A&A 411, L373-L376 (2003)
DOI: 10.1051/0004-6361:20031154
Letter
First results from the IBIS/ISGRI data obtained during the Galactic Plane Scan
II. The Vela region
J. Rodriguez1, 2, M. Del Santo3, F. Lebrun4, G. Belanger4, M. Cadolle-Bel4, F. Capitanio3, P. David1, L. Foschini5, P. Goldoni4, A. Goldwurm4, A. Gros4, P. Laurent4, A. Paizis6, 2, J. Paul4, R. Terrier1, S. E. Shaw7, 2 and P. Ubertini31 CEA Saclay, DSM/DAPNIA/SAp (CNRS FRE 2591), 91191 Gif-sur-Yvette Cedex, France
2 Integral Science Data Center, Chemin d'Écogia, 16, 1290 Versoix, Switzerland
3 IASF/CNR, via del Fosso del Cavaliere 100, 00133 Roma, Italy
4 CEA Saclay, DSM/DAPNIA/SAp, 91191 Gif-sur-Yvette Cedex, France
5 IASF/CNR, sezione di Bologna, via Gobetti 101, 40129 Bologna, Italy
6 IASF/CNR, Sezione di Milano, via Bassini 15, 20133 Milano, Italy
7 School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ UK
(Received 2 July 2003 / Accepted 30 July 2003)
Abstract
We report on INTEGRAL/IBIS observations of the Vela region
during a Galactic Plane Scan (hereafter GPS) presenting the IBIS in-flight
performances during these operations. Among all the known sources in the field
of view we clearly detect
4U 0836-429, Vela X-1, Cen X-3, GX 301-2, 1E 1145.1-6141,
and H0918-549 in the 20-40 keV energy range. Only Vela X-1 and GX 301-2
are detected in the 40-80 keV energy range, and no sources are visible above.
We present the results of each individual observation
(~
2200 s exposure), as well as those from the mosaic of these scans.
Key words: instrumentation: detectors -- Galaxy: disk --
Offprint request: J. Rodriguez, jrodriguez@cea.fr
SIMBAD Objects
© ESO 2003

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