IGR J14536-5522 is identified by Swift

Details IGR J14536-5522 is identified by Swift IGR J14536-5522 is identified by Swift

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..686....1m&link_type=abstract

The Astronomer's Telegram, #686

Astronomy and Astrophysics

Astronomy

4

X-Ray, Cataclysmic Variables

Scientific paper

The BAT survey source Swift J1453.4-5524 is coincident with IGR J14536-5522. This is a relatively soft BAT source (kT~30-45 keV for a single temperature Bremsstrahlung fit) that appears to be variable. In a pointed Swift XRT observation, we find a moderately bright (3.3e-11 ergs/cm^2 s keV in 0.4-10 keV) x-ray source at RA = 14h53m41.7s, dec=-55d21m42.8s, coincident with the ROSAT all sky survey source 1RXS J145341.1-552146.

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