The Large‐Scale Bias of the Hard X‐Ray Background
- 10 September 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 612 (2) , 647-651
- https://doi.org/10.1086/422678
Abstract
No abstract availableAll Related Versions
This publication has 36 references indexed in Scilit:
- Cross-correlation of the cosmic microwave background with the 2MASS galaxy survey: Signatures of dark energy, hot gas, and point sourcesPhysical Review D, 2004
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- Optical and Infrared Properties of the 2 Ms Chandra Deep Field North X-Ray SourcesThe Astronomical Journal, 2003
- X-Ray, Optical, and Infrared Imaging and Spectral Properties of the 1 M[CLC]s[/CLC] Chandra Deep Field North SourcesThe Astronomical Journal, 2002
- Supermassive Black Hole Accretion History Inferred from a Large Sample of [ITAL]CHANDRA[/ITAL][ITAL]Chandra[/ITAL] Hard X-Ray SourcesThe Astronomical Journal, 2001
- Optical Identification of theASCALarge Sky SurveyThe Astrophysical Journal, 2000
- The nature of galaxy bias and clusteringMonthly Notices of the Royal Astronomical Society, 2000
- X‐Ray Emission from the Local Supercluster: Possible Evidence for Hot, Diffuse GasThe Astrophysical Journal, 1999
- The cosmic x-ray backgroundPhysics Reports, 1987
- The spatial correlation function of rich clusters of galaxiesThe Astrophysical Journal, 1983