Fermi LAT detection of a GeV flare from B2 0619+33

Details Fermi LAT detection of a GeV flare from B2 0619+33 Fermi LAT detection of a GeV flare from B2 0619+33

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2829....1c&link_type=abstract

The Astronomer's Telegram, #2829

Astronomy and Astrophysics

Astronomy

Gamma Ray, >Gev, Request For Observations, Transients

Scientific paper

The Large Area Telescope (LAT), one of the two instruments on board the Fermi Gamma-ray Space Telescope, has observed an increased gamma-ray flux from a source positionally consistent with the radio source B2 0619+33/VCS J0622+3326 (RA: 06h22m52.221945s, Dec: +33d26m10.41027s, J2000; Kovalev et al. 2007, AJ 133, 1236). The source was detected in a high state September 1-4, 2010. Preliminary analysis indicates that on September 3, 2010 the flare reached a peak gamma-ray flux (E>100MeV) of 1.0 ±0.2*10-6 photons cm-2 s-1 (errors are statistical only).

Affiliated with

Also associated with

No associations

Rating

Fermi LAT detection of a GeV flare from B2 0619+33 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Fermi LAT detection of a GeV flare from B2 0619+33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fermi LAT detection of a GeV flare from B2 0619+33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-773757