To be published in Annu. Rev. Astron. Astrophys., Volume 43
(2005).
For a PDF version of the article, click
here.
astro-ph/0501058
Abstract. Deep surveys of the cosmic X-ray background are reviewed in the context of observational progress enabled by the Chandra X-ray Observatory and the X-ray Multi-Mirror Mission-Newton. The sources found by deep surveys are described along with their redshift and luminosity distributions, and the effectiveness of such surveys at selecting active galactic nuclei (AGN) is assessed. Some key results from deep surveys are highlighted including (1) measurements of AGN evolution and the growth of supermassive black holes, (2) constraints on the demography and physics of high-redshift AGN, (3) the X-ray AGN content of infrared and submillimeter galaxies, and (4) X-ray emission from distant starburst and normal galaxies. We also describe some outstanding problems and future prospects for deep extragalactic X-ray surveys.
Keywords: X-ray astronomy - Extragalactic surveys - Observational cosmology - Active galaxies - Starburst galaxies - Galaxies
Table of Contents
INTRODUCTION TO DEEP EXTRAGALACTIC X-RAY SURVEYS
Brief Historical Summary of X-ray Deep Field
Research
Current Deep Surveys with Chandra and XMM-Newton
Deep-Survey Number Counts and the Fraction of the
Cosmic X-ray Background Resolved
PROPERTIES OF THE SOURCES FOUND AND MISSED BY DEEP
EXTRAGALACTIC X-RAY SURVEYS
Source Classification Challenges
Basic Source Types
AGN Redshift and Luminosity Distributions
AGN Selection Completeness
SOME KEY RESULTS FROM DEEP EXTRAGALACTIC X-RAY
SURVEYS
X-ray Measurements of AGN Evolution and the Growth
of Supermassive Black Holes
X-ray Constraints on the Demography and Physics of
High-Redshift (z > 4) AGN
X-ray Constraints on AGN in Infrared and
Submillimeter Galaxies
X-ray Emission from Distant Starburst and Normal
Galaxies
FUTURE PROSPECTS FOR DEEP EXTRAGALACTIC X-RAY
SURVEYS
REFERENCES