Changeset 6864


Ignore:
Timestamp:
03/20/05 21:10:15 (20 years ago)
Author:
hbartko
Message:
*** empty log message ***
Location:
trunk/MagicSoft/GC-Proposal
Files:
2 edited

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  • trunk/MagicSoft/GC-Proposal/Changelog

    r6862 r6864  
     12005/03/20 Hendrik
     2* further corrections
     3
    142005/03/20 Sebastian
    25* Made some small corrections

  • trunk/MagicSoft/GC-Proposal/GC.tex

    r6863 r6864  
    140140\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}
    141141
    142 At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS, \cite{GC_whipple,
     142At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS \cite{GC_whipple,
    143143GC_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
    144144different reconstructed positions of the GC source. Recently a second TeV
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