The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era (Q58912291)

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volume

463

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issue

1

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page(s)

79–96

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The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source Catalogs

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Connecting Galaxy Evolution, Star Formation, and the Cosmic X‐Ray Background

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The HELLAS2XMM Survey. I. The X‐Ray Data and the log N–log SRelation

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The Iron Line Background

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The 2–8 keV cosmic X-ray background spectrum as observed with XMM-Newton

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The BeppoSAX High Energy Large Area Survey (HELLAS) -- II. Number counts and X-ray spectral properties

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Evidence for x Rays From Sources Outside the Solar System

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XMM-Newton observation of the Lockman Hole

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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

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The obscuration by dust of most of the growth of supermassive black holes

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The Chandra Deep Field–South: The 1 Million Second Exposure

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Spectral Statistics and Local Luminosity Function of a Complete Hard X-Ray Sample of the Brightest Active Galactic Nuclei

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New Results from the X‐Ray and Optical Survey of the Chandra Deep Field–South: The 300 Kilosecond Exposure. II

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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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