Swift observations of the flaring blazar B3 0650+453

Details Swift observations of the flaring blazar B3 0650+453 Swift observations of the flaring blazar B3 0650+453

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3609....1s&link_type=abstract

The Astronomer's Telegram, #3609

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, X-Ray, Agn, Blazar, Quasar

Scientific paper

Following the reported flaring activity of the flat spectrum radio quasar B3 0650+453 in GeV (ATel #3580) and radio (ATel #3596) bands, Swift observations of the source were performed on 2011 August 27, five days after the peak of the gamma-ray flare.
Swift/XRT data were taken in Photon Counting mode for a net exposure of 5.1 ksec. The X-ray spectrum can be fit by an absorbed power law with the HI column density fixed to the Galactic value of N_HI = 8.72 x 10^20 cm^-2 (Kalberla et al.

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