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arxiv: astro-ph/0211533 · v1 · pith:6VZDBYSWnew · submitted 2002-11-25 · 🌌 astro-ph

The XMM-Newton Survey Science Centre Medium Sensitivity Survey

X. Barcons (IFCA/Csic-Uc) , F.J. Carrera (IFCA/Csic-Uc) , M.T. Ceballos (IFCA/Csic-Uc) , S. Mateos (IFCA/Csic-Uc) , M.J. Page (MSSL) , I. Perez-Fournon (IAC) , M.G. Watson (Leicester) , the XMM-Newton Survey Science Centre This is my paper
classification 🌌 astro-ph
keywords surveycentremediumsciencesensitivitytypex-rayxmm-newton
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We present preliminary results on the XMM-Newton Survey Science Centre medium sensitivity survey (XMS), with 0.5-4.5 keV flux limit 2 10^{-14} erg/cm2/s. At present, 19 fields have been examined with a total of 239 X-ray sources. Identifications for about 2/3 of these reveal that type 1 AGN dominate, but type 2 AGN, absorption-line galaxies and clusters as well as stars are also present. We also discuss on a few X-ray selected Broad-Absorption-Line QSOs found in this survey.

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