A Large, Uniform Sample of X-ray Emitting AGN from the ROSAT All-Sky and Sloan Digital Sky Surveys: the Data Release 5 Sample
| dc.creator | Anderson, Scott F. | |
| dc.creator | Margon, Bruce | |
| dc.creator | Voges, Wolfgang | |
| dc.creator | Plotkin, Richard M. | |
| dc.creator | Syphers, David | |
| dc.creator | Haggard, Daryl | |
| dc.creator | Collinge, Matthew J. | |
| dc.creator | Meyer, Jillian | |
| dc.creator | Strauss, Michael A. | |
| dc.creator | Agueros, Marcel A. | |
| dc.creator | Hall, Patrick B. | |
| dc.creator | Homer, L. | |
| dc.creator | Ivezic, Zeljko | |
| dc.creator | Richards, Gordon T. | |
| dc.creator | Richmond, Michael W. | |
| dc.creator | Schneider, Donald P. | |
| dc.creator | Stinson, Gregory | |
| dc.creator | Berk, Daniel E. Vanden | |
| dc.creator | York, Donald G. | |
| dc.date | 2006-09-15 | |
| dc.date.accessioned | 2026-07-07T11:26:03Z | |
| dc.date.available | 2026-07-07T11:26:03Z | |
| dc.description | We describe further results of a program aimed to yield ~10^4 fully characterized optical identifications of ROSAT X-ray sources. Our program employs X-ray data from the ROSAT All-Sky Survey (RASS), and both optical imaging and spectroscopic data from the Sloan Digital Sky Survey (SDSS). RASS/SDSS data from 5740 deg^2 of sky spectroscopically covered in SDSS Data Release 5 (DR5) provide an expanded catalog of 7000 confirmed quasars and other AGN that are probable RASS identifications. Again in our expanded catalog, the identifications as X-ray sources are statistically secure, with only a few percent of the SDSS AGN likely to be randomly superposed on unrelated RASS X-ray sources. Most identifications continue to be quasars and Seyfert 1s with 15<m<21 and 0.01<z<4; but the total sample size has grown to include very substantial numbers of even quite rare AGN, e.g., now including several hundreds of candidate X-ray emitting BL Lacs and narrow-line Seyfert 1 galaxies. In addition to exploring rare subpopulations, such a large total sample may be useful when considering correlations between the X-ray and the optical, and may also serve as a resource list from which to select the "best" object (e.g., X-ray brightest AGN of a certain subclass, at a preferred redshift or luminosity) for follow-on X-ray spectral or alternate detailed studies. | |
| dc.description | Accepted for publication in AJ; 32 pages, including 11 figures, and 6 example tables | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0609458 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0609458 | |
| dc.identifier | Astron.J.133:313-329,2007 | |
| dc.identifier | doi:10.1086/509765 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/195701 | |
| dc.subject | Astrophysics | |
| dc.title | A Large, Uniform Sample of X-ray Emitting AGN from the ROSAT All-Sky and Sloan Digital Sky Surveys: the Data Release 5 Sample | |
| dc.type | text |