"uhrung ist die Zustimmung der Magic-Kollaboration und des +%IAC einzuholen. Nach Vorgespr"achen ist von der Erteilung dieser +%Zustimmung auszugehen. + +Before realization the consent of the Magic collaboration and the IAC +is required. According to preliminary talks this consent is expected to +be given. + +\subsection{Zusammensetzung der Arbeitsgruppe/The research team} + +\noindent {\bf Dortmund}: + +\begin{itemize} +\item Prof. Dr. Dr. Wolfgang Rhode (Grundausttattung) +\item Dr. Tanja Kneiske (Postdoc (Ph"anomenologie), Forschungsstipendium) +\item Dr. Julia Becker (Postdoc (Ph"anomenologie), Grundausttattung) +\item Dipl.-Phys. Jens Dreyer (Doktorand (IceCube), Grundausttattung) +\item Dipl.-Phys Kirsten M"unich (Doktorandin (IceCube), Projekt-finanziert) +\item Dipl.Phys. Marijke Haffke (Doctorandin (MAGIC), XXXXXXXXXXXXXXXXX) +\item M.Sci. Valentin Curtef (Doktorand (MAGIC), Projekt-finanziert) +\item cand. phys. Jan L"unemann (Diplomand (IceCube), zum F\"orderbeginn diplomiert) +\item cand. phys. Dominik Leier (Diplomand (Ph"anomenologie), zum F\"orderbeginn diplomiert) +\item cand. phys. Michael Backes (Diplomand (MAGIC), zum F\"orderbeginn diplomiert) +\item cand. phys. Daniela Hadasch (Diplomandin (MAGIC)) +\item Dipl.-Ing. Kai Warda (Elektronik) +\item PTA Matthias Domke (Systemadministration) +\end{itemize} + +\noindent{\bf W"urzburg}: + +\begin{itemize} +\item Prof. Dr. Karl Mannheim (Grundausttattung) +\item Dipl.-Phys. nn (Grundausstattung) +\item Dipl.-Phys. nn (Fremdfinanziert) +\end{itemize} + +\subsection{Zusammenarbeit mit anderen Wissenschaftlern\\Co-operation with other scientists} + +%Beide antragstellenden Arbeitsgruppen arbeiten in der internationalen +%MAGIC-Kollaboration mit den dort vertretenen Arbeitsgruppen zusammen. +%(W"urzburg gef"ordert vom BMBF, Dortmund z.Zt. mit Berufungsmitteln.)\\ + +Both applying groups co-operate with the international MAGIC-Collaboration +and the institutes represented therein. (W"urzburg funded by the BMBF, Dortmund +by means of appointment for the moment.)\\ +{\bf Dr.~Adrian Biland, Prof.~Dr.~Eckart Lorenz (both ETH Z"urich)}\\ +{\bf Prof.~Riccardo Paoletti (Università di Siena and INFN sez. di Pisa, Italy)}\\ + +%Die Arbeitsgruppe in Dortmund ist an dem IceCube-Experiment beteiligt +%(BMBF-F"orderung) und unterh"alt zu den Kollaborationspartnern enge +%Kontakte. Dar"uber hinaus bestehen auf dem Gebiet der Ph"anomenologie +%gute Arbeitskontakte zu der Gruppe von Prof.~Dr.~Reinhard~Schlickeiser, +%Ruhr-Universit"at Bochum und Prof.~Dr.~Peter~Biermann, MPIfR +%Bonn. Weitere Kontakte bestehen zu Dr.~Anita Reimer, Stanford (USA) und +%Prof.~Dr.~Ray~Protheroe, Adelaide (Australien).\\ + +\noindent The group in Dortmund is involved in the IceCube experiment +(BMBF funding) and maintains close contacts to the collaboration +partners. Moreover on the field of phenomenology there do exist good +working contacts to the groups of Prof.~Dr.~Reinhard~Schlickeiser, +Ruhr-Universit"at Bochum and Prof.~Dr.~Peter~Biermann, MPIfR Bonn. +There are furthermore contacts to Dr.~Anita Reimer, Stanford (USA) and +Prof.~Dr.~Ray~Protheroe, Adelaide (Australien).\\ {\bf Francis Halzen, +evtl. John Quenby}\\ + +\noindent W"urzburg is involved in ... maintains contacts to ...\\ +Prof.~Dr.~Wolfgang Dr\"oge\\ + +\subsection{Arbeiten im Ausland, Kooperation mit Partnern im Ausland\\Work outside Germany, Cooperation with foreign partners} +%Die Arbeiten an DWARF werden auf dem ORM der Spanischen Insel La Palma und in +%enger Zusammenarbeit mit der MAGIC-Kollaboration ausgef"uhrt. + +The work on DWARF will take place at the ORM on the Spanish island La +Palma. It will be performed in close collaboration with the +MAGIC-collaboration. + +\subsection{Apparative Ausstattung/Scientific equipment available} +%Sowohl in W"urzburg als auch in Dortmund stehen umfangreiche +%Rechnerkapazi"aten zur Datenspeicherung und -analyse zur Verf"ugung.\\ +Both in Dortmund and in W"urzburg there are extensive computer +capacities available for data storing as well as for data analysis. + +%Dortmund: Der Fachbereich Physik der Universit"at Dortmund verf"ugt "uber +%modern ausgestattete mechanische und elektronische Werkst"atten +%einschlie"slich einer Elektronik-Entwicklung. Der Lehrstuhlbereich +%Astroteilchenphysik verf"ugt "uber g"angige zur Erstellung moderner +%DAQ erforderliche apparative Ausstattung.\\ +Dortmund: The Fachbereich Physik at the Universit"at Dortmund has +modern equipped mechanical and electrical workshops including a +department for development of electronics at its command. The +Lehrstuhlbereich Astroteilchenphysik possesses common technical +equipment required for constructing modern DAQ. + +W"urzburg:... + +\subsection{Laufende Mittel f"ur Sachausgaben\\The institution's general contribution} + +%Das gegenw"artige Budget des Lehrstuhls f"ur Astronomie der Universit"at +%W"urzburg betr"agt $\approx $ 12345 EURO pro Jahr.\\ +%Das gegenw"artige Budget des Lehrstuhlbereiches Astroteilchnphysik der +%Universit"at Dortmund betr"agt $\approx $ 20000 EURO pro Jahr. +Current total institute budget from the Universit"at Dortmund $\approx$ +20000 EURO per year.\\ + +Current total institute budget from the Universit"at W"urzburg +$\approx$ xxxxx EURO per year.\\ + +\subsection{Sonstige Voraussetzungen/Other requirements} +%keine +none + +\subsection{Interessenskonflikte bei wirtschaftlichen Aktivit"aten\\Conflicts of interest in economic activities} +%keine +none + +\section{Erkl"arungen/Declarations} +\noindent +%{\bf 6.1} Ein Antrag auf Finanzierung dieses Vorhabens wurde bei +%keiner anderen Stelle eingereicht. Im Falle eines solchen Antrages +%wird die Deutsche Forschungsgemeinschaft von uns unverz"uglich +% benachrichtigt. +{\bf 6.1} A request for funding this project has not been submitted to +any other addressee. In case we submit such a request we will inform +the Deutsche Forschungsgemeinschaft immediately. + +\noindent +%{\bf 6.2} Die Vertrauensdozenten an der Universit"at W"urzbug +%(Prof. XXXX) und an der Universit"at Dortmund (Prof. Dr. Gather ) sind +%von der Antragstellung unterrichtet worden. +{\bf 6.2} The corresponding persons (Vertrauensdozenten) at the +Universit"at Dortmund (Prof. Dr. Gather) and at the Universit"at +W"urzburg (Prof. XXXXX) have been informed about the submission of this +proposal. + +\noindent +%{\bf 6.3} entf"allt +{\bf 6.3} N/A + + +\newpage +\section{Unterschriften/Signatures} + +\vspace{1 cm} +\noindent +01. 06. 2007 \hspace{4cm} Prof. Dr. Dr. Wolfgang Rhode + +\vspace{3 cm} +\noindent +01. 06. 2007 \hspace{4cm} Prof. Dr. Karl Mannheim +\clearpage + +\section*{Verzeichnis der Anlagen/List of appendages} + +\begin{itemize} +\item +%Schriftenverzeichnis der Antragsteller seit dem Jahr 2000 +List of refereed publications of the applicants since 2000 +\item +CV of Karl Mannheim +\item +CV of Wolfgang Rhode +\end{itemize} + +\newpage +%\section{References} + +\vskip0.3cm + +%\bibliographystyle{alpha} +\newpage +%(Referenzen aus unseren Gruppen sind mit einem Stern gekennzeichnet *) +(References of our groups are marked by an asterix *) +\bibliography{application} +%This in the bibtex style, is ok. +\bibliographystyle{plain} +References will be added in the final version. +%\begin{thebibliography}{99} +%\bibitem{andreas_05} *M.~Ackermann et al., ''On the selection of AGN neutrino +% source candidates $\ldots$'', submitted to {\app} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%\end{thebibliography} + +\end{document} Index: /trunk/Dwarf/Documents/ApplicationDFG/cam271.eps =================================================================== --- /trunk/Dwarf/Documents/ApplicationDFG/cam271.eps (revision 8596) +++ /trunk/Dwarf/Documents/ApplicationDFG/cam271.eps (revision 8596) @@ -0,0 +1,250 @@ +%!PS-Adobe-2.0 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/arrowdbldown 119 /ampersand 120 /omega1 121 /similar 122 /aleph ] def +/Symbol /Special accspe ReEncode +%%EndProlog +%%BeginSetup +%%EndSetup +newpath gsave .25 .25 scale gsave 0 0 t black[ ] 0 sd 3 lw 1 1 1 c 1990 1989 139 0 bf black 1 1 1 c 1990 1989 139 0 bf black 0.95 0.95 0.95 c black 239 99 m 298 X s 497 122 m 40 -23 d -40 -22 d s 0.95 0.95 0.95 c black 239 99 m 299 Y s 216 358 + m 23 40 d 22 -40 d s + gsave 288 149 + t 0 r 0 0 m /Helvetica-Bold findfont 73.04 sf 0 0 m (67mm) show gr + gsave 424 250 + t 0 r 0 0 m /Symbol findfont 73.04 sf 0 0 m (°) show gr + gsave 285 250 + t 0 r 0 0 m /Helvetica-Bold findfont 73.04 sf 0 0 m (0.80) show gr 0.999 0.999 0.999 c 1180 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1180 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1274 1022 m + -47 27 d -47 -27 d -54 Y 47 -27 d 47 27 d f black 1274 1022 m -47 27 d -47 -27 d -54 Y 47 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1227 1102 m -47 27 d -46 -27 d 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941 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 + 0.999 c 1553 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1553 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1507 1102 m -47 27 d -47 -27 d -53 Y 47 -27 d 47 27 d f black 1507 1102 m -47 27 d -47 -27 d + -53 Y 47 -27 d 47 27 d 53 Y cl s 0.999 0.999 0.999 c 1460 1183 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d f black 1460 1183 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1413 1264 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 + 27 d f black 1413 1264 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1367 1344 m -47 27 d -46 -27 d -53 Y 46 -27 d 47 27 d f black 1367 1344 m -47 27 d -46 -27 d -53 Y 46 -27 d 47 27 d 53 Y cl s 0.999 0.999 0.999 c 1274 + 1344 m -47 27 d -47 -27 d -53 Y 47 -27 d 47 27 d f black 1274 1344 m -47 27 d -47 -27 d -53 Y 47 -27 d 47 27 d 53 Y cl s 0.999 0.999 0.999 c 1180 1344 m -46 27 d -47 -27 d -53 Y 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m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d f black 1367 699 m + -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1413 780 m -46 26 d -47 -26 d -54 Y 47 -27 d 46 27 d f black 1413 780 m -46 26 d -47 -26 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1460 860 m -47 27 d -46 -27 d + -54 Y 46 -26 d 47 26 d f black 1460 860 m -47 27 d -46 -27 d -54 Y 46 -26 d 47 26 d 54 Y cl s 0.999 0.999 0.999 c 1507 941 m -47 27 d -47 -27 d -54 Y 47 -27 d 47 27 d f black 1507 941 m -47 27 d -47 -27 d -54 Y 47 -27 d 47 27 d 54 Y cl s 0.999 + 0.999 0.999 c 1646 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1646 1022 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1600 1102 m -47 27 d -46 -27 d -53 Y 46 -27 d 47 27 d f black 1600 1102 m -47 27 d -46 + -27 d -53 Y 46 -27 d 47 27 d 53 Y cl s 0.999 0.999 0.999 c 1553 1183 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1553 1183 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 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27 d -46 -27 d -54 Y 46 -27 d 47 27 d 54 Y cl s + 0.999 0.999 0.999 c 1320 618 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1320 618 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1413 618 m -46 27 d -47 -27 d -54 Y 47 -27 d 46 27 d f black 1413 618 m -46 27 d -47 + -27 d -54 Y 47 -27 d 46 27 d 54 Y cl s 0.999 0.999 0.999 c 1460 699 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d f black 1460 699 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1507 780 m -47 26 d -47 -26 d -54 Y 47 -27 d + 47 27 d f black 1507 780 m -47 26 d -47 -26 d -54 Y 47 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1553 860 m -46 27 d -47 -27 d -54 Y 47 -26 d 46 26 d f black 1553 860 m -46 27 d -47 -27 d -54 Y 47 -26 d 46 26 d 54 Y cl s 0.999 0.999 0.999 c 1600 + 941 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d f black 1600 941 m -47 27 d -46 -27 d -54 Y 46 -27 d 47 27 d 54 Y cl s 0.999 0.999 0.999 c 1740 1022 m -47 27 d -47 -27 d -54 Y 47 -27 d 47 27 d f 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[<0D15CD9C9825C6C2EAF6F4C69BC3C346><0D15CD9C9825C6C2EAF6F4C69BC3C346>] +>> +startxref +204445 +%%EOF Index: /trunk/Dwarf/Documents/ApplicationDFG/library.def =================================================================== --- /trunk/Dwarf/Documents/ApplicationDFG/library.def (revision 8596) +++ /trunk/Dwarf/Documents/ApplicationDFG/library.def (revision 8596) @@ -0,0 +1,116 @@ +\def\aj{AJ}% + % Astronomical Journal +\def\actaa{Acta Astron.}% + % Acta Astronomica +\def\araa{ARA\&A}% + % Annual Review of Astron and Astrophys +\def\apj{ApJ}% + % Astrophysical Journal +\def\apjl{ApJ}% + % Astrophysical Journal, Letters +\def\apjs{ApJS}% + % Astrophysical Journal, Supplement +\def\ao{Appl.~Opt.}% + % Applied Optics +\def\apss{Ap\&SS}% + % Astrophysics and Space Science +\def\aap{A\&A}% + % Astronomy and Astrophysics +\def\aapr{A\&A~Rev.}% + % Astronomy and Astrophysics Reviews +\def\aaps{A\&AS}% + % Astronomy and Astrophysics, Supplement +\def\azh{AZh}% + % Astronomicheskii Zhurnal +\def\baas{BAAS}% + % Bulletin of the AAS +\def\bac{Bull. astr. Inst. Czechosl.}% + % Bulletin of the Astronomical Institutes of Czechoslovakia +\def\caa{Chinese Astron. Astrophys.}% + % Chinese Astronomy and Astrophysics +\def\cjaa{Chinese J. Astron. Astrophys.}% + % Chinese Journal of Astronomy and Astrophysics +\def\icarus{Icarus}% + % Icarus +\def\jcap{J. Cosmology Astropart. Phys.}% + % Journal of Cosmology and Astroparticle Physics +\def\jrasc{JRASC}% + % Journal of the RAS of Canada +\def\mnras{MNRAS}% + % Monthly Notices of the RAS +\def\memras{MmRAS}% + % Memoirs of the RAS +\def\na{New A}% + % New Astronomy +\def\nar{New A Rev.}% + % New Astronomy Review +\def\pasa{PASA}% + % Publications of the Astron. Soc. of Australia +\def\pra{Phys.~Rev.~A}% + % Physical Review A: General Physics +\def\prb{Phys.~Rev.~B}% + % Physical Review B: Solid State +\def\prc{Phys.~Rev.~C}% + % Physical Review C +\def\prd{Phys.~Rev.~D}% + % Physical Review D +\def\pre{Phys.~Rev.~E}% + % Physical Review E +\def\prl{Phys.~Rev.~Lett.}% + % Physical Review Letters +\def\pasp{PASP}% + % Publications of the ASP +\def\pasj{PASJ}% + % Publications of the ASJ +\def\qjras{QJRAS}% + % Quarterly Journal of the RAS +\def\rmxaa{Rev. Mexicana Astron. Astrofis.}% + % Revista Mexicana de Astronomia y Astrofisica +\def\skytel{S\&T}% + % Sky and Telescope +\def\solphys{Sol.~Phys.}% + % Solar Physics +\def\sovast{Soviet~Ast.}% + % Soviet Astronomy +\def\ssr{Space~Sci.~Rev.}% + % Space Science Reviews +\def\zap{ZAp}% + % Zeitschrift fuer Astrophysik +\def\nat{Nature}% + % Nature +\def\iaucirc{IAU~Circ.}% + % IAU Cirulars +\def\aplett{Astrophys.~Lett.}% + % Astrophysics Letters +\def\apspr{Astrophys.~Space~Phys.~Res.}% + % Astrophysics Space Physics Research +\def\bain{Bull.~Astron.~Inst.~Netherlands}% + % Bulletin Astronomical Institute of the Netherlands +\def\fcp{Fund.~Cosmic~Phys.}% + % Fundamental Cosmic Physics +\def\gca{Geochim.~Cosmochim.~Acta}% + % Geochimica Cosmochimica Acta +\def\grl{Geophys.~Res.~Lett.}% + % Geophysics Research Letters +\def\jcp{J.~Chem.~Phys.}% + % Journal of Chemical Physics +\def\jgr{J.~Geophys.~Res.}% + % Journal of Geophysics Research +\def\jqsrt{J.~Quant.~Spec.~Radiat.~Transf.}% + % Journal of Quantitiative Spectroscopy and Radiative Trasfer +\def\memsai{Mem.~Soc.~Astron.~Italiana}% + % Mem. Societa Astronomica Italiana +\def\nphysa{Nucl.~Phys.~A}% + % Nuclear Physics A +\def\physrep{Phys.~Rep.}% + % Physics Reports +\def\physscr{Phys.~Scr}% + % Physica Scripta +\def\planss{Planet.~Space~Sci.}% + % Planetary Space Science +\def\procspie{Proc.~SPIE}% + % Proceedings of the SPIE +\let\astap=\aap +\let\apjlett=\apjl +\let\apjsupp=\apjs +\let\applopt=\ao Index: /trunk/Dwarf/Documents/ICRC2007/Makefile =================================================================== --- /trunk/Dwarf/Documents/ICRC2007/Makefile (revision 8596) +++ /trunk/Dwarf/Documents/ICRC2007/Makefile (revision 8596) @@ -0,0 +1,60 @@ +TARGET = icrc0974 + +TARGETLIST = $(TARGET).pdf +INTERMEDIATES = $(TARGET).dvi + +all: $(TARGETLIST) + +OPT = -file-line-error-style -interaction=nonstopmode + +.SILENT: + +define run-latex + @echo " - Producing $@ from" $< + ! (latex $(OPT) $< | grep -E \.tex:[0-9]*:\ ) + bibtex --terse $(<:.tex=) + latex $(OPT) $< > /dev/null + latex $(OPT) $< > /dev/null + ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +# ! (latex $(OPT) $< | grep -E \.tex:[0-9]*:\ ) && \ +# bibtex --terse $(<:.tex=); \ +# cp icrc0974.bbl icrc0974.bbl~ && \ +# sed icrc0974.bbl~ -e 's/^\(.*\)\\url\(.*\)%/\1\\url\2/' > icrc0974.bbl && \ +# (latex $(OPT) $< > /dev/null) && \ +# (latex $(OPT) $< > /dev/null) && \ +# ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +# && \ +# ! (latex $(OPT) $< | grep ^LaTeX\ Warning:\ ) +endef + +%.dvi: %.dtx + $(run-latex) + +%.dvi: %.tex + $(run-latex) + +%.ps: %.dvi + @echo " - Producing $@ from" $< + dvips -q $< $@~ && mv $@~ $@ + +%.pdf: %.dvi + @echo " - Producing $@ from" $< + dvipdf -q $< $@~ && mv $@~ $@ + +%: %.dvi + @echo " - Producing $@.pdf from" $< + dvipdf -q $< + +%.ps.gz: %.ps + @echo " - Producing booklet $@ from" $< + psbook -q $< | psnup -q -2 | pstops -q 2:0,1VH | gzip -c -9 > $@ + +%.bdf: %.ps.gz + @echo " - Producing booklet $@ from" $< + gzip -cd $< | ps2pdf - $@ + +clean: + @rm -f $(INTERMEDIATES) $(TARGETLIST) *.dvi *.aux *.blg *.lof *.log *.lot *.toc *.bbl *.bdf + +mrproper: clean + @rm -f *~ Index: /trunk/Dwarf/Documents/ICRC2007/icrc0974.bib =================================================================== --- /trunk/Dwarf/Documents/ICRC2007/icrc0974.bib (revision 8596) +++ /trunk/Dwarf/Documents/ICRC2007/icrc0974.bib (revision 8596) @@ -0,0 +1,2547 @@ +------------------------------------------------------------------------------ +Article (author, title, journal, year) + (volume, numbe,r pages, month, note) +Book (author/editor, title, publisher, year) + (volume/number, series, address, edition, month, note) +Conference (author, title, booktitle, year) + (editor, volume/number, organization, series, pages, publisher, address, month, note) +Inproceedings (author, title, booktitle, year) + (editor, volume/number, organization, series, pages, publisher, address, month, note) +Manual (title) + (author, organization, address, edition, month, year, note) +Masterthesis (author, title, school, year) + (address, month, note, type) +phdthesis (author, title, school, year) + (address, month, note, type) +unpublished (author, title, note) + (month, year) +misc () + (author, title, howpublished, month, year, note) +------------------------------------------------------------------------------ + +@MISC{www:fornaxa, key = {{www-01}}, title = {\url{http://www.nrao.edu/imagegallery/}}, year=2006, note={Credit: NRAO/AUI/NSF}} +@MISC{www:agnartist0, key = {{www-02}}, title = {\url{http://integral.esa.int/integ_pictures.html}}, year=2006} +@MISC{www:agnartist, key = {{www-03}}, title = {\url{http://www.spacetelescope.org/images/}}, year=2006, note={Credit: ESA/NASA, the AVO Project and Paolo Padovani}} +@MISC{www:compton, key = {{www-04}}, title = {\url{http://chandra.harvard.edu/resources/illustrations/xlightScatter.html}}, year=2006} +@MISC{www:shower, key = {{www-05}}, title = {\url{http://www.mpi-hd.mpg.de/hfm/CosmicRay/shower.png}}, year=2006} +@MISC{www:showerartist, key = {{www-06}}, title = {\url{http://abyss.uoregon.edu/~js/glossary/cosmic_rays.html}}, year=2006} +@MISC{www:mars, key = {{www-07}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/}}, year=2006} +@MISC{www:google, key = {{www-08}}, title = {\url{http://earth.google.com}}, year=2006} +@MISC{www:slalib, key = {{www-09}}, title = {\url{http://star-www.rl.ac.uk/star/docs/sun67.htx/sun67.html}}, year=2006} +@MISC{www:root, key = {{www-10}}, title = {\url{http://root.cern.ch}}, year=2006} +@MISC{www:htmldoc, key = {{www-11}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/htmldoc/}}, year=2006} +@MISC{www:mysql, key = {{www-12}}, title = {\url{http://www.mysql.com}}, year=2006} +@MISC{www:unified, key = {{www-13}}, title = {\url{http://chandra.harvard.edu/resources/illustrations/quasar.html}}, year=2006, note={Credit: NASA/CXC, Melissa Weiss}} +@MISC{www:asdc, key = {{www-14}}, title = {\url{http://www.asdc.asi.it/blazars/}}, year=2006} +@MISC{www:kva, key = {{www-15}}, title = {\url{http://tur3.tur.iac.es/}}, year=2006} +@MISC{www:integral, key = {{www-16}}, title = {\url{http://altamira.asu.cas.cz/iblwg/show.php?id=131}}, year=2006} +@MISC{www:ned, key = {{www-17}}, title = {\url{http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=1es1218+304}}, year=2006} + +%@MISC{www:BH1m, key = {{www-02}}, title = {\url{http://www.gsfc.nasa.gov/gsfc/spacesci/pictures/blackhole/BH1m.jpg}}, year=2006} +%@MISC{www:hillas, key = {{www-10}}, title = {\url{http://lpnhe-auger.in2p3.fr/slides/hillas.ps}}, year=2006} +%@MISC{www:agnartist2, key = {{www-03}}, title = {\url{http://upload.wikimedia.org/wikipedia/en/4/40/Galaxies_AGN_Inner-Structure-of.jpg}}, year=2006} + + +@BOOK{Peebles:1983, + author = {Peebles, Philip~James~Edwin}, + title = {Principles of Physical Cosmology}, + publisher = {Princton Series in Physics}, + year = 1983 +} + +@BOOK{Weekes:2003, + author = {Weekes, T.~C.}, + title = {Very high energy gamma-ray astronomy}, + series = {Astronomy and Astrophysics}, + publisher = {Institute of Physics Publishing}, + year = 2003 +} + +@BOOK{Rybicki:1979, + author = {{Rybicki}, George B. and {Lightman}, Alan P.}, + title = "Radiative Processes in Astrophysics", + publisher = { Wiley-Interscience }, + year = 1979 +} + +@BOOK{Begelman:1995, + author = {Begelman, M. and Rees, M.}, + title = "{Gravity's Fatal Attraction: Black Holes in the Universe}", + year = 1995, +publisher = {Scientific American Library} +} + +@BOOK{Mueller:2005, + author = {{M\"uller}, A.}, + title = "{Lexikon der Astrophysik}", + year = 2005, + month = sep, + url = {http://www.mpe.mpg.de/~amueller} +} + +@BOOK{Zensus:1987, + author = {{Pearson}, T.~J. and {Zensus}, J.~A.}, + year = 1987, + title = {Superluminal radio sources}, + publisher = {Cambridge University Press} +} + +@BOOK{Schlickeiser:2003, + author = {{Schlickeiser}, Reinhard}, + year = 2003, + title = {Cosmic Ray Astrophysics}, + publisher = {Springer} +} + +@BOOK{Landau:1971, + author = {{Landau}, L.~D. and {Lifshitz}, E.~M.}, + title = "{The classical theory of fields}", + publisher = {Course of theoretical physics - Pergamon International Library of Science, Technology, Engineering and Social Studies, Oxford: Pergamon Press, 1971, 3rd rev.~engl.~edition}, + year = 1971, + adsurl = 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{R\"ugamer, S.}, + title = {}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2006}, + note = {in preparation} +} + +@MASTERSTHESIS{Hoehne:Diploma, + author = {H\"ohne, D.}, + title = "{Beobachtung von HESS\,J1813-178 mit dem MAGIC-Teleskop}", + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + month = sep, + year = {2005}, +} + +@MASTERSTHESIS{Dorner:Diploma, + author = {Dorner, D.}, + title = {{S}ystem zum {A}usrichten und {N}achf\"uhren des {MAGIC}-{T}eleskops}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2003} +} + +@MASTERSTHESIS{Riegel:Diploma, + author = {Riegel, B.}, + title = {{S}ystematische {U}ntersuchung der {B}ildparameter f\"ur das {MAGIC}-{T}eleskop}, + school = {Bayerische Julius-Maximilians-Universit{\"a}t W{\"u}rzburg}, + year = {2005} +} + +@MASTERSTHESIS{Bretz:1999, + author = {Bretz, T.}, + title = {Magnetfeldeigenschaften des {S}pektrometers {HADES}}, + school = {Technische Universit{\"a}t M{\"u}nchen}, + year = {1999} +} + +%MASTERSTHESIS{Doro:2005, +% author = {Doro, Michele}, +% year = {2005} +% + +@MISC{Giommi:2006, + author = { Giommi, P. and others}, + year = 2006, + howpublished = {in preparation} +} + +@MISC{Giommi:2005, + author = { Giommi, P.}, + year = 2006, + howpublished = {private communication} +} + +@ARTICLE{Dondi:1995, + author = {{Dondi}, L. and {Ghisellini}, G.}, + title = "{Gamma-ray-loud blazars and beaming}", + journal = {\mnras}, + year = 1995, + month = apr, + volume = 273, + pages = {583-595}, + asdurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995MNRAS.273..583D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fermi:1954, + author = {{Fermi}, E.}, + title = "{Galactic Magnetic Fields and the Origin of Cosmic Radiation.}", + journal = {\apj}, + year = 1954, + month = jan, + volume = 119, + pages = {1-+}, + doi = {10.1086/145789}, + adsurl = 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pages = {891-921}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1905AnP....17..891E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Einstein:1916, + author = {{Einstein}, A.}, + title = "{Die Grundlage der allgemeinen Relativit{\"a}tstheorie}", + journal = {Annalen der Physik}, + year = 1916, + volume = 49, + pages = {769-822}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1916AnP....49..769E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Eddington:1935a, + author = {{Eddington}, A.~S.}, + title = "{On "relativistic degeneracy,"}", + journal = {\mnras}, + year = 1935, + month = jan, + volume = 95, + pages = {194-206}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1935MNRAS..95..194E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Rindler:1956, + author = {{Rindler}, W.}, + title = "{Visual horizons in world models}", + journal = {\mnras}, + year = 1956, + volume = 116, + pages = {662-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1956MNRAS.116..662R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}, +} + +@ARTICLE{Eddington:1935b, + author = {{Eddington}, A.~S.}, + title = "{Note on "relativistic degeneracy"}", + journal = {\mnras}, + year = 1935, + month = nov, + volume = 96, + pages = {20-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1935MNRAS..96...20E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Chandrasekhar:1931, + author = {{Chandrasekhar}, S.}, + title = "{The Maximum Mass of Ideal White Dwarfs}", + journal = {\apj}, + year = 1931, + month = jul, + volume = 74, + pages = {81-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1931ApJ....74...81C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Oppenheimer:1939, + author = {{Oppenheimer}, Julius Robert and {Snyder}, Hartland}, + title = {On continued gravitational contraction}, + journal = {Phys.~Rev.}, + volume = 56, + pages = 455, + year = {1939} +} + +@ARTICLE{Kerr:1963, + author = {{Kerr}, Roy Patrick}, + title = {Gravitational field of a spinning mass as an example of algebraically special metrics}, + journal = {\prl}, + volume = 11, + pages = 237, + year = {1963} +} + +@ARTICLE{Bolton:1971, + author = {{Bolton}, C.~T.}, + title = {Identification of {Cyg} {X}-1 with {HDE} 226868}, + journal = {\nat}, + year = 1972, + volume = 235, + pages = {271}, +} + +@ARTICLE{Shakura:1973, + author = {{Shakura}, N.~I. and {Sunyaev}, R.~A.}, + title = "{Black holes in binary systems. Observational appearance.}", + journal = {\aap}, + year = 1973, + volume = 24, + pages = {337-355}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1973A%26A....24..337S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hasinger:1998, + author = {{Hasinger}, G. and {Burg}, R. and {Giacconi}, R. and {Schmidt}, M. and + {Trumper}, J. and {Zamorani}, G.}, + title = "{The ROSAT Deep Survey. I. 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K.}, + title = {{\"U}ber das {G}ravitationsfeld eines {M}assenpunktes nach der {E}insteinschen {T}heorie}, +booktitle = {Sitzungsberichte der k\"oniglich preu\ss{}ischen {A}kademie der {W}issenschaften zu {B}erlin}, + year = {1916}, + pages = {189-196}, + note = {physics/9905030} +} + +@INPROCEEDINGS{Schwarzschild:1916b, + author = {Schwarzschild, K.}, + title = {{\"U}ber das {G}ravitationsfeld einer {K}ugel aus inkompressibler {F}l\"ussigkeit nach der {E}insteinschen {T}heorie}, +booktitle = {Sitzungsberichte der k\"oniglich preu\ss{}ischen {A}kademie der {W}issenschaften zu {B}erlin}, + year = {1916}, + pages = {424-434}, + note = {physics/9912033} +} + +@ARTICLE{MAGIC:30GeV, + author = {{Moralejo}, A. and others}, + title = {The {MAGIC} telescope for gamma-ray astronomy above 30 {GeV}}, + journal = {\cjaa}, + year = 2003, + month = dec, + volume = 3, + pages = {531-538}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003ChJAA...3S.531M&db_key=AST}, + adsnote = 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Blanton, M.~R. and Eisenstein, D.~J. }, + title = {The {K} correction}, + year = 2002, + month = oct, + journal = {astro-ph}, + note = {astro-ph/0210394} +} + +@ARTICLE{Holder:2006, + author = {Holder, J. and others}, + title = "{The First VERITAS Telescope}", + year = 2006, + month = apr, + journal = {submitted}, + note = {astro-ph/0604119} +} + +@ARTICLE{Lorenz:2004, + author = {{Lorenz}, E.}, + title = "{Status of the 17 m MAGIC telescope}", + journal = {New Astronomy Review}, + year = 2004, + month = apr, + volume = 48, + pages = {339-344}, + doi = {10.1016/j.newar.2003.12.059}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004NewAR..48..339L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kubo:2004, + author = {{Kubo}, H. and others}, + title = "{Status of the CANGAROO-III project}", + journal = {New Astronomy Review}, + year = 2004, + month = apr, + volume = 48, + pages = {323-329}, + doi = 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{http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005Sci...307.1938A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Bradbury:2002, + author = {{Bradbury}, S.~M. and {Rose}, H.~J.}, + title = "{Pattern recognition trigger electronics for an imaging atmospheric Cherenkov telescope}", + journal = {Nuclear Instruments and Methods in Physics Research A}, + year = 2002, + month = apr, + volume = 481, + pages = {521-528}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2002NIMPA.481..521B&db_key=PHY}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Pulhofer:2003, + author = {{P{\"u}hlhofer}, G. and others}, + title = "{The technical performance of the HEGRA system of imaging air Cherenkov telescopes}", + journal = {Astroparticle Physics}, + year = 2003, + month = dec, + volume = 20, + pages = {267-291}, + doi = {10.1016/S0927-6505(03)00194-4}, + adsurl = 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Their Nature and Implications for the Active Galactic Nucleus Luminosity Function}", + journal = {\apj}, + year = 1999, + month = apr, + volume = 514, + pages = {746-764}, + doi = {10.1086/306972}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999ApJ...514..746S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Janiuk:2006, + author = {{Janiuk}, A. and {Czerny}, B. and {Moderski}, R. and {Cline}, D.~B. and + {Matthey}, C. and {Otwinowski}, S.}, + title = "{On the origin of the bimodal duration distribution of gamma-ray bursts and the subjet model}", + journal = {\mnras}, + year = 2006, + month = jan, + volume = 365, + pages = {874-884}, + doi = {10.1111/j.1365-2966.2005.09768.x}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2006MNRAS.365..874J&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Klebesadel:1973, + author = {{Klebesadel}, R.~W. and {Strong}, I.~B. and {Olson}, R.~A.}, + title = "{Observations of Gamma-Ray Bursts of Cosmic Origin}", + journal = {\apjl}, + year = 1973, + month = jun, + volume = 182, + pages = {L85+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1973ApJ...182L..85K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Meszaros:1997, + author = {{Meszaros}, P. and {Rees}, M.~J.}, + title = "{Optical and Long-Wavelength Afterglow from Gamma-Ray Bursts}", + journal = {\apj}, + year = 1997, + month = feb, + volume = 476, + pages = {232-+}, + doi = {10.1086/303625}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997ApJ...476..232M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Waxman:1995, + author = {{Waxman}, E.}, + title = "{Cosmological Gamma-Ray Bursts and the Highest Energy Cosmic Rays}", + journal = {\prl}, + year = 1995, + month = jul, + volume = 75, + pages = {386-389}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995PhRvL..75..386W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Aharonian:2004a, + author = {{Aharonian}, F. and others}, + title = "{Calibration of cameras of the H.E.S.S. detector}", + journal = {Astroparticle Physics}, + year = 2004, + month = nov, + volume = 22, + pages = {109-125}, + doi = {10.1016/j.astropartphys.2004.06.006}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004APh....22..109A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mirzoyan:1994, + author = {{Mirzoyan}, R. and others}, + title = "{The first telescope of the HEGRA air Cherenkov imaging telescope array}", + journal = {Nuclear Instruments and Methods in Physics Research A}, + year = 1994, + month = dec, + volume = 351, + pages = {513-526}, + doi = {10.1016/0168-9002(94)91381-1}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994NIMPA.351..513M&db_key=PHY}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@PHDTHESIS{Krull:1997, + author = {Krull, F.}, + title = {Soft X-ray excess in Aktiven Galaxienkernen}, + school = {Eberhard-Karls Universit\"at T\"ubingen}, + year = 1997 +} + +@PHDTHESIS{Kneiske:2004phd, + author = {Kneiske, T.}, + title = "{Wechselwirkung von Gammastrahlung mit dem metagalaktischen Strahlungsfeld}", + school = {Bayerische Julius-Maximilians-Universit\"at W\"urzburg}, + year = 2004 +} + +@ARTICLE{Veron:2003, + author = {{V{\'e}ron-Cetty}, M.-P. and {V{\'e}ron}, P.}, + title = "{A catalogue of quasars and active nuclei: 11th edition}", + journal = {\aap}, + year = 2003, + month = dec, + volume = 412, + pages = {399-403}, + doi = {10.1051/0004-6361:20034225}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003A%26A...412..399V&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sbarufatti:2005, + author = {{Sbarufatti}, B. and {Treves}, A. and {Falomo}, R.}, + title = "{Imaging Redshifts of BL Lacertae Objects}", + journal = {\apj}, + year = 2005, + month = dec, + volume = 635, + pages = {173-179}, + doi = {10.1086/497022}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005ApJ...635..173S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Elvis:1992, + author = {{Elvis}, M. and {Plummer}, D. and {Schachter}, J. and {Fabbiano}, G. + }, + title = "{The Einstein Slew Survey}", + journal = {\apjs}, + year = 1992, + month = may, + volume = 80, + pages = {257-303}, + doi = {10.1086/191665}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1992ApJS...80..257E&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Muecke:2001, + author = {{M{\"u}cke}, A. and {Protheroe}, R.~J.}, + title = "{A proton synchrotron blazar model for flaring in Markarian 501}", + journal = {Astroparticle Physics}, + year = 2001, + month = mar, + volume = 15, + pages = {121-136}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001APh....15..121M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1996b, + author = {{Mannheim}, K. and {Westerhoff}, S. and {Meyer}, H. and {Fink}, H.-H. + }, + title = "{Beacons at the gamma ray horizon.}", + journal = {\aap}, + year = 1996, + month = nov, + volume = 315, + pages = {77-85}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26A...315...77M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Stecker:1992, + author = {{Stecker}, F.~W. and {de Jager}, O.~C. and {Salamon}, M.~H.}, + title = "{TeV gamma rays from 3C~279 - A possible probe of origin and intergalactic infrared radiation fields}", + journal = {\apjl}, + year = 1992, + month = may, + volume = 390, + pages = {L49-L52}, + doi = {10.1086/186369}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992ApJ...390L..49S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ben:2002, + author = {{Ben-Zhong}, Dai and {Ghunag-Zhong}, Xie and {Ze-Jun}, Jiang}, + title = {Properties of BL Lac Objects with Redshift $\le$ 2}, + journal = {\cjaa}, + year = 2002, + volume = 2, + pages = {8-16} +} + +@ARTICLE{LiMa:1983, + author = {{Li}, T.-P. and {Ma}, Y.-Q.}, + title = "{Analysis methods for results in gamma-ray astronomy}", + journal = {\apj}, + year = 1983, + month = sep, + volume = 272, + pages = {317-324}, + doi = {10.1086/161295}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1983ApJ...272..317L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Bartko:2005pa, + author = {Bartko, H. and Gaug, M. and Moralejo, A. and Sidro, N.}, + collaboration = {MAGIC}, + title = {{FADC} pulse reconstruction using a digital filter for the {MAGIC} telescope}, + year = {2005}, + note = {astro-ph/0506459}, + eprint = {astro-ph/0506459}, + journal = {astro-ph}, + SLACcitation = {%%CITATION = ASTRO-PH 0506459;%%} +} + +@INPROCEEDINGS{Hillas:1985icrc, + author = {{Hillas}, A.~M.}, + title = {Cerenkov light images of {EAS} produced by primary gamma}, +booktitle = {$19^{th}$ International Cosmic Ray Conference}, + year = 1985, + month = Aug, + pages = {445-448}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ICRC....3..445H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Blandford:1993, + author = {{Blandford, R.~D.}}, + title = {Gamma ray jets from active galactiv nuclei}, +booktitle = {Compton Gamma Ray Observatory}, + journal = {AIP Conf. Proc.}, + volume = 280, + year = 1993, + pages = {533}, + editor = {Gehrels} +} + +@ARTICLE{Kneiske:2004, + author = {{Kneiske}, T.~M. and {Bretz}, T. and {Mannheim}, K. and {Hartmann}, D.~H.}, + title = {Implications of cosmological gamma-ray absorption. {II}. Modification of gamma-ray spectra}, + journal = {\aap}, + year = 2004, + month = jan, + volume = 413, + pages = {807-815}, + doi = {10.1051/0004-6361:20031542}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004A%26A...413..807K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kneiske:2002, + author = {{Kneiske}, T.~M. and {Mannheim}, K. and {Hartmann}, D.~H.}, + title = {Implications of cosmological gamma-ray absorption. {I}. {E}volution of the metagalactic radiation field}, + journal = {\aap}, + year = 2002, + month = apr, + volume = 386, + pages = {1-11}, + doi = {10.1051/0004-6361:20020211}, + adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2002A%26A...386....1K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hernandez:2005, + author = {{Hern{\'a}ndez-Rey}, J.~J.}, + title = "{The Neutrino Telescope Antares}", + journal = {\apss}, + year = 2005, + month = jun, + volume = 297, + pages = {257-267}, + doi = {10.1007/s10509-005-7628-4}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005Ap%26SS.297..257H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Bretz:2003icrc, + author = {{Bretz}, T.}, + title = {The {MAGIC} {A}nalysis and {R}econstruction {S}oftware}, +booktitle = {$28^{th}$ International Cosmic Ray Conference}, + year = 2003, + month = Aug +} + +@INPROCEEDINGS{Bretz:2004gamma, + author = {{Bretz}, T.}, + title = {{MARS} - {R}oadmap to a standard analysis}, +booktitle = {$2^{nd}$ International Symposium on High Energy Gamma-Ray Astronomy}, + year = 2004, + month = Jul +} + +@INPROCEEDINGS{Bretz:2005paris, + author = {{Bretz}, T. and Dorner, D.}, + title = {{MARS} - {A} framework for a standard analysis}, +booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, + year = 2005, + month = Apr +} + +@INPROCEEDINGS{Dorner:2005paris, + author = {{Dorner}, D. and Bretz, T.}, + title = {A concept for data managment and processing}, +booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, + pages = {571-575}, + year = 2005, + month = Apr +} + +@INPROCEEDINGS{Bastieri:2005, + author = {Bastieri, D. and others}, + title = {The mirrors of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Dorner:2005icrc, + author = {Dorner, D. and Berger, K. and Bretz, T. and Gaug, M. and others}, + title = {Data Managment and Processing for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 175, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Beixeras:2005, + author = {Beixeras, C. and others}, + title = "{MAGIC II}", +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + volume = 5, + pages = {227}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Cortina:2005, + author = {Cortina, J. and others}, + title = {Technical performance of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Bretz:2005mars, + author = {Bretz, T.}, + title = {Standard Analysis for the {MAGIC} Telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + volume = 4, + year = 2005, + pages = 315, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Gaug:2005, + author = {Gaug, M. and Bartko, H. and Cortina, J. and Rico, J. and others}, + title = {Calibration of the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Riegel:2005icrc, + author = {{Riegel}, B. and Bretz, T.}, + title = {A systematic study of the interdependance of the {IACT} image parameters}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 215, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Riegel:2005icrc2, + author = {{Riegel}, B. and Bretz, T. and Dorner, D. and Wagner, R.~M. and others}, + title = {A tracking monitor for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + volume = 5, + pages = 219, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Goebel:2005, + author = {{Goebel}, F. and Mase, K. and Meyer, M. and Mirzoyan, R. and Shayduk, M. and Teshima, M. and others}, + title = {Absolute energy scale calibration of the {MAGIC} telescope using muon images}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Majumdar:2005icrc, + author = {{Majumdar}, P. and {Moralejo}, A. and {Bigongiari}, C. and {Blanch}, O. and {Sobczynska}, D.}, + title = {{M}onte {C}arlo simulation for the {MAGIC} telescope}, +booktitle = {$29^{th}$ International Cosmic Ray Conference}, + year = 2005, + month = Aug, + note = {astro-ph/0508274} +} + +@INPROCEEDINGS{Meyer:2005icrc, + author = {{Meyer}, M. and Mannheim, K. and Bretz, T. and Dorner, D. and Riegel, B. and H\"ohne, D. and Berger, K. and others}, + title = {{MAGIC} observations of high-peaked {BL} {L}ac objects}, +booktitle = {$28^{th}$ International Cosmic Ray Conference}, + volume = 4, + pages = 335, + year = 2005, + month = Aug, + note = {astro-ph/0508273} +} + +@ARTICLE{Lessard:2001, + author = {{Lessard}, R.~W. and {Buckley}, J.~H. and {Connaughton}, V. and {Le Bohec}, S.}, + title = "{A new analysis method for reconstructing the arrival direction of TeV gamma rays using a single imaging atmospheric Cherenkov telescope}", + journal = {Astroparticle Physics}, + year = 2001, + month = mar, + volume = 15, + pages = {1-18}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001APh....15....1L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Urry:1995, + author = {{Urry}, C.~M. and {Padovani}, P.}, + title = "{Unified Schemes for Radio-Loud Active Galactic Nuclei}", + journal = {\pasp}, + year = 1995, + month = sep, + volume = 107, + pages = {803-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995PASP..107..803U&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Urry:2000, + author = {{Urry}, C.~M. and {Scarpa}, R. and {O'Dowd}, M. and {Falomo}, R. and + {Pesce}, J.~E. and {Treves}, A.}, + title = "{The Hubble Space Telescope Survey of BL Lacertae Objects. II. Host Galaxies}", + journal = {\apj}, + year = 2000, + month = apr, + volume = 532, + pages = {816-829}, + doi = {10.1086/308616}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000ApJ...532..816U&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Porter:1960, + author = {Hill, D.~A. and Porter, N.~A}, + title = "{Photography of \v{C}erenkov Light from Extensive Air Showers in the Atmosphere}", + month = aug, + year = 1960, + journal = {\nat}, + volume = 191, + pages = 690, + note = {Letters to Editor} +} + +@ARTICLE{Jelley:1963, + author = {{Jelley}, J.~V. and {Porter}, N.~A.}, + title = "{{\v C}erenkov Radiation from the Night Sky, and its Application to {$\gamma$}-Ray Astronomy}", + journal = {\qjras}, + year = 1963, + month = sep, + volume = 4, + pages = {275-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1963QJRAS...4..275J&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Padovani:1995, + author = {{Padovani}, P. and {Giommi}, P.}, + title = "{The connection between x-ray- and radio-selected BL Lacertae objects}", + journal = {\apj}, + year = 1995, + month = may, + volume = 444, + pages = {567-581}, + doi = {10.1086/175631}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...444..567P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Boella:1997, + author = {{Boella}, G. and {Butler}, R.~C. and {Perola}, G.~C. and {Piro}, L. and + {Scarsi}, L. and {Bleeker}, J.~A.~M.}, + title = "{BeppoSAX, the wide band mission for X-ray astronomy}", + journal = {\aaps}, + year = 1997, + month = apr, + volume = 122, + pages = {299-307}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997A%26AS..122..299B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Catanese:1999, + author = {{Catanese}, M. and {Weekes}, T.~C.}, + title = "{Very High Energy Gamma-Ray Astronomy}", + journal = {\pasp}, + year = 1999, + month = oct, + volume = 111, + pages = {1193-1222}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999PASP..111.1193C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Daum:1997, + author = {{Daum}, A. and others}, + title = "{First results on the performance of the HEGRA IACT array}", + journal = {Astroparticle Physics}, + year = 1997, + month = dec, + volume = 8, + pages = {1-2}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997APh.....8....1D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Aharonian:2004, + author = {{Aharonian}, F. and others}, + title = "{Observations of 54 Active Galactic Nuclei with the HEGRA system of Cherenkov telescopes}", + journal = {\aap}, + year = 2004, + month = jul, + volume = 421, + pages = {529-537}, + doi = {10.1051/0004-6361:20035764}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004A%26A...421..529A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Pohl:2000, + author = {{Pohl}, M. and {Schlickeiser}, R.}, + title = "{On the conversion of blast wave energy into radiation in active galactic nuclei and gamma-ray bursts}", + journal = {\aap}, + year = 2000, + month = feb, + volume = 354, + pages = {395-410}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000A%26A...354..395P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1993, + author = {{Mannheim}, K.}, + title = "{The proton blazar}", + journal = {\aap}, + year = 1993, + month = mar, + volume = 269, + pages = {67-76}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993A%26A...269...67M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# CHECK AGAIN! +@INPROCEEDINGS{Sikora:2001, + author = {{Sikora}, M.}, + title = "{Jets in Quasars}", +booktitle = {ASP Conf. Ser. 227: Blazar Demographics and Physics}, + year = 2001, + pages = {95-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ASPC..227...95S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sikora:1987, + author = {{Sikora}, M. and {Kirk}, J.~G. and {Begelman}, M.~C. and {Schneider}, P. + }, + title = "{Electron injection by relativistic protons in active galactic nuclei}", + journal = {\apjl}, + year = 1987, + month = sep, + volume = 320, + pages = {L81-L85}, + doi = {10.1086/184980}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987ApJ...320L..81S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# CHECK AGAIN +@ARTICLE{Burns:1982, + author = {{Burns}, M.~L. and {Lovelace}, R.~V.~E.}, + title = "{Theory of electron-positron showers in double radio sources}", + journal = {\apj}, + year = 1982, + month = nov, + volume = 262, + pages = {87-99}, + doi = {10.1086/160399}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...262...87B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Svensson:1987, + author = {{Svensson}, R.}, + title = "{Non-thermal pair production in compact X-ray sources - First-order Compton cascades is soft radiation fields}", + journal = {\mnras}, + year = 1987, + month = jul, + volume = 227, + pages = {403-451}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987MNRAS.227..403S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@BOOK{Berezinskii:1990, + author = {{Berezinskii}, V.~S. and {Bulanov}, S.~V. and {Dogiel}, V.~A. and + {Ptuskin}, V.~S.}, + title = "{Astrophysics of cosmic rays}", +publisher = {Amsterdam: North-Holland, 1990, edited by Ginzburg, V.L.}, +year = 1990, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1990acr..book.....B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1991, + author = {{Mannheim}, K. and {Biermann}, P.~L. and {Kruells}, W.~M.}, + title = "{A novel mechanism for nonthermal X-ray emission}", + journal = {\aap}, + year = 1991, + month = nov, + volume = 251, + pages = {723-731}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1991A%26A...251..723M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Mannheim:1997, + author = {{Mannheim}, K.}, + title = "{AGN Models: High-Energy Emission.}", +booktitle = {Very High Energy Phenomena in the Universe; Moriond Workshop}, + year = 1997, + pages = {17-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997vhep.conf...17M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Mannheim:1998, + author = {{Mannheim}, K.}, + title = "{Possible Production of High-Energy Gamma Rays from Proton Acceleration in the Extragalactic Radio Source Markarian 501}", + journal = {Science}, + year = 1998, + month = jan, + volume = 279, + pages = {684-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998Sci...279..684M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Hauser:2001, + author = {{Hauser}, M.~G. and {Dwek}, E.}, + title = "{The Cosmic Infrared Background: Measurements and Implications}", + journal = {\araa}, + year = 2001, + volume = 39, + pages = {249-307}, + doi = {10.1146/annurev.astro.39.1.249}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ARA%26A..39..249H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +# TO BE CHECKED! +@ARTICLE{Perlman:1998, + author = {{Perlman}, E.~S. and {Padovani}, P. and {Giommi}, P. and {Sambruna}, R. and + {Jones}, L.~R. and {Tzioumis}, A. and {Reynolds}, J.}, + title = "{The Deep X-Ray Radio Blazar Survey. I. Methods and First Results}", + journal = {\aj}, + year = 1998, + month = apr, + volume = 115, + pages = {1253-1294}, + doi = {10.1086/300283}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998AJ....115.1253P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Laurent-Muehleisen:1998, + author = {{Laurent-Muehleisen}, S.~A. and {Kollgaard}, R.~I. and {Feigelson}, E.~D. + }, + title = "{The Rosat-Green Bank Sample of Intermediate BL Lac Objects}", +booktitle = {ASP Conf. Ser. 144: IAU Colloq. 164: Radio Emission from Galactic and Extragalactic Compact Sources}, + year = 1998, + pages = {163-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998ASPC..144..163L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Caccianiga:1999, + author = {{Caccianiga}, A. and {Maccacaro}, T. and {Wolter}, A. and {della Ceca}, R. and + {Gioia}, I.~M.}, + title = "{The REX Survey: A Search for Radio-emitting X-Ray Sources}", + journal = {\apj}, + year = 1999, + month = mar, + volume = 513, + pages = {51-68}, + doi = {10.1086/306822}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999ApJ...513...51C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Caccianiga:2004, + author = {{Caccianiga}, A. and {March{\~a}}, M.~J.~M.}, + title = "{The CLASS blazar survey: testing the blazar sequence}", + journal = {\mnras}, + year = 2004, + month = mar, + volume = 348, + pages = {937-954}, + doi = {10.1111/j.1365-2966.2004.07415.x}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004MNRAS.348..937C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kellermann:1989, + author = {{Kellermann}, K.~I. and {Sramek}, R. and {Schmidt}, M. and {Shaffer}, D.~B. and + {Green}, R.}, + title = "{VLA observations of objects in the Palomar Bright Quasar Survey}", + journal = {\aj}, + year = 1989, + month = oct, + volume = 98, + pages = {1195-1207}, + doi = {10.1086/115207}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1989AJ.....98.1195K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Rowan:1977, + author = {{Rowan-Robinson}, M.}, + title = "{On the unity of activity in galaxies}", + journal = {\apj}, + year = 1977, + month = may, + volume = 213, + pages = {635-647}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1977ApJ...213..635R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lawrence:1982, + author = {{Lawrence}, A. and {Elvis}, M.}, + title = "{Obscuration and the various kinds of Seyfert galaxies}", + journal = {\apj}, + year = 1982, + month = may, + volume = 256, + pages = {410-426}, + doi = {10.1086/159918}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...256..410L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Giommi:1994, + author = {{Giommi}, P. and {Padovani}, P.}, + title = "{Bl-Lacertae Reunification}", + journal = {\mnras}, + year = 1994, + month = may, + volume = 268, + pages = {L51+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994MNRAS.268L..51G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Antonucci:1985, + author = {{Antonucci}, R.~R.~J. and {Ulvestad}, J.~S.}, + title = "{Extended radio emission and the nature of blazars}", + journal = {\apj}, + year = 1985, + month = jul, + volume = 294, + pages = {158-182}, + doi = {10.1086/163284}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ApJ...294..158A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fossati:1998, + author = {{Fossati}, G. and {Maraschi}, L. and {Celotti}, A. and {Comastri}, A. and + {Ghisellini}, G.}, + title = "{A unifying view of the spectral energy distributions of blazars}", + journal = {\mnras}, + year = 1998, + month = sep, + volume = 299, + pages = {433-448}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998MNRAS.299..433F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Aharonian:2000, + author = {{Aharonian}, F.}, + title = "{TeV gamma rays from BL Lac objects due to synchrotron radiation of extremely high energy protons}", + journal = {\na}, + year = 2000, + month = nov, + volume = 5, + pages = {377-395}, + doi = {10.1016/S1384-1076(00)00039-7}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000NewA....5..377A&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Muecke:2003, + author = {{M{\"u}cke}, A. and {Protheroe}, R.~J. and {Engel}, R. and {Rachen}, J.~P. and + {Stanev}, T.}, + title = "{BL Lac objects in the synchrotron proton blazar model}", + journal = {Astroparticle Physics}, + year = 2003, + month = mar, + volume = 18, + pages = {593-613}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003APh....18..593M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Schlickeiser:2000, + author = {{Pohl}, M. and {Schlickeiser}, R.}, + title = "{On the conversion of blast wave energy into radiation in active galactic nuclei and gamma-ray bursts}", + journal = {\aap}, + year = 2000, + month = feb, + volume = 354, + pages = {395-410}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000A%26A...354..395P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lyutikov:2005, + author = {{Lyutikov}, M.}, + title = "{Composition of ultra-relativistic jets}", + journal = {American Astronomical Society Meeting Abstracts}, + year = 2005, + month = may, + volume = 206, + pages = {-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005AAS...206.3008L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sikora:2005, + author = {{Sikora}, M. and {Begelman}, M.~C. and {Madejski}, G.~M. and + {Lasota}, J.-P.}, + title = "{Are Quasar Jets Dominated by Poynting Flux?}", + journal = {\apj}, + year = 2005, + month = may, + volume = 625, + pages = {72-77}, + doi = {10.1086/429314}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005ApJ...625...72S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Montigny:1995, + author = {{von Montigny}, C. and others}, + title = "{High-Energy Gamma-Ray Emission from Active Galaxies: EGRET Observations and Their Implications}", + journal = {\apj}, + year = 1995, + month = feb, + volume = 440, + pages = {525-+}, + doi = {10.1086/175294}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...440..525V&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fichtel:1994, + author = {{Fichtel}, C.~E. and others}, + title = "{The first energetic gamma-ray experiment telescope (EGRET) source catalog}", + journal = {\apjs}, + year = 1994, + month = oct, + volume = 94, + pages = {551-581}, + doi = {10.1086/192082}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994ApJS...94..551F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Thompson:1995, + author = {{Thompson}, D.~J. and others}, + title = "{The Second EGRET Catalog of High-Energy Gamma-Ray Sources}", + journal = {\apjs}, + year = 1995, + month = dec, + volume = 101, + pages = {259-+}, + doi = {10.1086/192240}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJS..101..259T&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ghisellini:1989, + author = {{Ghisellini}, G. and {Maraschi}, L.}, + title = "{Bulk acceleration in relativistic jets and the spectral properties of blazars}", + journal = {\apj}, + year = 1989, + month = may, + volume = 340, + pages = {181-189}, + doi = {10.1086/167383}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1989ApJ...340..181G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Weekes:1996, + author = {{Weekes}, T.~C. and others}, + title = "{Observations of gamma-ray sources at energies $>$300GeV.}", + journal = {\aaps}, + year = 1996, + month = dec, + volume = 120, + pages = {C603+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26AS..120C.603W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Petry:1996, + author = {{Petry}, D. and others}, + title = "{Detection of VHE {$\gamma$}-rays from MKN 421 with the HEGRA Cherenkov Telescopes.}", + journal = {\aap}, + year = 1996, + month = jul, + volume = 311, + pages = {L13-L16}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26A...311L..13P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Tavecchio:1998, + author = {{Tavecchio}, F. and {Maraschi}, L. and {Ghisellini}, G.}, + title = "{Constraints on the Physical Parameters of TeV Blazars}", + journal = {\apj}, + year = 1998, + month = dec, + volume = 509, + pages = {608-619}, + doi = {10.1086/306526}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998ApJ...509..608T&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Bloom:1993, + author = {{Bloom}, S.~D. and {Marscher}, A.~P. and {Gear}, W.~K.}, + title = "{Multiwavelength Observations of Flat Radio Spectrum Quasars and Active Galaxies}", + journal = {\baas}, + year = 1993, + month = may, + volume = 25, + pages = {920-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993AAS...182.7007B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Schmidt:1963, + author = {{Schmidt}, M.}, + title = "{3C 273: a star-like object with large red-shift.}", + journal = {\nat}, + year = 1963, + volume = 197, + pages = {1040-1040}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1963Natur.197.1040S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ghisellini:1994, + author = {Ghisellini, G. and Maraschi, L.}, + title = {Are $\gamma$-rays from {HPQ}s and {BL} {L}acs due to the same process?}, +booktitle = {Proceedings of the Second Compton Symposium}, + journal = {AIP Conf. Proc.}, + pages = 616, + year = 1994, + volume = 304, +} + +@ARTICLE{Dermer:1993, + author = {{Dermer}, C.~D. and {Schlickeiser}, R.}, + title = "{Model for the High-Energy Emission from Blazars}", + journal = {\apj}, + year = 1993, + month = oct, + volume = 416, + pages = {458-+}, + doi = {10.1086/173251}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993ApJ...416..458D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Dermer:2002, + author = {{Dermer}, C.~D.}, + title = "{Neutrino, Neutron, and Cosmic-Ray Production in the External Shock Model of Gamma-Ray Bursts}", + journal = {\apj}, + year = 2002, + month = jul, + volume = 574, + pages = {65-87}, + doi = {10.1086/340893}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2002ApJ...574...65D&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Sikora:1994, + author = {{Sikora}, M. and {Begelman}, M.~C. and {Rees}, M.~J.}, + title = "{Comptonization of diffuse ambient radiation by a relativistic jet: The source of gamma rays from blazars?}", + journal = {\apj}, + year = 1994, + month = jan, + volume = 421, + pages = {153-162}, + doi = {10.1086/173633}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994ApJ...421..153S&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Blandford:1995, + author = {{Blandford}, R.~D. and {Levinson}, A.}, + title = "{Pair cascades in extragalactic jets. 1: Gamma rays}", + journal = {\apj}, + year = 1995, + month = mar, + volume = 441, + pages = {79-95}, + doi = {10.1086/175338}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...441...79B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Wagner:1995, + author = {{Wagner}, S.~J. and others}, + title = "{High-Energy Gamma Rays from PKS 1406-076 and the Observation of Correlated Gamma-Ray and Optical Emission}", + journal = {\apjl}, + year = 1995, + month = dec, + volume = 454, + pages = {L97+}, + doi = {10.1086/309776}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...454L..97W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Blandford:1978, + author = {{Blandford}, R.~D. and {Rees}, M.~J.}, + title = "{Some comments on radiation mechanisms in Lacertids}", +booktitle = {Pittsburgh Conference on BL Lac Objects, Pittsburgh, Pa., April 24-26, 1978, Proceedings. (A79-30026 11-90) Pittsburgh, Pa., University of Pittsburgh, 1978, p. 328-341; Discussion, p. 341-347. NATO-supported research}, + year = 1978, + pages = {328-341}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1978bllo.conf..328B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Bradbury:1997, + author = {{Bradbury}, S.~M. and others}, + title = "{Detection of {$\gamma$}-rays above 1.5TeV from MKN 501.}", + journal = {\aap}, + year = 1997, + month = apr, + volume = 320, + pages = {L5-L8}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997A%26A...320L...5B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Browne:1983, + author = {{Browne}, I.~W.~A.}, + title = "{Is it possible to turn an elliptical radio galaxy into a BL Lac object?}", + journal = {\mnras}, + year = 1983, + month = jul, + volume = 204, + pages = {23P-27P}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1983MNRAS.204P..23B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Celotti:2003, + author = {{Celotti}, A.}, + title = "{On the energetics and composition of jets}", + journal = {\nar}, + year = 2003, + month = oct, + volume = 47, + pages = {525-528}, + doi = {10.1016/S1387-6473(03)00086-1}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003NewAR..47..525C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Wardle:1984, + author = {{Wardle}, J.~F.~C. and {Moore}, R.~L. and {Angel}, J.~R.~P.}, + title = "{The radio morphology of blazars and relationships to optical polarization and to normal radio galaxies}", + journal = {\apj}, + year = 1984, + month = apr, + volume = 279, + pages = {93-98}, + doi = {10.1086/161868}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1984ApJ...279...93W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lind:1985, + author = {{Lind}, K.~R. and {Blandford}, R.~D.}, + title = "{Semidynamical models of radio jets - Relativistic beaming and source counts}", + journal = {\apj}, + year = 1985, + month = aug, + volume = 295, + pages = {358-367}, + doi = {10.1086/163380}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ApJ...295..358L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Phinney:1986, + author = {{Phinney}}, + title = {Astrophysics of {A}ctive {G}alaxies and {QSO}s}, +publisher = {Oxford University Press}, + editor = {R.W.Miller}, + year = 1986, + page = 453, +} + +@ARTICLE{Fazio:1979, + author = {{Fazio}, G.~G. and {Stecker}, F.~W.}, + year = 1979, + volume = 226, + pages = {135-+}, + title = {Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin}, + journal = {\nat} +} + +@ARTICLE{Punch:1992, + author = {{Punch}, M. and others}, + title = "{Detection of TeV photons from the active galaxy Markarian 421}", + journal = {\nat}, + year = 1992, + month = aug, + volume = 358, + pages = {477-+}, + doi = {10.1038/358477a0}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992Natur.358..477P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Fanaroff:1974, + author = {{Fanaroff}, B.~L. and {Riley}, J.~M.}, + title = "{The morphology of extragalactic radio sources of high and low luminosity}", + journal = {\mnras}, + year = 1974, + month = may, + volume = 167, + pages = {31P-36P}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1974MNRAS.167P..31F&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Odell:1974, + author = {{Jones}, T.~W. and {O'dell}, S.~L. and {Stein}, W.~A.}, + title = "{Physics of Compact Nonthermal Sources. Theory of Radiation Processes}", + journal = {\apj}, + year = 1974, + month = mar, + volume = 188, + pages = {353-368}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1974ApJ...188..353J&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ghisellini:1993, + author = {{Ghisellini}, G. and {Padovani}, P. and {Celotti}, A. and {Maraschi}, L. + }, + title = "{Relativistic bulk motion in active galactic nuclei}", + journal = {\apj}, + year = 1993, + month = apr, + volume = 407, + pages = {65-82}, + doi = {10.1086/172493}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993ApJ...407...65G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ghisellini:1998, + author = {{Ghisellini}, G. and {Celotti}, A. and {Fossati}, G. and {Maraschi}, L. and + {Comastri}, A.}, + title = "{A theoretical unifying scheme for gamma-ray bright blazars}", + journal = 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acceleration of charged particles at relativistic shock fronts}", + journal = {\apj}, + year = 1987, + month = apr, + volume = 315, + pages = {425-433}, + doi = {10.1086/165147}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987ApJ...315..425K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Kirk:1998, + author = {{Kirk}, J.~G. and {Rieger}, F.~M. and {Mastichiadis}, A.}, + title = "{Particle acceleration and synchrotron emission in blazar jets}", + journal = {\aap}, + year = 1998, + month = may, + volume = 333, + pages = {452-458}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998A%26A...333..452K&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lawrence:1987, + author = {{Lawrence}, A.}, + title = "{Classification of active galaxies and the prospect of a unified phenomenology}", + journal = {\pasp}, + year = 1987, + month = may, + volume = 99, + pages = {309-334}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987PASP...99..309L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Padovani:1993, + author = {{Padovani}, P.}, + title = "{The Radio Loud Fraction of QSOs and its Dependence on Magnitude and Redshift}", + journal = {\mnras}, + year = 1993, + month = jul, + volume = 263, + pages = {461-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993MNRAS.263..461P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{LaFranca:1994, + author = {{La Franca}, F. and {Gregorini}, L. and {Cristiani}, S. and + {de Ruiter}, H. and {Owen}, F.}, + title = "{Deep VLA observations of an optically selected sample of intermediate redshift QSOs and the optical luminosity function of the radio loud QSOs}", + journal = {\aj}, + year = 1994, + month = nov, + volume = 108, + pages = 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month = nov, + volume = 399, + pages = {L23-L26}, + doi = {10.1086/186597}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992ApJ...399L..23P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Pier:1993, + author = {{Pier}, E.~A. and {Krolik}, J.~H.}, + title = "{Infrared Spectra of Obscuring Dust Tori around Active Galactic Nuclei. 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Stretching the blazar sequence}", + journal = {\aap}, + year = 2001, + month = may, + volume = 371, + pages = {512-526}, + doi = {10.1051/0004-6361:20010412}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001A%26A...371..512C&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + + +@ARTICLE{Blandford:1979, + author = {{Blandford}, R.~D. and {K\"onigl}, A.}, + title = "{Relativistic jets as compact radio sources}", + journal = {\apj}, + year = 1979, + month = aug, + volume = 232, + pages = {34-48}, + doi = {10.1086/157262}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1979ApJ...232...34B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Ghisellini:1996b, + author = {{Ghisellini}, G. and {Maraschi}, L. and {Dondi}, L.}, + title = "{Diagnostics of Inverse-Compton models for the {$\gamma$}-ray emission of 3C~279 and MKN 421.}", + journal = {\aaps}, + year = 1996, + month = dec, + volume = 120, + pages = {C503+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26AS..120C.503G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lamer:1996, + author = {{Lamer}, G. and {Brunner}, H. and {Staubert}, R.}, + title = "{ROSAT observations of BL Lacertae objects.}", + journal = {\aap}, + year = 1996, + month = jul, + volume = 311, + pages = {384-392}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26A...311..384L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Blustin:2004, + author = {{Blustin}, A.~J. and {Page}, M.~J. and {Branduardi-Raymont}, G. + }, + title = "{Intrinsic absorbers in BL Lac objects: The XMM-Newton view}", + journal = {\aap}, + year = 2004, + month = apr, + volume = 417, + pages = {61-70}, + doi = {10.1051/0004-6361:20034517}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004A%26A...417...61B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Spergel:2006, + author = {{Spergel}, D.~N. and others}, + title = "{Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for cosmology}", + journal = {in preparation}, + year = 2006, + note= {\url{http://lambda.gsfc.nasa.gov/product/map/dr2/map_bibliography.cfm}} +} + +@ARTICLE{Weekes:1989, + author = {{Weekes}, T.~C. and {Cawley}, M.~F. and {Fegan}, D.~J. and {Gibbs}, K.~G. and + {Hillas}, A.~M. and {Kowk}, P.~W. and {Lamb}, R.~C. and {Lewis}, D.~A. and + {Macomb}, D. and {Porter}, N.~A. and {Reynolds}, P.~T. and {Vacanti}, G. + }, + title = "{Observation of TeV gamma rays from the Crab nebula using the atmospheric Cerenkov imaging technique}", + journal = {\apj}, + year = 1989, + month = jul, + volume = 342, + pages = {379-395}, + doi = {10.1086/167599}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1989ApJ...342..379W&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Morrison:1958, + author = {Morrison, P.}, + title = {On Gamma-Ray Astronomy}, + journal = {Il nuovo cimento}, + year = 1958, + volume = {Vol.\,VII, N.\,6}, +} + +@ARTICLE{Blasi:2005, + author = {{Blasi}, P. and {Vietri}, M.}, + title = "{On Particle Acceleration around Shocks. 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A Fully General Method for Arbitrary Shock Velocities and Scattering Media}", + journal = {\apj}, + year = 2005, + month = jun, + volume = 626, + pages = {877-886}, + doi = {10.1086/430164}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005ApJ...626..877B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Blandford:1982, + author = {{Blandford}, R.~D. and {Payne}, D.~G.}, + title = "{Hydromagnetic flows from accretion discs and the production of radio jets}", + journal = {\mnras}, + year = 1982, + month = jun, + volume = 199, + pages = {883-903}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982MNRAS.199..883B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Hillas:1983, + author = {{Hillas}, A.~M.}, + title = "{Ultra high energy cosmic rays}", +booktitle = {NATO ASIC Proc. 107: Composition and Origin of Cosmic Rays}, + year = 1983, + pages = {125-148}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1983cocr.proc..125H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@PROCEEDINGS{Holt:1992, + editor = {{Holt}, S.~S. and {Neff}, S.~G. and {Urry}, C.~M.}, + title = "{Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oct. 14-16, 1991}", +booktitle = {American Institute of Physics Conference Series}, + year = 1992, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992AIPC..254.....H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@BOOK{Heitler:1957, + author = {{Heitler}, W.}, + title = "{Quantum theory of radiation}", +publisher = {International Series of Monographs on Physics, Oxford: Clarendon, 1954, 3rd ed.}, +year = 1954, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1954qtr..book.....H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Halzen:1992b, + author = {{Halzen}, F.}, + title = "{Gamma-Ray Astronomy - Catching Photons from Hell}", + journal = {\nat}, + year = 1992, + month = aug, + volume = 358, + pages = {452-+}, + doi = {10.1038/358452a0}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992Natur.358..452H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Halzen:1991, + author = {{Halzen}, F. and {Zas}, E. and {MacGibbon}, J.~H. and {Weekes}, T.~C. + }, + title = "{Gamma rays and energetic particles from primordial black holes}", + journal = {\nat}, + year = 1991, + month = oct, + volume = 353, + pages = {807-815}, + doi = {10.1038/353807a0}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1991Natur.353..807H&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Halzen:1992, + author = {{Halzen}, F. and {Zas}, E.}, + title = "{Giant horizontal air showers. 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Ser. 100: Energy Transport in Radio Galaxies and Quasars}, + year = 1996, + editor = {{Hardee}, P.~E. and {Bridle}, A.~H. and {Zensus}, J.~A.}, + pages = {45-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996ASPC..100...45M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Marscher:1996b, + author = {{Marscher}, A.~P. and {Travis}, J.~P.}, + title = "{Synchrotron self-Compton interpretation of multiwaveband observations of gamma-ray bright blazars.}", + journal = {\aaps}, + year = 1996, + month = dec, + volume = 120, + pages = {C537+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1996A%26AS..120C.537M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Maraschi:1992, + author = {{Maraschi}, L. and {Ghisellini}, G. and {Celotti}, A.}, + title = "{A jet model for the gamma-ray emitting blazar 3C~279}", + journal = {\apjl}, + year = 1992, + month = sep, + volume = 397, + pages = {L5-L9}, + doi = {10.1086/186531}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1992ApJ...397L...5M&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Giommi:1999, + author = {{Giommi}, P. and {Menna}, M.~T. and {Padovani}, P.}, + title = "{The sedentary multifrequency survey - I. Statistical identification and cosmological properties of high-energy peaked BL Lacs}", + journal = {\mnras}, + year = 1999, + month = dec, + volume = 310, + pages = {465-475}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999MNRAS.310..465G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Padovani:2003, + author = {{Padovani}, P. and {Perlman}, E.~S. and {Landt}, H. and {Giommi}, P. and + {Perri}, M.}, + title = "{What Types of Jets Does Nature Make? A New Population of Radio Quasars}", + journal = {\apj}, + year = 2003, + month = may, + volume = 588, + pages = {128-142}, + doi = {10.1086/373899}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2003ApJ...588..128P&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Giommi:2005b, + author = {{Giommi}, P. and {Piranomonte}, S. and {Perri}, M. and {Padovani},P. + }, + title = "{The sedentary survey of extreme high energy peaked BL Lacs}", + journal = {\aap}, + year = 2005, + month = apr, + volume = 434, + pages = {385-396}, + doi = {10.1051/0004-6361:20041789}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005A%26A...434..385G&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Nieppola:2006, + author = {{Nieppola}, E. and {Tornikoski}, M. and {Valtaoja}, E.}, + title = "{Spectral energy distributions of a large sample of BL Lacertae objects}", + journal = {\aap}, + year = 2006, + month = jan, + volume = 445, + pages = {441-450}, + doi = {10.1051/0004-6361:20053316}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2006A%26A...445..441N&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Gould:1965, + author = {{Gould}, R.~J.}, + title = "{High-Energy Photons from the Compton-Synchrotron Process in the Crab Nebula}", + journal = {\prl}, + year = 1965, + month = oct, + volume = 15, + pages = {577-579}, + doi = {10.1103/PhysRevLett.15.577}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1965PhRvL..15..577G&db_key=PHY}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Lamb:1997, + author = {{Lamb}, R.~C. and {Macomb}, D.~J.}, + title = "{Point Sources of GeV Gamma Rays}", + journal = {\apj}, + year = 1997, + month = oct, + volume = 488, + pages = {872-+}, + doi = {10.1086/304736}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997ApJ...488..872L&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Buckley:1998, + author = {{Buckley}, J.~H.}, + title = "{ASTROPHYSICS: What the Wild Things Are}", + journal = {Science}, + year = 1998, + month = jan, + volume = 279, + pages = {676-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998Sci...279..676B&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{Dermer:1994, + author = {Dermer, C.~D.}, +booktitle = "{NATO Advanced Study Institute: The Gamma-Ray Sky}", + year = 1994, +publisher = {Dodrecht: Kluwer Academic}, + pages = {39} +} + +@ARTICLE{Rees:1966, + author = {{Rees}, M.~J.}, + title = "{Appearance of Relativistically Expanding Radio Sources}", + journal = {\nat}, + year = 1966, + volume = 211, + pages = {468-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1966Natur.211..468R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{Rees:1966b, + author = {{Rees}, M.~J. and {Sciama}, D.~W.}, + title = "{Inverse Compton Effect in Quasars}", + journal = {\nat}, + year = 1966, + volume = 211, + pages = {805-+}, + adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1966Natur.211..805R&db_key=AST}, + adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} +} + +@ARTICLE{n/a, + author = {n/a}, + title = {n/a}, + journal = {n/a}, + year = 0 +} + +---------------------------------------------------------------------------------- + +\bibitem{Magic-PMT} +A.~Ostankov et~al., +\newblock {\em A study of the new hemispherical 6-dynodes PMT from electron + tubes}, +\newblock Nucl. Instrum. Meth. {\bf A442} (2000) 117. + +\bibitem{MAGIC-analog-link-2} +E.~Lorenz et~al., +\newblock {\em A fast, large dynamic range analog signal transfer system based + on optical fibers}, +\newblock Nucl. Instrum. Meth. {\bf A461} (2001) 517. + +\bibitem{Magic-DAQ} +J.~Cortina et~al. (MAGIC Collab.), +\newblock {\em The data acquisition of the MAGIC telescope}, +\newblock Prepared for International Symposium: The Universe Viewed in Gamma + Rays, Kashiwa, Chiba, Japan, 25-28 Sep 2002. + +\bibitem{MAGIC-design} +J.~A. Barrio, \ et~al. (MAGIC Collab.), +\newblock {\em The MAGIC Telescope -- Design Study for the Construction of a + 17\,m Cherenkov Telescope for Gamma Astronomy above 10\,GeV}, +\newblock (1998), MPI-PhE 98-05. + +\bibitem{MAGIC-calibration} +T.~Schweizer et~al., +\newblock {\em The optical calibration of the MAGIC telescope camera}, +\newblock IEEE Trans. Nucl. Sci. {\bf 49} (2002) 2497. + +\bibitem{MC_timing_Indians} +V.~R. {Chitnis} and P.~N. {Bhat}, +\newblock {\em {Possible discrimination between gamma rays and hadrons using + {\v C}erenkov photon timing measurements}}, +\newblock Astroparticle Physics {\bf 15} (2001) 29. + +----------------------------------------------------------------------------------- Index: /trunk/Dwarf/Documents/ICRC2007/icrc0974.def =================================================================== --- /trunk/Dwarf/Documents/ICRC2007/icrc0974.def (revision 8596) +++ /trunk/Dwarf/Documents/ICRC2007/icrc0974.def (revision 8596) @@ -0,0 +1,116 @@ +\def\aj{AJ}% + % Astronomical Journal +\def\actaa{Acta Astron.}% + % Acta Astronomica +\def\araa{ARA\&A}% + % Annual Review of Astron and Astrophys +\def\apj{ApJ}% + % Astrophysical Journal +\def\apjl{ApJ}% + % Astrophysical Journal, Letters +\def\apjs{ApJS}% + % Astrophysical Journal, Supplement +\def\ao{Appl.~Opt.}% + % Applied Optics +\def\apss{Ap\&SS}% + % Astrophysics and Space Science +\def\aap{A\&A}% + % Astronomy and Astrophysics +\def\aapr{A\&A~Rev.}% + % Astronomy and Astrophysics Reviews +\def\aaps{A\&AS}% + % Astronomy and Astrophysics, Supplement +\def\azh{AZh}% + % Astronomicheskii Zhurnal +\def\baas{BAAS}% + % Bulletin of the AAS +\def\bac{Bull. astr. Inst. Czechosl.}% + % Bulletin of the Astronomical Institutes of Czechoslovakia +\def\caa{Chinese Astron. Astrophys.}% + % Chinese Astronomy and Astrophysics +\def\cjaa{Chinese J. Astron. Astrophys.}% + % Chinese Journal of Astronomy and Astrophysics +\def\icarus{Icarus}% + % Icarus +\def\jcap{J. Cosmology Astropart. Phys.}% + % Journal of Cosmology and Astroparticle Physics +\def\jrasc{JRASC}% + % Journal of the RAS of Canada +\def\mnras{MNRAS}% + % Monthly Notices of the RAS +\def\memras{MmRAS}% + % Memoirs of the RAS +\def\na{New A}% + % New Astronomy +\def\nar{New A Rev.}% + % New Astronomy Review +\def\pasa{PASA}% + % Publications of the Astron. Soc. of Australia +\def\pra{Phys.~Rev.~A}% + % Physical Review A: General Physics +\def\prb{Phys.~Rev.~B}% + % Physical Review B: Solid State +\def\prc{Phys.~Rev.~C}% + % Physical Review C +\def\prd{Phys.~Rev.~D}% + % Physical Review D +\def\pre{Phys.~Rev.~E}% + % Physical Review E +\def\prl{Phys.~Rev.~Lett.}% + % Physical Review Letters +\def\pasp{PASP}% + % Publications of the ASP +\def\pasj{PASJ}% + % Publications of the ASJ +\def\qjras{QJRAS}% + % Quarterly Journal of the RAS +\def\rmxaa{Rev. Mexicana Astron. Astrofis.}% + % Revista Mexicana de Astronomia y Astrofisica +\def\skytel{S\&T}% + % Sky and Telescope +\def\solphys{Sol.~Phys.}% + % Solar Physics +\def\sovast{Soviet~Ast.}% + % Soviet Astronomy +\def\ssr{Space~Sci.~Rev.}% + % Space Science Reviews +\def\zap{ZAp}% + % Zeitschrift fuer Astrophysik +\def\nat{Nature}% + % Nature +\def\iaucirc{IAU~Circ.}% + % IAU Cirulars +\def\aplett{Astrophys.~Lett.}% + % Astrophysics Letters +\def\apspr{Astrophys.~Space~Phys.~Res.}% + % Astrophysics Space Physics Research +\def\bain{Bull.~Astron.~Inst.~Netherlands}% + % Bulletin Astronomical Institute of the Netherlands +\def\fcp{Fund.~Cosmic~Phys.}% + % Fundamental Cosmic Physics +\def\gca{Geochim.~Cosmochim.~Acta}% + % Geochimica Cosmochimica Acta +\def\grl{Geophys.~Res.~Lett.}% + % Geophysics Research Letters +\def\jcp{J.~Chem.~Phys.}% + % Journal of Chemical Physics +\def\jgr{J.~Geophys.~Res.}% + % Journal of Geophysics Research +\def\jqsrt{J.~Quant.~Spec.~Radiat.~Transf.}% + % Journal of Quantitiative Spectroscopy and Radiative Trasfer +\def\memsai{Mem.~Soc.~Astron.~Italiana}% + % Mem. Societa Astronomica Italiana +\def\nphysa{Nucl.~Phys.~A}% + % Nuclear Physics A +\def\physrep{Phys.~Rep.}% + % Physics Reports +\def\physscr{Phys.~Scr}% + % Physica Scripta +\def\planss{Planet.~Space~Sci.}% + % Planetary Space Science +\def\procspie{Proc.~SPIE}% + % Proceedings of the SPIE +\let\astap=\aap +\let\apjlett=\apjl +\let\apjsupp=\apjs +\let\applopt=\ao Index: /trunk/Dwarf/Documents/ICRC2007/icrc0974.tex =================================================================== --- /trunk/Dwarf/Documents/ICRC2007/icrc0974.tex (revision 8596) +++ /trunk/Dwarf/Documents/ICRC2007/icrc0974.tex (revision 8596) @@ -0,0 +1,312 @@ +%% +% International Cosmic Ray Conference 2007 Merida Yucatan Mexico +%% + +%Class Requeried +\documentclass[dvips,openbib]{article} +%The ICRC Style +\usepackage{icrctc07} + +%The paper title +\title{Long-term VHE $\gamma$-ray monitoring of bright blazars with a dedicated Cherenkov telescope} +%Short title to print in the headers to the final publication (Not showed in this print). +\shorttitle{Blazar monitoring with a dedicated IACT} +%All paper authors +\authors{T.~Bretz$^{1}$, M.~Backes$^{2}$, W.~Rhode$^{2}$, K.~Mannheim$^{1}$, J.~Becker$^{2}$, D.~Dorner$^{1}$, T.~Kneiske$^{2}$, M.~Meyer$^{1}$.} +%Short title to print in the headers to the final puplication (Not showed in this print). +\shortauthors{T. Bretz and M. Backes and et al} +%All the affiliations. +\afiliations{$^1$Universit\"{a}t W\"{u}rzburg, Am Hubland, 97074 W\"{u}rzburg, Germany\\ +$^2$Universit\"{a}t Dortmund, Otto-Hahn-Stra{\ss}e 4, 44227 Dortmund, Germany} +\email{tbretz@astro.uni-wuerzburg.de} + +%The abstract. +\abstract{High-peaked BL Lacertae objects are a prime source +population for studies with Cherenkov telescopes. It is obvious that +monitoring observations of strong blazars are orthogonal to the mission +of the larger Cherenkov telescopes, as H.E.S.S. and MAGIC with their +discovery potential for new sources (luminosity function, redshift +distribution). We propose to set up a Cherenkov telescope with low-cost +but high performance design for robotic operation. The goal is to +achieve long-term monitoring of bright blazars which will unravel the +origin and nature of their variability. The telescope design is based +on a technological upgrade of one of the former telescopes of the HEGRA +collaboration on the Canarian Island La Palma (Spain). A first study +is presented.} + +%%%%%%%%%%%%%%%%%%%% B E G I N D O C U M E N T%%%%%%%%%%%%%%%%%%%%%%% +\begin{document} + +\input icrc0974.def + +\maketitle +%Begin the section. + +\paragraph{Introduction} + +Since \cite{Chandrasekhar:1931} the termination of the HEGRA observations, the succeeding +experiments MAGIC and H.E.S.S.\ have impressively extended the physical +scope of gamma ray observations by detecting tens of formerly unknown +gamma ray sources and analyzing their energy spectra and temporal +behavior. This became possible by lowering the energy threshold from +700 GeV to less than 100 GeV and increasing at the same time the +sensitivity by a factor of five. + +To fully exploit the discovery potential of the improved sensitivity, +the discovery of new, faint objects has become the major task for the +new telescopes. A diversity of astrophysical source types such as +pulsar wind nebulae, supernova remnants, microquasars, pulsars, radio +galaxies, clusters of galaxies, gamma ray bursts, and blazars can be +studied with these telescopes and limits their availability for +monitoring purposes of well-known bright sources. + +But there are strong reasons to make an effort for the continuous +monitoring of the few exceptionally bright blazars. This can be +achieved by operating a dedicated monitoring telescope of the +HEGRA-type, referred to in the following as DWARF (Dedicated +multiWavelength Agn Research Facility). The reasons are outlined in +detail below. + +\paragraph{Science case} +The variability of blazars, seen across the entire electromagnetic +spectrum, arises from the dynamics of relativistic jets and the +particle acceleration going on in them. The jets are launched in the +vicinity of accreting supermassive black holes. Theoretical models +predict variability arising from the interplay between jet expansion, +particle injection, acceleration and cooling. + +Long-term monitor observations of bright blazars are the key to obtain +a solid data base for variability investigations. + +An understanding of this variability will deepen our knowledge about +\begin{itemize} +\item the composition and generation of the jets, intimately connected +to the physics of the ergosphere of rapidly spinning black holes +embedded into the hot plasma from the accretion flow. +\item the plasma physics responsible for highly efficient particle +acceleration, bearing similarities to plasma physics of the interaction +between extremely intense laser beams and matter. +\item the orbital modulation of jets due to binary black holes +expected from galaxy merger models. +\end{itemize} +Assuming conservatively the performance of a single HEGRA-type telescope, +long-term monitoring of at least the following blazars is possible: +Mrk421, Mrk501, 1ES\,2344+514, 1ES\,1959+650, H\,1426+428, PKS\,2155-304. +We emphasize that DWARF will run as a facility dedicated to these +targets only, providing a maximum observation time for the program. +\begin{itemize} +\item Flux variations will be determined and compared with variability +properties in other wavelength ranges. +\item Hadronic emission processes and possible coincidences between +VHE-gamma and neutrino-emission will be investigated. +\item The search for signatures of binary black hole systems from +orbital modulation of VHE gamma ray emission will be performed. +\end{itemize} +Furthermore, we seek to obtain know-how for the operation of future +networks of Cherenkov telescopes (e.g. a monitoring array around the +globe or CTA) or telescopes at inaccessible sites. + +At least one of the proposed targets will be visible any time of the +year. For calibration purposes, some time will be scheduled for +observations of the Crab nebula, which is the brightest known VHE +emitter with constant flux. + +In detail the following investigations are planned: +\begin{itemize} +\item As a direct result of the measurements, the duty cycle, the +baseline emission, and the power spectrum of flux variations will be +determined and compared with variability properties in other wavelength +ranges. +\item The lightcurves will be interpreted using models for the +nonthermal emission from relativistically expanding plasma jets. +\item The black hole mass and accretion rate will be determined from +the emission models. Estimates of the black hole mass from emission +models, a possible orbital modulation, and the Magorrian relation +(relating the black hole mass with the stellar bulge mass of the host +galaxy) will be compared. +\item When flaring states will be discovered during the monitor +program, MAGIC will issue a Target of Opportunity observation to obtain +better time resolution. +\item Correlating the arrival times of neutrinos detected by the +neutrino telescope IceCube with simultaneous measurements of DWARF will +allow to test the hypothesis that flares in blazar jets are connected +to hadronic emission processes and thus to neutrino emission from these +sources. The investigation proposed here is complete for both neutrino +and gamma observations, and can therefore lead to conclusive results. +\item The diffuse flux of escaping UHE cosmic rays obtained from +AUGER or flux limits of neutrinos from IceCube, respectively, will be +used to constrain models of UHE cosmic ray origin and large-scale +magnetic fields. +\item Multi-frequency observations together with the Metsähovi Radio +Observatory and the optical Tuorla Observatory are planned. The +measurements will be correlated with INTEGRAL and GLAST results, when +available. X-ray monitoring using the SWIFT and Suzaku facilities will +be proposed. +\item The most ambitious scientific goal of this proposal is the search +for signatures of binary black hole systems from orbital modulation of +VHE gamma ray emission. In case of a confirmation of the present hints +in the temporal behaviour of Mrk501, gravitational wave templates could +be computed with high accuracy to establish their discovery with LISA. +\end{itemize} + +\paragraph{Technical setup} + +At the Observatorio del Roque de los Muchachos (ORM), at the MAGIC site, the +mount of the former HEGRA telescope CT3 now owned by the MAGIC +collaboration is still operational. +Basic support from the shift crew of MAGIC is guaranteed, although +robotic operation is the primary goal. Robotic operation is necessary +to reduce costs and man power demands. Furthermore, we seek to obtain +know-how for the operation of future networks of Cherenkov telescopes. +>From the experience with the construction and operation of MAGIC or +HEGRA, respectively, the proposing groups consider the planned focused +approach (small number of experienced scientists) as optimal for +achieving the project goals. The available automatic analysis package +developed for MAGIC is modular and flexible, and can thus be used with +minor changes for the DWARF project. + +To complete the mount to a functional Cherenkov telescope, the following steps are necessary: + +{\em Camera} For long-term observations stability of the camera is a +major criterion. To keep the systematic errors small good background +estimation is mandatory. The only possibility for a synchronous +determination of the background is the determination from the night-sky +observed in the same field-of-view with the same instrument. To achieve +this the observed position is moved out of the camera center which +allows the estimation of the background from positions symmetric with +respect to the camera center (so called wobble-mode). This observation +mode increases the sensitivity by at least a factor of two because +spending observation for dedicated background observations becomes +obsolete, which also ensures a better time coverage of the observed +sources. Having a camera large enough allowing more than one +independent position for background estimation increases sensitivity +further by better background statistics. This is the case if the source +can be shifted 0.6$^\circ$-0.7$^\circ$ out of the camera center. +To decrease the dependence of the background measurement on the camera +geometry, a camera layout as symmetric as possible will be chosen. +Consequently a camera allowing for wobble-mode observations should be +round and have a diameter of 4.5$^\circ$-5.0$^\circ$ to completely +contain shower images of events in the TeV energy range. To achieve +this requirements a 313 pixel camera can be build +based on the experience with HEGRA and MAGIC. Photomultipliers with a +diameter of 19\,mm and with a quantum efficiency improved by 20\% with +respect to the old CT3 system are considered. + +They ensure a granularity which is enough to guarantee good results +even below the flux peak energy. Each individual pixel has to be +equipped with a preamplifier, an active high-voltage supply and +control. If development of G-APDs ($QE \ge50\%$) will be fast enough, +respectively the price low enough, and their long term stability is +proven well in time, their usage will be considered. For a transition +time one of the old HEGRA cameras might be used. With a special +coating (wavelength shifter) its quantum efficiency might be improved +by ~8$\%$. + +{\em Camera support} The camera chassis must be water tight. An +automatic lid protecting the PMs at day-time will be installed. For +further protection a plexi-glass window will be installed in the front +of the camera. By over-coating the window with an anti-reflex layer of +magnesium-fluoride a gain in transmission of 5$\%$ is expected. Each PM +will be equipped with a light-guide. The current design will be +improved by using a high reflectivity mirror-foil, to reach a +reflectivity in the order of 98$\%$. In total this will gain another ~15$\%$ in +light-collection efficiency compared to the old CT3 system. + +For this setup the camera holding has to be redesigned. An electric and +optical shielding of the individual PMs is planned. + +{\em Data acquisition} For the data acquisition system a low-cost +hardware readout based on an analog ring buffer (Domino II/III), +currently developed for the MAGIC II readout, will be used. +The low power consumption will allow to include the digitization near +the signal source which makes an analog signal transfer obsolete. The +advantage is less pick-up noise and less signal dispersion. By high +sampling rates (0.5\,GHz-1.2\,GHz), additional information about the +pulse shape can be obtained. This increases the over-all sensitivity +further, because the short integration time allows for almost perfect +suppression of noise due to night-sky background photons. The estimated +trigger-rate of the telescope is below 100\,Hz (HEGRA: +$<$10\,Hz) which allows to use a low-cost industrial solution for readout +of the system like USB2.0. As for the HEGRA telescopes, a simple +multiplicity trigger is enough, but also a simple three-next-neighbors +(closed package) could be programmed. +Additional data reduction and preprocessing in the readout hardware or +the readout computer is provided. Assuming conservatively storage of +raw-data at a readout rate of 30\,Hz the storage space needed is less +than 250\,GB/month or 3\,TB/year. + +{\em On-site computing} For on-site computing three standard +PCs are needed. This includes readout and storage, preprocessing, and +telescope control. +The data will be transmitted as soon as possible after data taking via +Internet to the Datacenter in W\"urzburg. Absolute timing necessary for an +accurate source tracking will be achived by a GPS clock. + +{\em Mount and Drive} The present mount is used. Only smaller +changes for safety, corrosion protection, cable ducts, etc. is +needed. For movement motors, shaft encoders and control electronics +have to be bought. The drive system should allow for relatively fast +repositioning for three reasons: +\begin{itemize} +\item Fast movement is in most cases mandatory for future ToO observations. +\item Wobble-mode observations will be done changing the +wobble-position continuously (each 20\,min) for symmetry reasons. +\item To ensure good time coverage of more than one source visible at +the same the observed source will be changed in constant time intervals +($\sim$20min). +\end{itemize} +Therefore three 150\,Watt servo motors are intended. A microcontroller +based motion control unit (SPS) similar to the one of the current MAGIC +II drive system will be used. For communication with the readout-system +a standard Ethernet connection based on the TCP/IP- and UDP-protocol is +applied. + +{\em Mirrors} The existing mirrors are replaced by new plastic mirrors. +The cheap and light-weight material has formerly been used for Winston +cones flown in balloon experiments. The mirrors are copied from a +master, coated with a reflecting and a protective material. +By a change of the mirror geometry the mirror area can be increased +from 8.5\,m$^2$ to 13\,m$^2$; this includes an increase +of $\sim$10$\%$ per mirror by using a hexagonal layout. +To keep track of the alignment, reflectivity and optical quality of the +individual mirrors, and the point-spread function of the total mirror, +during long-term observations the application of an automatic mirror +adjustment system, as successfully operated on the MAGIC telescope, is +intended. + +{\em Pointing calibration} To correct for axis misalignments +a pointing correction algorithm as used in the MAGIC tracking system +will be applied. It is calibrated by measuring the reflection of +bright guide stars on the camera surface and ensures a pointing +accuracy well below the pixel diameter. Therefore a high sensitive +low-cost video camera, as already in operation for MAGIC I and II, will +be installed. + +{\em PM Gain calibration} For the calibration of the PM gain a +calibration system as used for the MAGIC telescope is build. + +\paragraph{Conclusion} +The setup of a small telescope dedicated for long-term AGN monitoring +is easily feasible. Such an activity is motivated by a variety of physical +questions to be answered by the integration of this instrument in +multiwavelength observations. + +\paragraph{Future extensions} +The known duty cycle of 10\% ($\sim$1000h/year) for a Cherenkov +telescope operated at La Palma limits the time-coverage of the +observations. Therefore we propose a worldwide network of ($<10$) small +scale Cherenkov telescopes to be build in the future allowing 24h +monitoring of the bright AGNs. Such a system is so far completely +unique in this energy range. + +\section{Acknowledgements} +We would like to thank Eckart Lorenz, Riccardo Paoletti, Adrian Biland, +Maria Victoria Fonseca and Jos$\acute{e}$ Luis Contreras for intense discussions +and Christian Spiering, Brenda Dingus, Maria Magdalena Gonzalez Sanchez +and the Magic collaboration for helpful support.\\ + +\bibliography{icrc0974} +%This in the bibtex style, is ok. +\bibliographystyle{plain} +References will be added in the final version. +\end{document} Index: /trunk/Dwarf/Documents/ICRC2007/icrctc07.sty =================================================================== --- /trunk/Dwarf/Documents/ICRC2007/icrctc07.sty (revision 8596) +++ /trunk/Dwarf/Documents/ICRC2007/icrctc07.sty (revision 8596) @@ -0,0 +1,159 @@ +% Style to International Cosmic Ray Conference Merida Yucatan Mexico 2007 +% icrctc07.sty LATex 2e Version 1.6 +%% Copyright 2007 by Victor De la Luz +% +% This work may be distributed and/or modified under the +% conditions of the LaTeX Project Public License, either version 1.3 +% of this license or (at your option) any later version. +% The latest version of this license is in +% http://www.latex-project.org/lppl.txt +% and version 1.3 or later is part of all distributions of LaTeX +% version 2003/12/01 or later. +% +% This work has the LPPL maintenance status "maintained". +% +% This Current Maintainer of this work is Victor De la Luz. +% +% +% This work consists of the files icrctc07.sty. +% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% HISTORY: +% Revision: 22/April/2007 +% Revision: 17/April/2007 +% Revision: 9/April/2007 +% Revision: 4/April/2007 +% Revision: 31/March/2007 +% +\NeedsTeXFormat{LaTeX2e} +\ProvidesPackage{icrctc07}[1994/06/01 Standard LaTeX package] +\usepackage{graphicx} +\usepackage{ftnright} +\usepackage{fancyhdr} +\usepackage{times} +\DeclareOption{twoside}{\@twosidetrue} +\ExecuteOptions{twoside} +\twocolumn +%\flushbottom +\sloppy +%Preliminary Declarations +\hoffset 0mm +\voffset 0mm +%tope de impresion 25.4mm +\oddsidemargin -10.4mm %Margen impar +\evensidemargin -10.4mm %Margen par +\textwidth 150mm +%---------------------- +\paperwidth 180mm +\topmargin 2mm +\headheight 4mm +\headsep 5mm +\textheight 210mm +\footskip 8mm +%-------------------- +\paperheight 240mm +\columnsep 8mm +\parskip 1mm +\parindent 0mm +\marginparsep 0mm +\headwidth 150mm +\def\addcontentsline#1#2#3{} +%New declarations to Authors, paperid, etc. +\newcommand{\@authors}{} +\newcommand{\authors}[1]{\renewcommand{\@authors}{#1}} +\newcommand{\@paperid}{} +\newcommand{\paperid}[1]{\renewcommand{\@paperid}{#1}} +\newcommand{\@shorttitle}{} +\newcommand{\shorttitle}[1]{\renewcommand{\@shorttitle}{#1}} +\newcommand{\@shortauthors}{} +\newcommand{\shortauthors}[1]{\renewcommand{\@shortauthors}{#1}} +\newcommand{\@afiliations}{} +\newcommand{\afiliations}[1]{\renewcommand{\@afiliations}{#1}} +\newcommand{\@email}{} +\newcommand{\email}[1]{\renewcommand{\@email}{#1}} +\newcommand{\@abstract}{} +\renewcommand{\abstract}[1]{\renewcommand{\@abstract}{#1}} +%fonts +\def\@normalsize{\@setsize\normalsize{10pt}\xipt\@xipt} % 10 point on 11 +\def\small{\@setsize\small{10pt}\ixpt\@ixpt} % 9 point on 10 +\def\footnotesize{\@setsize\footnotesize{10pt}\ixpt\@ixpt} % 9 point on 10 +\def\scriptsize{\@setsize\scriptsize{8pt}\viipt\@viipt} % 7 point on 8 +\def\tiny{\@setsize\tiny{7pt}\vipt\@vipt} % 6 point on 7 +\def\large{\@setsize\large{12pt}\xipt\@xipt} % 11 point on 12 +\def\Large{\@setsize\Large{14pt}\xiipt\@xiipt} % 12 point on 14 +\def\LARGE{\@setsize\LARGE{16pt}\xivpt\@xivpt} % 14 point on 16 +\def\huge{\@setsize\huge{20pt}\xviipt\@xviipt} % 17 point on 20 +\def\Huge{\@setsize\Huge{23pt}\xxpt\@xxpt} % 20 point on 23 +%The logoblack.eps source +\newcommand{\@logosource}{logoblack} +\DeclareOption{black}{\gdef\@logosource{logoblack}} +\newcommand{\logosource}[1]{\gdef\@logosource{#1}} +\newlength{\@line} +\setlength{\@line}{12pt} +\pagestyle{fancyplain} +%special Headings +\lhead[\small \sc \@shorttitle \hfill]{} +\rhead[]{\small \sc30th International Cosmic Ray Conference\hfill} +%don't work! 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+UArXAJcC<$JcD_LJ,~> +UArXAJcC<$JcD_LJ,~> +UArXAJcC<$JcD_LJ,~> +Sc@IFJcC<$JcDPGJ,~> +Sc@IFJcC<$JcDPGJ,~> +Sc@IFJcC<$JcDPGJ,~> +PlL.OJcC<$JcD5>J,~> +PlL.OJcC<$JcD5>J,~> +PlL.OJcC<$JcD5>J,~> +%%EndData +showpage +%%Trailer +end +%%EOF Index: /trunk/Dwarf/Documents/macros/sensitivity.C =================================================================== --- /trunk/Dwarf/Documents/macros/sensitivity.C (revision 8596) +++ /trunk/Dwarf/Documents/macros/sensitivity.C (revision 8596) @@ -0,0 +1,156 @@ +sensitivity(){ +TGraph dwarf; +dwarf.SetName("DWARF"); +dwarf.SetTitle("Differential Flux Sensitivity"); +TLegend leg(0.75, 0.75, 0.95, 0.95); //x1, y1, x2, y2 in % +//dwarf.SetPoint(dwarf.GetN()+1, x1, y1); +//dwarf.SetPoint(dwarf.GetN()+1, x2, y2); +dwarf.SetPoint(dwarf.GetN(), 0.001, 6E-12); +dwarf.SetPoint(dwarf.GetN(), 0.25, 6E-12); +dwarf.SetPoint(dwarf.GetN(), 0.31, 4.38E-12); +dwarf.SetPoint(dwarf.GetN(), 0.39, 2.1E-12); +dwarf.SetPoint(dwarf.GetN(), 0.45, 1.54E-12); +dwarf.SetPoint(dwarf.GetN(), 0.5, 1.4E-12); +dwarf.SetPoint(dwarf.GetN(), 1, 7.5E-13); +dwarf.SetPoint(dwarf.GetN(), 10, 2.25E-13); +dwarf.SetPoint(dwarf.GetN(), 50, 3.13E-13); +dwarf.SetLineColor(kBlue); +dwarf.SetLineWidth(5); + +TGraph *gclone = dwarf.DrawClone("AC"); + +TH1 *h = gclone->GetHistogram(); + +TAxis *axex = h->GetXaxis(); +TAxis *axey = h->GetYaxis(); +//axex->SetLabelOffset(x); +//axey->SetLabelOffset(y); +//axex->SetLabelSize(x); +//axey->SetLabelSize(y); +axex->SetTitleOffset(1.30); +axey->SetTitleOffset(1.2); +//axex->SetTitleSize(x); +//axey->SetTitleSize(y); + +axex->SetMoreLogLabels(); +//axey->SetMoreLogLabels(); + +axex->SetTitle("E_0 [TeV]"); +axey->SetTitle("F(ESetRangeUser(0.005, 100); +axey->SetRangeUser(1E-13, 2E-10); +gclone->RemovePoint(0); +leg.AddEntry("DWARF", "DWARF", "l"); + + +TGraph hegras; +hegras.SetName("HEGRAS"); +hegras.SetPoint(hegras.GetN(), 0.5, 1.7E-12); +hegras.SetPoint(hegras.GetN(), 1, 1E-12); +hegras.SetPoint(hegras.GetN(), 10, 2.5E-13); +hegras.SetPoint(hegras.GetN(), 50, 2.5E-13); +hegras.SetLineColor(kGreen); +hegras.SetLineWidth(5); +hegras.DrawClone("C"); +leg.AddEntry("HEGRAS", "HEGRA CT System", "l"); + +//TGraph hegra2; +//hegra.SetName("HEGRA2"); +//hegra2.SetPoint(hegra2.GetN(), 0.4, 1.7E-12); //1.2E-12 +//hegra2.SetLineColor(kBlue); +//hegra2.SetMarkerStyle(kFullDotMedium); +//hegra2.DrawClone("P"); +//leg.AddEntry("HEGRA2", "HEGRA CT System 2", "p"); + +TF1* pow2=new TF1("pow2","1.7e-12/pow(0.4,-0.73)*pow(x,-0.73)",0.4,7); +pow2->SetLineColor(kGreen); +pow2->SetLineStyle(kDashed); +pow2->Draw("same"); +leg.AddEntry("pow2", "HEGRA CT System 2", "l"); + +//TGraph hegra; +//hegra.SetName("HEGRA"); +//hegra.SetPoint(hegra.GetN(), 0.75, 7.1E-12); //1E-11 +//hegra.SetLineColor(kBlue); +//hegra.SetMarkerStyle(kFullDotMedium); +//hegra.SetMarkerSize(5); +//hegra.DrawClone("P"); +//leg.AddEntry("HEGRA", "1 HEGRA CT", "p"); + +TF1* pow3=new TF1("pow3","7.1e-12/pow(0.75,-0.73)*pow(x,-0.73)",0.75,7); +pow3->SetLineColor(kBlue); +pow3->SetLineStyle(kDashed); +pow3->Draw("same"); +leg.AddEntry("pow3", "1 single HEGRA CT", "l"); + +TGraph whipple; +whipple.SetName("Whipple"); +whipple.SetPoint(whipple.GetN(), 0.25, 1E-11); +whipple.SetPoint(whipple.GetN(), 1, 2.7E-12); +whipple.SetPoint(whipple.GetN(), 3, 1E-12); +whipple.SetPoint(whipple.GetN(), 10, 1E-12); +whipple.SetLineColor(kRed); +whipple.SetLineWidth(5); +whipple.DrawClone("C"); +leg.AddEntry("Whipple", "Whipple", "l"); + +//TGraph whipple2; +//whipple2.SetName("Whipple2"); +//whipple2.SetPoint(whipple2.GetN(), 0.3, 9.2E-12); //1.3E-11 +//whipple2.SetLineColor(kBlue); +//whipple2.SetMarkerStyle(kFullDotMedium); +//whipple2.DrawClone("P"); +//leg.AddEntry("Whipple2", "Whipple2", "p"); + +TF1* pow1=new TF1("pow1","1.3e-11/pow(0.3,-0.95)*pow(x,-0.95)",0.3,3.5); +pow1->SetLineColor(kRed); +pow1->SetLineStyle(kDashed); +pow1->Draw("same"); +leg.AddEntry("pow1", "Whipple 2", "l"); + +TGraph magic_loi; +magic_loi.SetName("magic_loi"); +magic_loi.SetPoint(magic_loi.GetN(), 0.01, 1E-10); +magic_loi.SetPoint(magic_loi.GetN(), 0.045, 1E-11); +magic_loi.SetPoint(magic_loi.GetN(), 0.095, 4.5E-12); +magic_loi.SetPoint(magic_loi.GetN(), 0.55, 1E-12); +magic_loi.SetPoint(magic_loi.GetN(), 1, 6E-13); +magic_loi.SetLineColor(kCyan); +magic_loi.SetLineWidth(5); +magic_loi.SetLineStyle(kDashed); +magic_loi.DrawClone("C"); +leg.AddEntry("magic_loi", "MAGIC LoI", "l"); + +TGraph magic; +magic.SetName("magic"); +magic.SetPoint(magic.GetN(), 0.036, 1.2E-10); +magic.SetPoint(magic.GetN(), 0.045, 8E-11); +magic.SetPoint(magic.GetN(), 0.063, 5E-11); +magic.SetPoint(magic.GetN(), 0.095, 2.3E-11); +magic.SetPoint(magic.GetN(), 0.12, 1.3E-11); +magic.SetPoint(magic.GetN(), 0.15, 7E-12); +magic.SetPoint(magic.GetN(), 0.18, 5E-12); +magic.SetPoint(magic.GetN(), 0.25, 3E-12); +magic.SetPoint(magic.GetN(), 0.31, 2.5E-12); +magic.SetPoint(magic.GetN(), 0.45, 1.1E-12); +magic.SetPoint(magic.GetN(), 0.5, 1.05E-12); +magic.SetPoint(magic.GetN(), 0.6, 9E-13); +magic.SetPoint(magic.GetN(), 0.8, 6E-13); +magic.SetPoint(magic.GetN(), 0.9, 6E-13); +magic.SetPoint(magic.GetN(), 1, 4E-13); +magic.SetLineColor(kCyan); +magic.SetLineWidth(5); +magic.DrawClone("C"); +leg.AddEntry("magic", "MAGIC", "l"); + +leg.DrawClone(); +gPad->SetGridx(); +gPad->SetGridx(); +gPad->SetLogx(); +gPad->SetLogy(); +gPad->SetFillColor(kWhite); +gPad->SetBottomMargin(0.13); +gPad->SetLeftMargin(0.11); + +}