A FULL YEAR'S CHANDRA EXPOSURE ON SLOAN DIGITAL SKY SURVEY QUASARS FROM THE CHANDRA MULTIWAVELENGTH PROJECT

作者：Green Paul J^*; Aldcroft T L; Richards G T; Barkhouse W A; Constantin A; Haggard D; Karovska M; Kim D W; Kim M; Vikhlinin A; Anderson S F; Mossman A; Kashyap V; Myers A C; Silverman J D; Wilkes B J; Tananbaum H

来源：Astrophysical Journal, 2009, 690(1): 644-669.

DOI：10.1088/0004-637X/690/1/644

• galaxies: active
• quasars: absorption lines
• quasars: general
• surveys
• X-rays: general

We study the spectral energy distributions and evolution of a large sample of optically selected quasars from the Sloan Digital Sky Survey that were observed in 323 Chandra images analyzed by the Chandra Multiwavelength Project. Our highest-confidence matched sample includes 1135 X-ray detected quasars in the redshift range 0.2 < z < 5.4, representing some 36 Msec of effective exposure. We provide catalogs of QSO properties, and describe our novel method of calculating X-ray flux upper limits and effective sky coverage. Spectroscopic redshifts are available for about 1/3 of the detected sample; elsewhere, redshifts are estimated photometrically. We detect 56 QSOs with redshift z > 3, substantially expanding the known sample. We find no evidence for evolution out to z similar to 5 for either the X-ray photon index Gamma or for the ratio of optical/UV to X-ray flux alpha(ox). About 10% of detected QSOs show best-fit intrinsic absorbing columns greater than 10(22) cm(-2), but the fraction might reach similar to 1/3 if most nondetections are absorbed. We confirm a significant correlation between alpha(ox) and optical luminosity, but it flattens or disappears for fainter (M(B) greater than or similar to -23) active galactic nucleus (AGN) alone. We report significant hardening of Gamma both toward higher X-ray luminosity, and for relatively X-ray loud quasars. These trends may represent a relative increase in nonthermal X-ray emission, and our findings thereby strengthen analogies between Galactic black hole binaries and AGN. For uniformly selected subsamples of narrow-line Seyfert 1s and narrow absorption line QSOs, we find no evidence for unusual distributions of either alpha(ox) or Gamma.

• 出版日期2009-1-1