Announcement of INTEGRAL Galactic Bulge monitoring program and (re)brightening of GRO J1655-40

Details Announcement of INTEGRAL Galactic Bulge monitoring program and (re)brightening of GRO J1655-40 Announcement of INTEGRAL Galactic Bulge monitoring program and (re)brightening of GRO J1655-40

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..438....1k&link_type=abstract

The Astronomer's Telegram, #438

Astronomy and Astrophysics

Astronomy

22

X-Ray, Gamma Ray, Binaries, Black Holes, Globular Clusters, Neutron Stars, Soft Gamma-Ray Repeaters, Transients, Variables

Scientific paper

The Galactic Bulge is a region rich in bright and variable high-energy X-ray and gamma-ray sources. From February 17, 2005 and onwards we will observe this region regularly, using the European gamma-ray satellite INTEGRAL, during all the Galactic Bulge visibility periods under an approved AO-3 proposal (PI: Kuulkers). One complete hexagonal dither pattern (7 pointings of 1800 sec each) is performed during each INTEGRAL revolution (i.e., every 3 days).

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