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Issue A&A
Volume 411, Number 1, November III 2003
Special letters issue on: first science with integral
Page(s) L373 - L376
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20031154



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. Ubertini3

1  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 -- $\gamma$-rays: observations -- X-rays: binaries

Offprint request: J. Rodriguez, jrodriguez@cea.fr

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