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/10.1086/499558
XMM‐NewtonObservations of the Supernova Remnant IC 443. I. Soft X‐Ray Emission from Shocked Interstellar Medium
E. Troja, F. Bocchino and F. RealeThe Astrophysical Journal 649 (1) 258 (2006)
https://doi.org/10.1086/506378
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
Does the AGN Unified Model Evolve with Redshift? Using the X‐Ray Background to Predict the Mid‐Infrared Emission of AGNs
D. R. Ballantyne, Y. Shi, G. H. Rieke, et al.The Astrophysical Journal 653 (2) 1070 (2006)
https://doi.org/10.1086/508801
The effect of stellar feedback and quasar winds on the active galactic nucleus population
Fabio Fontanot, Pierluigi Monaco, Stefano Cristiani and Paolo TozziMonthly Notices of the Royal Astronomical Society 373 (3) 1173 (2006)
https://doi.org/10.1111/j.1365-2966.2006.11094.x
Absolute Measurement of the Unresolved Cosmic X‐Ray Background in the 0.5–8 keV Band withChandra
Ryan C. Hickox and Maxim MarkevitchThe Astrophysical Journal 645 (1) 95 (2006)
https://doi.org/10.1086/504070