AGILE detection of Cygnus X-3 above 400 MeV

Details AGILE detection of Cygnus X-3 above 400 MeV AGILE detection of Cygnus X-3 above 400 MeV

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3239....1b&link_type=abstract

The Astronomer's Telegram, #3239

Astronomy and Astrophysics

Astronomy

1

X-Ray, Gamma Ray, Binary, Black Hole, Neutron Star, Transient

Scientific paper

The AGILE satellite has been monitoring the Cygnus X-3 region in the spinning mode. The AGILE-GRID detector does not detect significant gamma-ray emission during the period of the Fermi-LAT detection on MJD 55642 (March 22, 2011, ATel #3233). Integrating during the period MJD 55641-55642 (a standard 2-day integration of the AGILE spinning mode) we obtain a 95% confidence level upper limit of 1.1 x 10-6 ph cm-2 s-1 (E > 100 MeV).

Affiliated with

Also associated with

No associations

Rating

AGILE detection of Cygnus X-3 above 400 MeV 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 AGILE detection of Cygnus X-3 above 400 MeV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and AGILE detection of Cygnus X-3 above 400 MeV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-861991