Search for diffuse gamma rays from the Galactic anticentre region above 100 GeV with CELESTE

R. J. Britto; A. Jacholkowska; F. Piron; E. Brion; J. Bussons Gordo; G. Debiais; B. Fabre; J. Lavalle; F. Munz; E. Nuss; R. C. Rannot; T. Reposeur

doi:10.1051/0004-6361/200811476

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Volume 498 / No 2 (May I 2009)

A&A, 498 2 (2009) L25-L28

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Table 1:

CELESTE sensitivity to the diffuse signal for the spectral models of Eq. (1) and an observation time of 10h, in case of no diffuse signal expected in the OFF₂ region.
$\Gamma$	$n_\gamma$ $({\rm min}^{-1})$	Q	$N_{\sigma}$ for $T_{\rm obs}=10$ h
2.0	$1.45 \pm 0.03$	1.39	0.9
2.5	$0.36 \pm 0.01$	0.96	0.2

Source LaTeX | All tables | In the text

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