Significant increase of the X-ray flux and slight softening of the spectrum of Aql X-1

Details Significant increase of the X-ray flux and slight softening of the spectrum of Aql X-1 Significant increase of the X-ray flux and slight softening of the spectrum of Aql X-1

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..464....1r&link_type=abstract

The Astronomer's Telegram, #464

Astronomy and Astrophysics

Astronomy

2

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

Scientific paper

On April 12th, 2005, 20:49:01 UTC, INTEGRAL performed an observation of GRS 1915+105 as part of a monitoring campaign of this microquasar. During this observation, Aql X-1 has always been in the IBIS/ISGRI partially coded field of view. The IBIS/ISGRI telescope detected the source at a flux level of 141+-1 mCrab in the 18-45 keV band and 101+-3 mCrab in the 45-80 keV energy range (average values over a ~100 ksec observation, assuming a crab-like spectrum).

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