Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 147, Number 1, November II 2000
Page(s) 75 - 91
DOI https://doi.org/10.1051/aas:2000290
Published online 15 November 2000
DOI: 10.1051/aas:2000290

Astron. Astrophys. Suppl. Ser. 147, 75-91

ROSAT HRI catalogue of X-ray sources in the SMC region

M. Sasaki, F. Haberl, and W. Pietsch

Send offprint request: M. Sasaki;
e-mail: manami@mpe.mpg.de

Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany

Received March 24; accepted August 22, 2000

Abstract:

During the operational phase of the ROSAT satellite between 1990 and 1998 the X-ray telescope pointed 71 times to the Small Magellanic Cloud (SMC) for observations with the High Resolution Imager (HRI), covering a field of 5$^\circ$ $\times$ 5$^\circ$. From these data a catalogue of 121 discrete X-ray sources was derived. By cross-correlating the source catalogue with the SIMBAD data base and the TYCHO catalogue, the systematic positional error of the HRI source positions could be reduced. In total the X-ray position for 99 HRI sources was corrected yielding positional errors between 1 $^{\prime\prime}$ and 16 $^{\prime\prime}$. The HRI catalogue was also cross-correlated with the catalogues derived from the ROSAT Position Sensitive Propotional Counter (PSPC) pointings (Kahabka et al. 1999; Haberl et al. 2000). For 75 HRI sources PSPC counterparts were found and thus hardness ratios are given. With the help of the information obtained from the cross-correlations 56 HRI sources were identified with objects of known or proposed nature. Four foreground stars, six supernova remnants, four supersoft sources, 12 X-ray binaries, and one AGN were detected by the HRI. Based on the existence of a likely optical counterpart or properties like hardness ratio and X-ray to optical flux ratio, further 15 HRI sources were classified into different source types.

Key words: catalogs -- galaxies: magellanic clouds -- galaxies: stellar content -- X-rays: galaxies -- X-rays: stars

SIMBAD Objects

Copyright The European Southern Observatory (ESO)

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