Swift follow-up confirms the high flaring state of the blazar PMN J2345-1555

Details Swift follow-up confirms the high flaring state of the blazar PMN J2345-1555 Swift follow-up confirms the high flaring state of the blazar PMN J2345-1555

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2986....1k&link_type=abstract

The Astronomer's Telegram, #2986

Astronomy and Astrophysics

Astronomy

Ultra-Violet, X-Ray, Gamma Ray, >Gev, Tev, Vhe, Blazar, Transient

Scientific paper

Following the detection on 24 October 2010 of simultaneous optical and gamma-ray flares from the intermediate redshift (z=0.621) flat spectrum radio quasar PMN J2345-1555 by ATOM and Fermi LAT (ATel #2972), Swift target of opportunity observations have been performed on 27/28 October. Swift/XRT data were taken in Photon Counting mode for a total exposure of 9.7 ks. The X-ray spectrum (0.3-10 keV) can be fit by an absorbed power law model with a HI column density consistent with the Galactic value in the direction of the source.

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