AGN Populations in Large Volume X-ray Surveys: Photometric Redshifts and Population Types found in the Stripe 82X Survey
arXiv:1710.01296 · doi:10.3847/1538-4357/aa937d
Abstract
Multi-wavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high luminosity and/or high redshift active galactic nuclei (AGN). Stripe 82X is a 31.3 deg X-ray survey with and -Newton observations overlapping the legacy Sloan Digital Sky Survey (SDSS) Stripe 82 field, which has a rich investment of multi-wavelength coverage from the ultraviolet to the radio. The wide-area nature of this survey presents new challenges for photometric redshifts for AGN compared to previous work on narrow-deep fields because it probes different populations of objects that need to be identified and represented in the library of templates. Here we present an updated X-ray plus multi-wavelength matched catalog, including counterparts, and estimated photometric redshifts for 5961 (96% of a total of 6181) X-ray sources, which have a normalized median absolute deviation, = 0.06 and an outlier fraction, = 13.7%. The populations found in this survey, and the template libraries used for photometric redshifts, provide important guiding principles for upcoming large-area surveys such as and 3 (in X-ray) and the Large Synoptic Survey Telescope (LSST; optical).
Accepted for publication by The Astrophysical Journal (33 pages, 20 figures, 13 tables). Final catalog of counterparts and photo-z supplementing the paper available here: http://stripe82x.com/docs/stripe82x-photometric-redshifts-and-multiwavelength-data-catalog/
References in corpus (19)
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue
- The Sloan Digital Sky Survey Quasar Catalog: twelfth data release
- Photometric redshift and classification for the XMM-COSMOS sources
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- Obscuration-dependent evolution of Active Galactic Nuclei
- The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. IV. H Time Lags and Implications for Super-Eddington Accretion
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey
- The 2dF-SDSS LRG and QSO Survey: The spectroscopic QSO catalogue
- Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic Nuclei
- The Sloan Digital Sky Survey Stripe 82 Imaging Data: Depth-Optimized Co-adds Over 300 Deg^2 in Five Filters
- High-resolution VLA Imaging of SDSS Stripe 82 at 1.4 GHz
- The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions