Candidate Type II Quasars from the Sloan Digital Sky Survey. I. Selection and Optical Properties of a Sample at 0.3 < Z < 0.83
/ Authors
N. Zakamska, M. Strauss, J. Krolik, M. Collinge, P. Hall, L. Hao, T. Heckman, Ž. Ivezić, G. Richards, D. Schlegel
and 5 more authors
D. Schneider, I. Strateva, D. V. vanden Berk, S. Anderson, J. Brinkmann
/ Abstract
Type II quasars are the long-sought luminous analogs of type 2 (narrow emission line) Seyfert galaxies, suggested by unification models of active galactic nuclei (AGNs) and postulated to account for an appreciable fraction of the cosmic hard X-ray background. We present a sample of 291 type II AGNs at redshifts 0.3 < Z < 0.83 from the spectroscopic data of the Sloan Digital Sky Survey. These objects have narrow (FWHM < 2000 km s-1), high equivalent width emission lines with high-ionization line ratios. We describe the selection procedure and discuss the optical properties of the sample. About 50% of the objects have [O III] λ5008 line luminosities in the range 3 × 108–1010 L⊙, comparable to those of luminous (-27 < MB < -23) quasars; this, along with other evidence, suggests that the objects in the luminous subsample are type II quasars.
Journal: The Astronomical Journal
DOI: 10.1086/378610