activity
20062008
most citedThe XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

489 citations · 1.2k across the 12 of their papers we have counts for

collaborators

11 papers

astro-ph200811 cited

An extreme EXO: a type 2 QSO at z=1.87

A. Del Moro, M. G. Watson, S. Mateos +6

We aim to understand the multi-wavelength properties of 2XMM J123204+215255, the source with the most extreme X-ray-to-optical flux ratio amongst a sample of bright X-ray selected…

astro-ph200846 cited

Average Fe K-alpha emission from distant AGN

A. Corral, M. J. Page, F. J. Carrera +7

One of the most important parameters in the XRB (X-ray background) synthesis models is the average efficiency of accretion onto SMBH (super-massive black holes). This can be inferr…

astro-ph2008489 cited

The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

M. G. Watson, A. C. Schröder, D. Fyfe +47

Aims: Pointed observations with XMM-Newton provide the basis for creating catalogues of X-ray sources detected serendipitously in each field. This paper describes the creation and…

astro-ph2008184 cited

The Subaru/XMM-Newton Deep Survey (SXDS): III. X-Ray Data

Yoshihiro Ueda, Michael G. Watson, Ian M. Stewart +10

We present the X-ray source catalog in the Subaru/XMM-Newton deep survey. A continuous area of 1.14 deg^2 centered at R.A. = 02h18m and Dec. = -05d is mapped by seven pointings wit…

astro-ph2008105 cited

The cosmological properties of AGN in the XMM-Newton Hard Bright Survey

R. Della Ceca, A. Caccianiga, P. Severgnini +7

(ABRIDGED) We investigate here the XLF of absorbed (Nh between 4E21 and E24 cm-2) and unabsorbed (Nh < 4E21 cm-2) AGN, the fraction of absorbed AGN as a function of Lx (and z), the…

astro-ph200827 cited

X-ray absorption in distant type II QSOs

M. Krumpe, G. Lamer, A. Corral +7

We present the results of the X-ray spectral analysis of an XMM-Newton-selected type II QSO sample with z>0.5 and 0.5-10 keV flux of 0.3-33 x 10^{-14} erg/s/cm^2. The distribution…