skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Deep CFHT Y-band Imaging of VVDS-F22 Field. II. Quasar Selection and Quasar Luminosity Function

Journal Article · · Astronomical Journal (New York, N.Y. Online)
; ; ; ; ; ;  [1];  [2];  [3];  [4]
  1. Department of Astronomy, School of Physics, Peking University, Beijing 100871 (China)
  2. Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871 (China)
  3. Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)
  4. Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn (Germany)

We report the results of a faint quasar survey in a one-square-degree field. The aim is to test the Y−K/g−z and J−K/i−Y color selection criteria for quasars at faint magnitudes to obtain a complete sample of quasars based on deep optical and near-infrared color–color selection and to measure the faint end of the quasar luminosity function (QLF) over a wide redshift range. We carried out a quasar survey based on the Y−K/g−z and J−K/i−Y quasar selection criteria, using the deep Y-band data obtained from our CFHT/WIRCam Y-band images in a two-degree field within the F22 field of the VIMOS VLT deep survey, optical co-added data from Sloan Digital Sky Survey Stripe 82 and deep near-infrared data from the UKIDSS Deep Extragalactic Survey in the same field. We discovered 25 new quasars at 0.5<4.5 and i<22.5 mag within one-square-degree field. The survey significantly increases the number of faint quasars in this field, especially at z∼2--3. It confirms that our color selections are highly complete in a wide redshift range (z<4.5), especially over the quasar number density peak at z∼2--3, even for faint quasars. Combining all previous known quasars and new discoveries, we construct a sample with 109 quasars and measure the binned QLF and parametric QLF. Although the sample is small, our results agree with a pure luminosity evolution at lower redshift and luminosity evolution and density evolution model at redshift z>2.5.

OSTI ID:
22897422
Journal Information:
Astronomical Journal (New York, N.Y. Online), Vol. 155, Issue 3; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
Country of Publication:
United States
Language:
English

Similar Records

DEEP CFHT Y-BAND IMAGING OF VVDS-F22 FIELD. I. DATA PRODUCTS AND PHOTOMETRIC REDSHIFTS
Journal Article · Wed Feb 01 00:00:00 EST 2017 · The Astronomical Journal (Online) · OSTI ID:22897422

Minor Contribution of Quasars to Ionizing Photon Budget at z ∼ 6: Update on Quasar Luminosity Function at the Faint End with Subaru/Suprime-Cam
Journal Article · Sun Oct 01 00:00:00 EDT 2017 · Astrophysical Journal Letters · OSTI ID:22897422

THE FAINT END OF THE QUASAR LUMINOSITY FUNCTION AT z {approx} 4
Journal Article · Sat Feb 20 00:00:00 EST 2010 · Astrophysical Journal · OSTI ID:22897422