AGN surveys to study galaxy evolution along cosmic times
arXiv:1312.4294 · doi:10.1017/S1743921314003718
Abstract
Various observational techniques have been used to survey galaxies and AGN, from X-rays to radio frequencies, both photometric and spectroscopic. I will review these techniques aimed at the study of galaxy evolution and of the role of AGNs and star formation as the two main energy production mechanisms. I will then present as a new observational approach the far-IR spectroscopic surveys that could be done with planned astronomical facilities of the next future, such as SPICA from the space and CCAT from the ground.
To be published in "Multiwavelength AGN surveys and studies", Proceedings of IAU Symposium No. 304, 2013, International Astronomical Union A. Mickaelian, F. Aharonian, D. Sanders, eds. arXiv admin note: text overlap with arXiv:1309.7862
References in corpus (5)
- Swift BAT Survey of AGN
- Emission-line Diagnostics of Low Metallicity AGN
- Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 I: the Spectra
- The Spitzer mid-infrared AGN survey. I - optical and near-infrared spectroscopy of candidate obscured and normal AGN selected in the mid-infrared
- The INTEGRAL/IBIS AGN catalogue I: X-ray absorption properties versus optical classification