INTEGRAL observation of GRO J1655-40

Details INTEGRAL observation of GRO J1655-40 INTEGRAL observation of GRO J1655-40

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..422....1p&link_type=abstract

The Astronomer's Telegram, #422

Astronomy and Astrophysics

Astronomy

1

Gamma Ray, Binaries, Transients, Variables, Stars

Scientific paper

During INTEGRAL observations of the Galactic Disk, the superluminal source GRO J1655-40 was observed with the ISGRI detector. The source was detected in 5 ~2000second long pointings between 2005-02-18 and 2005-02-19 at a flux between 3 and 4 cps in the 20-50 keV band (corresponding to approx 30mCrab). This measurement confirms that of ATEL 415 and 414, which showed that the source is slowly brightening in the 2-10 keV band.

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