Changeset 6864 for trunk/MagicSoft/GC-Proposal
- Timestamp:
- 03/20/05 21:10:15 (20 years ago)
- Location:
- trunk/MagicSoft/GC-Proposal
- Files:
-
- 2 edited
Legend:
- Unmodified
- Added
- Removed
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trunk/MagicSoft/GC-Proposal/Changelog
r6862 r6864 1 2005/03/20 Hendrik 2 * further corrections 3 1 4 2005/03/20 Sebastian 2 5 * Made some small corrections -
trunk/MagicSoft/GC-Proposal/GC.tex
r6863 r6864 140 140 \cite{Hooper2002} indicates a point source whose position is different from the GC at a confidence level beyond 99.9 \%. %\cite{Hooper2002, A&A 335 (1998) 161} 141 141 142 At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS ,\cite{GC_whipple,142 At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS \cite{GC_whipple, 143 143 GC_cangaroo,GC_hess}. The spectra as measured by these experiments are displayed in Figure \ref{fig:GC_gamma_flux} while Figure \ref{fig:GC_source_location} shows the 144 144 different reconstructed positions of the GC source. Recently a second TeV
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