The X-ray-Infrared/Submillimetre Connection and the Legacy Era of Cosmology
arXiv:0802.0175 · doi:10.1002/asna.200710895
Abstract
We review some recent results on the identification and characterisation of Active Galactic Nuclei (AGN) obtained by cross correlating X-ray surveys with infrared and submillimetre surveys. We also look toward the scientific gains that could be achieved from an XMM-Newton survey of the medium-deep legacy fields that are being observed at ~1-850um.
4 pages, contribution for "XMM-Newton: The Next Decade", AN in press
References in corpus (7)
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
- Chandra and Spitzer unveil heavily obscured quasars in the SWIRE/Chandra Survey
- Spitzer 70-micron Source Counts in GOODS-North
- The growth of the nuclear black holes in submillimeter galaxies
- Evidence for a large fraction of Compton-thick quasars at high redshift