vix.ing · top · new · best · stats · spec

The INTEGRAL Galactic bulge monitoring program: the first 1.5 years

2007/01/09 by E. Kuulkers, S. E. Shaw, A. Paizis +18 · 4 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Black hole (networking) #Bulge #Galactic Center #Galaxy #Homogeneous #Neutron star #Optics #Physics #Pulsars and Gravitational Waves Research #Visibility #X-ray #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066651

published as PoS Integral08:121,2008 · 27 pages, 42 figures, accepted for publication in A&A. Abstract abridged. Tables 3,4,6,7 appear at the end. Images have been compressed and are reduced in quality; original PostScript images can be retrieved from http://isdc.unige.ch/~kuulkers/bulge/

arxiv created 2007/01/09 · openalex publication_date 2007/01/22 · arxiv updated 2010/04/30 · openalex created_date 2018/03/29 · openalex updated_date 2026/08/05

Abstract

Aims.The Galactic bulge region is a rich host of variable high-energy point sources. Since 2005, February 17 we are monitoring the source activity in the Galactic bulge region regularly and frequently, i.e., about every three days, with the instruments onboard INTEGRAL. Thanks to the large field of view, the imaging capabilities and the sensitivity at hard X-rays, we are able to present for the first time a detailed homogeneous (hard) X-ray view of a sample of 76 sources in the Galactic bulge region.

Citations

Cited by