Changeset 6219 for trunk/MagicSoft


Ignore:
Timestamp:
02/03/05 09:05:02 (20 years ago)
Author:
gaug
Message:
*** empty log message ***
Location:
trunk/MagicSoft/GRB-Proposal
Files:
3 edited

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  • trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex

    r6218 r6219  
    121121Hartmann D.H., Kneiske T.M., Mannheim K.,Watanabe K., AIP Conference Proceedings, 662, 442, 2003.
    122122\bibitem{MANNHEIM} Mannheim K., Hartmann D., Burkhardt F., AsJ, 467, 532, 1996.
    123 \bibitem{SALOMON} Absorption of HE Gamma Rays by Interactions with Extragalactic Starlight Photons at High Redshifts and the HE Gamma-Ray Background, Salomon M.H., Stecker F.J., ApJ, 493, 547, 1998.
    124123\bibitem{DERMER} Beaming, Baryon loading, and the Synchrotron Self-Compton Component in Gamma-Ray Bursts,
    125124Dermer \& Chiang, ApJ, 537, 785, 2000.
    … …  
    177176
    178177\bibitem{KNEISKE} Kneiske T.M., Bretz T., Mannheim K., Hartmann D.H., A\&A 413, 807, 2004.
     178\bibitem{SALOMON} Absorption of HE Gamma Rays by Interactions with Extragalactic Starlight Photons at High Redshifts and the HE Gamma-Ray Background, Salomon M.H., Stecker F.J., ApJ, 493, 547, 1998.
    179179\bibitem{GRB030329} Spectra of the burst: http://space.mit.edu/HETE/Bursts/GRB030329/
    180180\bibitem{ecl} Private communication with Lorenz E.

  • trunk/MagicSoft/GRB-Proposal/Introduction.tex

    r6213 r6219  
    77the objective to turn the telescope to the burst position within 10-30\,sec.
    88in order to have a fair chance to detect a burst when the prompt $\gamma$--emission is still ongoing.
    9 During the commissioning phase it could be proven that our goal was reached.
    10 The telescope is able to turn 180 degrees in azimuth within 20\,sec. and 80 degrees in zenith within 10\,sec.\\
    11 
     9During the commissioning phase, it could be proven that our goal was reached.
     10The telescope is able to turn 180\,deg. in azimuth within 20\,sec. and 90\,deg. in zenith within 10\,sec.\\
    1211
    1312Very high energy (VHE) GRB observations have the potential to constrain the current GRB models
    14 on both the prompt and extended phases of GRB emission~\cite{HARTMANN,MANNHEIM,SALOMON}.
    15 Models based on both internal and external shocks predicts VHE fluence comparable to,
     13on both the prompt and extended phases of GRB emission~\cite{HARTMANN,MANNHEIM}.
     14Models based on both internal and external shocks predict VHE gamma-ray fluences comparable to,
    1615or in certain situations stronger than, the keV-MeV radiation,
    17 with duration ranging from shorter than the keV-MeV burst to extended TeV afterglows~\cite{DERMER, PILLA, ZHANG1, RAZZAQUE}.
     16with durations ranging from shorter than the keV-MeV burst to extended TeV
     17afterglows~\cite{DERMER, PILLA, ZHANG1, RAZZAQUE}.
    1818
    1919\par
    … …  
    7272
    7373
     74
     75%%% Local Variables:
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     77%%% TeX-master: "GRB_proposal_2005"
     78%%% End:

  • trunk/MagicSoft/GRB-Proposal/Strategies.tex

    r6165 r6219  
    7373
    7474We determine the maximum zenith angle for GRB observations by requiring that the overwhelming majority of possible GRBs will have an in principle observable spectrum. Figure~\ref{fig:grh}
    75 shows the gamma-ray horizon (GRH) as computed in~\cite{KNEISKE}. The GRH is defined as the
     75shows the gamma-ray horizon (GRH) as computed in~\cite{KNEISKE,SALOMON}. The GRH is defined as the
    7676gamma-ray energy at which a part of $1/e$ of a hypothesied mono-energetic flux gets absorbed after
    7777travelling a distance of $d$, expressed in redshift $z$ from the earth. One can see that at typical
    … …  
    113113\item In the other case for having off-data at exactly the same sky location.
    114114\end{itemize}
     115
     116%%% Local Variables:
     117%%% mode: latex
     118%%% TeX-master: "GRB_proposal_2005"
     119%%% End:
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