A high energy perspective of the co-evolution of black holes and their host galaxies
Thanks to the Chandra and XMM–Newton surveys, the hard X-ray sky is now probed down to a flux limit where the bulk of the X-ray background is almost completely resolved into discrete sources, at least in the 2–8 keV band. Extensive programs of multiwavelength follow-up observations showed that th...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Doctoral Thesis |
| Language: | en |
| Published: |
Alma Mater Studiorum - Università di Bologna
2007
|
| Subjects: | |
| Online Access: | http://amsdottorato.unibo.it/351/ |