The 2–8 keV cosmic X-ray background spectrum as observed with XMM-Newton
A&A, 419 3 (2004) 837-848
Published online: 2004-05-07
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https://doi.org/10.1051/0004-6361:20053868
The XMM large scale structure survey: properties and two-point angular correlations of point-like sources
P. Gandhi, O. Garcet, L. Disseau, et al.Astronomy & Astrophysics 457 (2) 393 (2006)
https://doi.org/10.1051/0004-6361:20065284
The Evolution of Obscuration in Active Galactic Nuclei
Ezequiel Treister and C. Megan UrryThe Astrophysical Journal 652 (2) L79 (2006)
https://doi.org/10.1086/510237
Connecting Galaxy Evolution, Star Formation, and the Cosmic X‐Ray Background
D. R. Ballantyne, J. E. Everett and N. MurrayThe Astrophysical Journal 639 (2) 740 (2006)
https://doi.org/10.1086/499558
XMM-Newton Detection of the Supernova Remnant G337.2+0.1
Jorge A. Combi, Juan F. Albacete Colombo, Gustavo E. Romero and Paula BenagliaThe Astrophysical Journal 653 (1) L41 (2006)
https://doi.org/10.1086/510329
X-ray properties in massive galaxy clusters: XMM-Newton observations of the REFLEX-DXL sample
Y.-Y. Zhang, H. Böhringer, A. Finoguenov, et al.Astronomy & Astrophysics 456 (1) 55 (2006)
https://doi.org/10.1051/0004-6361:20053650