In "Physics of Active Galactic Nuclei at All Scales",
eds. Alloin D., Johnson R., Lira P. (Springer-Verlag, Berlin), 2004.
astro-ph/0403646
For a PDF version of the article, click
here.
X-RAY SURVEY RESULTS ON ACTIVE GALAXY PHYSICS AND EVOLUTION
W.N. Brandt 1, D.M. Alexander
2, F.E. Bauer 2, and C. Vignali
3
1 Department of
Astronomy & Astrophysics,
The Pennsylvania State
University, 525 Davey Lab, University Park, PA 16802, USA
(niel@astro.psu.edu)
2 Institute
of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
(dma@ast.cam.ac.uk,
feb@ast.cam.ac.uk)
3 INAF - Osservatorio Astronomico di Bologna, Via Ranzani 1,
40127 Bologna, Italy
(cristian@anastasia.bo.astro.it)
Table of Contents
INTRODUCTION
- CHANDRA AND XMM-NEWTON EXTRAGALACTIC SURVEYS
- Deep X-ray Surveys
- Wider X-ray Surveys
- SOME IMPLICATIONS FOR AGN PHYSICS AND EVOLUTION
- Properties of the X-ray Sources
- Recent X-ray Results on AGN Evolution
- X-ray Emitting AGN in Luminous Submillimeter
Galaxies
- High-Redshift (z > 4) AGN Demography and
Physics
- SOME FUTURE PROSPECTS
- Future Prospects for Chandra and XMM-Newton
- Upcoming and Planned X-ray Missions
- SOME KEY RECENT REFERENCES
