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Cited article:

The Absence of Adiabatic Contraction of the Radial Dark Matter Profile in the Galaxy Cluster A2589

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Can the unresolved X-ray background be explained by the emission from the optically-detected faint galaxies of the GOODS project?

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Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation

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XMM-Newton study of the two-dimensional structure of the REFLEX-DXL galaxy clusters

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Astronomy & Astrophysics 442 (3) 827 (2005)
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Astrophysics in 2004

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Constraints on the distribution of absorption in the X-ray-selected AGN population found in the 13HXMM-Newton/Chandradeep field

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X-ray pre-ionization powered by accretion on the first black holes - II. Cosmological simulations and observational signatures

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On the Polar Caps of the Three Musketeers

A. De Luca, P. A. Caraveo, S. Mereghetti, M. Negroni and G. F. Bignami
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The Iron Line Background

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Exploring the structure of galaxy clusters: XMM-Newton observations of the REFLEX-DXL clusters at z∼ 0.3

Y.-Y. Zhang, H. Böhringer, A. Finoguenov, Y. Ikebe, K. Matsushita, P. Schuecker, L. Guzzo and C.A. Collins
Advances in Space Research 36 (4) 667 (2005)
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XMM‐NewtonEPIC Background Modeling for Extended Sources

J. Nevalainen, M. Markevitch and D. Lumb
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The nature of the X-ray halo of the plerion G21.5–0.9 unveiled by XMM-Newton and Chandra

F. Bocchino, E. van der Swaluw, R. Chevalier and R. Bandiera
Astronomy & Astrophysics 442 (2) 539 (2005)
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The HELLAS2XMM Survey. VII. The Hard X‐Ray Luminosity Function of AGNs up toz= 4: More Absorbed AGNs at Low Luminosities and High Redshifts

F. La Franca, F. Fiore, A. Comastri, et al.
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Active Galactic Nuclei Unification and the X‐Ray Background

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XMM-Newton observations of the Lockman Hole IV: spectra of the brightest AGN

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Astronomy & Astrophysics 444 (1) 79 (2005)
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The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM--Newton deep fields

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XMM-Newton Observations of G32.45+0.1 and G38.55+0.0: Diffuse Hard X-Ray Sources Found by the ASCA Galactic Plane Survey

Hiroya Yamaguchi, Masaru Ueno, Katsuji Koyama, Aya Bamba and Shigeo Yamauchi
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X-ray pre-ionization powered by accretion on the first black holes - I. A model for theWMAPpolarization measurement

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