401. Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios
- Author
-
Cristian Vignali, Chiara Feruglio, Enrico Piconcelli, Mara Salvato, Carlotta Gruppioni, Giorgio Lanzuisi, Fabrizio Fiore, Lanzuisi G., Piconcelli E., Fiore F., Feruglio C., Vignali C., Salvato M., and Gruppioni C.
- Subjects
Physics ,Supermassive black hole ,education.field_of_study ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::High Energy Astrophysical Phenomena ,Population ,Flux ,FOS: Physical sciences ,Astronomy and Astrophysics ,Context (language use) ,Quasar ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Luminosity ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,Absorption (electromagnetic radiation) ,education ,galaxies: active – galaxies: high-redshift – galaxies: nuclei – infrared: galaxies – X-rays: galaxies ,Astrophysics::Galaxy Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Recent works have suggested that selection criteria based on MIR colors can be used to reveal a population of dust-enshrouded, extremely luminous quasars at z>1. However the X-ray spectral properties of these intriguing sources still remain largely unexplored. We report on an X-ray spectroscopic study of a sample of 44 very bright mid-IR galaxies with extreme mid-IR to optical flux ratios (MIR/O>2000). The X-ray coverage of the sample is highly inhomogeneous (from snap-shot 5 ks Chandra observations to medium-deep XMM exposures of 70 ks) and, consequently, a sizable fraction of them (~43%) remains undetected in the 0.5-10 keV band. The vast majority (95%) of the detected sources (23) show an absorption column density NH>10e22 cm-2 and, remarkably, we also find that 50% of them can be classified as Type 2 quasars on the basis of their absorption properties and X-ray luminosity. Moreover, most of the X-ray undetected sources show extreme mid-IR colors, consistent with being luminous AGN-powered objects, suggesting they might host heavily obscured (possibly Compton-thick) quasars in X-rays. This demonstrates that our selection criteria applied to a wide area survey is very efficient in finding a large number of Type 2 quasars at z > 1. The existence of this class of very powerful, obscured quasars at high z could have important implications in the context of the formation and cosmological evolution of accreting supermassive black holes and their host galaxies., Accepted for publication in Astronomy and Astrophysics (2009A&A, 498, 67L)
- Published
- 2009