The XMM‐Newton Survey Science Centre Medium Sensitivity Survey | Zendy

Barcons X. | Zendy; Carrera F.J. | Zendy; Ceballos M.T. | Zendy; Mateos S. | Zendy; Page M.J. | Zendy; PérezFour I. | Zendy; Watson M.G. | Zendy

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The XMM‐Newton Survey Science Centre Medium Sensitivity Survey

Author(s) -

Barcons X.,

Carrera F.J.,

Ceballos M.T.,

Mateos S.,

Page M.J.,

PérezFour I.,

Watson M.G.

Publication year - 2003

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.200310012

Subject(s) - qsos , physics , astrophysics , galaxy , stars , flux (metallurgy) , sensitivity (control systems) , absorption (acoustics) , astronomy , line (geometry) , active galactic nucleus , quasar , optics , geometry , mathematics , electronic engineering , engineering , materials science , metallurgy

We present preliminary results on the XMM‐Newton Survey Science Centre medium sensitivity survey, with 0.5‐4.5 keV flux limit 2 × 10 –14 erg cm –2 s –1 . 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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