GeV emission from SHBL J001355.9-185406

Details GeV emission from SHBL J001355.9-185406 GeV emission from SHBL J001355.9-185406

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3014....1s&link_type=abstract

The Astronomer's Telegram, #3014

Astronomy and Astrophysics

Astronomy

2

Gamma Ray, >Gev, Tev, Agn

Scientific paper

The Large Area Telescope (LAT), one of the two instruments on the Fermi Gamma-ray Space Telescope, has detected a source positionally consistent with the High energy peaked BL Lac SHBL J001355.9-185406 (R.A: 00:13:56.054 Dec.: -18:54:06.48), recently detected above 300 GeV by the High Energy Stereoscopic System (H.E.S.S., see ATEL # 3007 and references therein).
A preliminary analysis indicates a faint, hard source with a flux, averaged over 2 years of data, above 100 MeV of (0.9 +/- 0.7)x10^9 ph cm^-2 s^-1 and a photon index of 1.5 +/ 0.2 (errors are statistical only).

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