Changeset 828

Timestamp:

06/01/01 11:00:52 (23 years ago)

Author:

blanch

Message:

Comments from Manel nad Sasha implemented.

File:

• trunk/ICRC_01/mccontrib.tex (modified) (7 diffs)

trunk/ICRC_01/mccontrib.tex

@@ -18 +18 @@
 \affil[3]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany}
 
-\correspondence{O.Blanch blanch@ifae.es), H. Kornmayer (h.kornmayer@web.de)}
+\correspondence{O.Blanch (blanch@ifae.es), H. Kornmayer (h.kornmayer@web.de)}
 \affil[ ]{ }
 \affil[ ]{\large (for the MAGIC Collaboration)}
@@ -129 +129 @@
         $\Theta = 10^\circ$ &  $\approx 5 \cdot 10^5$ & $\approx 1 \cdot 10^6$  \\
         $\Theta = 15^\circ$ &  $\approx 2 \cdot 10^6$    &  $\approx 5 \cdot 10^6$  \\
-        $\Theta = 20^\circ$ &  production   &  production  \\
-        $\Theta = 25^\circ$ &  production   &  production  \\
+        $\Theta = 20^\circ$ &  in production   &  in production  \\
+        $\Theta = 25^\circ$ &  in production   &  in production  \\
     \hline
   \end{tabular}
@@ -233 +233 @@
 These stars will contribute locally to the noise in the 
 camera and have to be taken into account. 
-A program that allows to simulate the star light together 
-with the generated showers has been developed. 
+A program was developed to simulate the star light together 
+with the generated showers. 
 This program considers all stars in the field of view of the camera
 around a chosen direction. The light of these stars is traced up to 
@@ -300 +300 @@
 
  
-\subsubsection{Effective trigger collection area}
-
-
-
-The effective trigger collection area is defined as the integral 
+\subsubsection{Trigger collection area}
+
+
+
+The rigger collection area is defined as the integral 
 \begin{equation} 
   A(E,\Theta)  = \int_{F}{ T(E,\Theta,F) dF}
@@ -313 +313 @@
 for different discriminator thresholds are shown in figure
 \ref{fig_collarea}.
-At low energies ($ E < 100 ~\mathrm{GeV}$), the effective trigger collection 
+At low energies ($ E < 100 ~\mathrm{GeV}$), the trigger collection 
 area decreases with increasing zenith angle , and it decreases with 
 %
@@ -322 +322 @@
  \includegraphics[width=8.3cm]{collarea.eps} % .eps for Latex,
                                             % pdfLatex allows .pdf, .jpg, .png and .tif
- \caption{The effective trigger collection area for gamma showers as a function
+ \caption{The trigger collection area for gamma showers as a function
  of energy $E$.}
  \label{fig_collarea}
@@ -456 +456 @@
 
 \begin{acknowledgements}
-The authors thanks all the "simulators" of the MAGIC collaboration
+The authors thank all the "simulators" of the MAGIC collaboration
 for their support in the production of the big amount of Monte Carlo
-data. The support of MAGIC by the BMBF (Germany) and the CYCIT (Spain) 
-is acknowledged. 
+data. We thank also M. Dosil and D. Petry for writing the Star field 
+adder program. The support of MAGIC by the BMBF (Germany) and the CYCIT 
+(Spain) is acknowledged.