Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare

Details Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2047....1d&link_type=abstract

The Astronomer's Telegram, #2047

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Agn

Scientific paper

Following the extraordinary optical brightness level of the blazar PKS 1510-089 on May 08.9 (Larionov et al., ATel #2045), we report on the analysis of Swift data obtained immediately after the optical flare. The Swift/BAT hard X-ray transient monitor detected an outburst in PKS 1510-089 in the 15-50 keV energy band. On 2009 May 10 (MJD 54961) the count rate was 0.009 +/- 0.005 cts/s/cm^2 (40 mCrab).

Affiliated with

Also associated with

No associations

Rating

Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare 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 Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Swift follow-up observations of the blazar PKS 1510-089 after a high optical flare will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-807022