The XMM-Newton serendipitous survey ******

Authors :: Carrera, F. J.
Ebrero, J.
Mateos, S.
Ceballos, M. T.
Corral, A.
Barcons, X.
Page, M. J.
Rosen, S. R.
Watson, M. G.
Tedds, J. A.
Della Ceca, R.
Maccacaro, T.
Brunner, H.
Freyberg, M.
Lamer, G.
Bauer, F. E.
Ueda, Y.
Carrera, F. J.
Ebrero, J.
Mateos, S.
Ceballos, M. T.
Corral, A.
Barcons, X.
Page, M. J.
Rosen, S. R.
Watson, M. G.
Tedds, J. A.
Della Ceca, R.
Maccacaro, T.
Brunner, H.
Freyberg, M.
Lamer, G.
Bauer, F. E.
Ueda, Y.
Source :: Astronomy and Astrophysics; July 2007, Vol. 469 Issue: 1 p27-46, 20p
Publication Year :: 2007
Abstract: Context.Recent results have revised upwards the total X-ray background (XRB) intensity below ~10 keV, therefore an accurate determination of the source counts is needed. There are also contradictory results on the clustering of X-ray selected sources.

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