%0 Unpublished work
%T Galactic diffuse gamma-ray flux at the energy about 175 TeV
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%A Martirosov, Romen M.
%A Ter-Antonyan, Samvel V.
%A Erlykin, Anatoly D.
%A Garyaka, Alexandr P.
%A Nikolskaya, Natalya M.
%A Gallant, Yves
%A Jones, Lawrence W.
%Z Submitted to the 31-th ICRC, Lodz (Pologne) 2009, July 7-15
%Z 09-074
%8 2009-05-30
%D 2009
%Z 0905.3593
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]
%Z Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Preprints, Working Papers, ...
%X We present an upper limit of galactic diffuse gamma-ray flux, measured withthe GAMMA experiment at energy about 175 TeV. The results were obtained usingselection of muon poor extensive air showers at mountain level (700 g/cm^2, Mt.Aragats, Armenia) for 5 GeV muon energy threshold. An upper limit for thedifferential flux at energy E=175+/-25 TeV is equal to (5.8-7.0)x10^-12 [ergm^2 s sr]^-1 for 95% confidence level.
%G English
%L hal-00430142
%U https://hal.science/hal-00430142
%~ IN2P3
%~ LPTA
%~ CNRS
%~ UNIV-MONTP2
%~ UNIV-MONTPELLIER
%~ UM1-UM2