99 citations · 137 across the 2 of their papers we have counts for
6 papers · 1 filter
High precision X-ray logN-logS distributions: implications for the obscured AGN population
S. Mateos, R. S. Warwick, F. J. Carrera +13
We have constrained the extragalactic source count distributions over a broad range of X-ray fluxes and in various energy bands to test whether the predictions from X-ray backgroun…
XMM-Newton observations of the Lockman Hole IV: spectra of the brightest AGN
S. Mateos, X. Barcons, F. J. Carrera +5
This paper presents the results of a detailed X-ray spectral analysis of a sample of 123 X-ray sources (46 being type-1 AGN and 28 type-2 AGN) detected with XMM-Newton in the Lockm…
X-ray spectra of XMM-Newton serendipitous medium flux sources
S. Mateos, X. Barcons, F. J. Carrera +7
We report on the results of a detailed analysis of the X-ray spectral properties of a large sample of sources detected serendipitously with the XMM-Newton observatory in 25 selecte…
The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields
M. A. Worsley, A. C. Fabian, F. E. Bauer +6
We extend our earlier work on X-ray source stacking in the deep XMM-Newton observation of the Lockman Hole, to the 2 Ms Chandra Deep Field North and the 1 Ms Chandra Deep Field Sou…
XMM-Newton observations of the Lockman Hole: III. A relativistic Fe line in the mean X-ray spectra of type-1 and type-2 AGN
A. Streblyanska, G. Hasinger, A. Finoguenov +3
Using the 770 ksec XMM-Newton survey of the Lockman Hole field in combination with extensive optical identifications of the AGN population, we derive an average rest-frame spectrum…
The (un)resolved X-ray background in the Lockman Hole
M. A. Worsley, A. C. Fabian, X. Barcons +3
Most of the soft and a growing fraction of the harder X-ray background has been resolved into emission from point sources, yet the resolved fraction above 7 keV has only been poorl…