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01/28/05 18:58:51 (20 years ago)
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gaug
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  • trunk/MagicSoft/GRB-Proposal/Strategies.tex

    r6101 r6105  
    7676We determine the maximum zenith angle by requiring that the overwhelming majority of
    7777possible GRBs will yield an in principle observable spectrum. Figure~\ref{fig:grh}
     78shows the gamma-ray horizon (GRH) as computed in~\cite{KNEISKE}. The GRH is defined as the
     79gamma-ray energy at which a part of $1/e$ of a hypothiszed mono-energetic flux is absorbed after
     80travelling a distance of $d$, expressed in redshift $z$ from the earth. One can see that at typical
     81GRB distances of $z=1$, all gamma-rays above 100\,GeV get absorbed before they reach the earth.
     82\par
     83Even the closest GRB with known redshift ever observed, GRB030329~\cite{GRB030329}, lies at a redshift
     84of $z=0.1685$. In this case, gamma-rays above 200\,GeV get absorbed.
    7885
    79 
    80 \begin{figure}
     86\begin{figure}[htp]
    8187\centering
    82 \includegraphics[width=0.99\linewidth]{f4.eps}
    83 \caption{}
     88\includegraphics[width=0.85\linewidth]{f4.eps}
     89\caption{Gamma Ray Horizon, as derived in~\cite{KNEISKE}}
    8490\label{fig:grh}
    8591\end{figure}
     92
     93\par
     94We assume now an energy threshold of 50\,GeV for MAGIC at a zenith angle of $\theta = 0$. According
     95to~\cite{eckart}, the energy threshold of a Cherenkov telescope scales with zenith angle like:
     96
     97\begin{equation}
     98E^{thr}(\theta) = E^{thr}(0) \cdot \cos(\theta)^{-2.7}
     99\label{eq:ethrvszenith}
     100\end{equation}
     101
     102Eq.~\ref{eq:ethrvszenith} leads to an energy threshold of about 900\,GeV at $\theta = 70^\circ$ and
     103500\,GeV at $\theta = 65^\circ$. Inserting these results into the GRH (figure~\ref{fig:grh}), one gets
     104a maximal observable GRB distance of $z = 0.1$ and $z = 0.2$, respectively. We think that the probability for
     105GRBs to occur at these distances is suffiently small in order to neglect the very difficult observations
     106beyond these limits.
    86107
    87108\subsection{In case of follow-up: Next steps}
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