Swift/BAT detection of IGR J19294+1816

Details Swift/BAT detection of IGR J19294+1816 Swift/BAT detection of IGR J19294+1816

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1999....1k&link_type=abstract

The Astronomer's Telegram, #1999

Astronomy and Astrophysics

Astronomy

2

X-Ray, Black Holes, Neutron Stars, Pulsars, Transients

Scientific paper

Examination of archival data from the Swift/BAT hard X-ray transient monitor reveals that Swift/BAT has detected the newly discovered source IGR J19294+1816 (Turler et al, ATel #1997) several times during the past three years. The detections were 2006-01-13 = MJD 53748: 0.002 ± 0.0003 ct/s/cm^2 (7 mCrab) 2006-11-13 = MJD 54052: 0.001 ± 0.0004 ct/s/cm^2 (6 mCrab) 2007-04-27 = MJD 54217: 0.003 ± 0.0006 ct/s/cm^2 (11 mCrab) 2007-12-15 = MJD 54449: 0.002 ± 0.0004 ct/s/cm^2 (8 mCrab) 2008-08-03 = MJD 54681: 0.002 ± 0.0003 ct/s/cm^2 (7 mCrab) 2008-09-28 = MJD 54737: 0.001 ± 0.0006 ct/s/cm^2 (6 mCrab) 2008-12-01 = MJD 54801: 0.002 ± 0.0006 ct/s/cm^2 (9 mCrab) All results are for 8-day averages starting on the day listed and are for the 15-50 keV band.

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