The BMW-Chandra survey. Serendipitous Source Catalogue
| dc.creator | Romano, P. | |
| dc.creator | Mignani, R. P. | |
| dc.creator | Campana, S. | |
| dc.creator | Moretti, A. | |
| dc.creator | Panzera, M. R. | |
| dc.creator | Tagliaferri, G. | |
| dc.creator | Mottini, M. | |
| dc.date | 2009-02-05 | |
| dc.date.accessioned | 2026-07-07T12:38:17Z | |
| dc.date.available | 2026-07-07T12:38:17Z | |
| dc.description | We present the BMW-Chandra source catalogue derived from Chandra ACIS-I observations (exposure time >10ks) public as of March 2003 by using a wavelet detection algorithm (Lazzati et al. 1999; Campana et al. 1999). The catalogue contains a total of 21325 sources, 16758 of which are serendipitous. Our sky coverage in the soft band (0.5-2 keV, S/N =3) is ~8 deg^2 for F_X > 10^-13 erg cm^-2 s-1, and ~2 deg^2 for F_X >10^-15 erg cm^-2 s^-1. The catalogue contains information on positions, count rates (and errors) in three energy bands. (total, 0.5-7 keV; soft, 0.5-2 keV; and hard, 2-7keV), and in four additional energy bands, SB1 (0.5-1keV), SB2 (1-2 keV), HB1 (2-4 keV), and HB2 (4-7keV), as well as information on the source extension, and cross-matches with the FIRST, IRAS, 2MASS, and GSC-2 catalogues. | |
| dc.description | 2 pages, to be published in the Proceedings of the Conference "Multiwavelength Astronomy and the Virtual Observatory", held at ESAC-Madrid, December 1-3 2008 | |
| dc.identifier | https://arxiv.org/abs/0902.0969 | |
| dc.identifier | http://arxiv.org/abs/0902.0969 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/218706 | |
| dc.subject | High Energy Astrophysical Phenomena | |
| dc.title | The BMW-Chandra survey. Serendipitous Source Catalogue | |
| dc.type | text |