X-ray Outburst of the blazar, 3C454.3

Details X-ray Outburst of the blazar, 3C454.3 X-ray Outburst of the blazar, 3C454.3

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..484....1r&link_type=abstract

The Astronomer's Telegram, #484

Astronomy and Astrophysics

Astronomy

6

X-Ray, Quasars

Scientific paper

The X-ray light curve of the blazar 3C454.3 was processed from observations with the RXTE All-Sky Monitor, following the report by Balonek (VSNET Alert) of an optical outburst. An X-ray detection is evident when the results are examined on timescales of one week or longer. Over the recent time interval, MJD 53490.0 to 53501.5, the average flux (2-12 keV) is 10.8 (1.7) mCrab, implying that 3C454.3 is currently one of the brightest AGN in the X-ray sky.

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