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 hess2004paper.tex, PRL, 2006, accepted
References: <453F1336.5090909@lapp.in2p3.fr> <Pine.LNX.4.64.0610250648570.23482@euro>
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Hi,
Sorry ! I forgot to retype these.. Here are the definitions:
\gr     $\gamma$-ray
\grs    $\gamma$-rays
\GC   GC

Thanks !
Loic


GCNEWS newsletter wrote:

>Hi, 
>
>To properly process your abstract into the newsletter,
>could you give me the definitions for \grs \gr \GC etc?
>Thanks
>Lorant
>
>
>\begin{abstract}
>The detection of \grs\ from the source HESS\,J1745$-$290
>in the Galactic Center (\GC) region with the \hess\ array of Cherenkov
>telescopes in 2004 is presented.
>After subtraction of the diffuse \gr\ emission from the \GC\ ridge,
>the source is compatible with a point-source with spatial extent
>less than $1.2'\mbox{(stat.)}$ (95\% CL).
>The measured energy spectrum above 160~GeV is compatible with
>a power-law with photon index of $2.25 \pm 0.04 \mbox{(stat.)} \pm 0.10
>\mbox{(syst.)}$
>and no significant flux variation is detected.
>These measurements are discussed in the framework of dark matter
>annihilation. It is found that the bulk of the VHE emission must
>have non-dark-matter origin. Loose constraints on the velocity-weighted
>annihilation cross section $\left<\sigma\times v\right>$ are derived
>assuming the presence of an astrophysical non-dark-matter \gr\
>contribution.
>\end{abstract}
>
>  
>

-- 
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|         Loic Rolland           |
|  CNRS/IN2P3/LAPP               |
|  Phone:  +33 (0)4 50 09 16 69  |
|  Fax:    +33 (0)4 50 27 94 95  |
|  e-mail: rollandl@in2p3.fr     |
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