The Extremely Luminous Quasar Survey in the SDSS Footprint. I. Infrared-based Candidate Selection

Jan Torge Schindler, Xiaohui Fan, Ian D. McGreer, Qian Yang, Jin Wu, Linhua Jiang, Richard Green

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

Studies of the most luminous quasars at high redshift directly probe the evolution of the most massive black holes in the early universe and their connection to massive galaxy formation. However, extremely luminous quasars at high redshift are very rare objects. Only wide-area surveys have a chance to constrain their population. The Sloan Digital Sky Survey (SDSS) has so far provided the most widely adopted measurements of the quasar luminosity function at z > 3. However, a careful re-examination of the SDSS quasar sample revealed that the SDSS quasar selection is in fact missing a significant fraction of z ≳ 3 quasars at the brightest end. We identified the purely optical-color selection of SDSS, where quasars at these redshifts are strongly contaminated by late-type dwarfs, and the spectroscopic incompleteness of the SDSS footprint as the main reasons. Therefore, we designed the Extremely Luminous Quasar Survey (ELQS), based on a novel near-infrared JKW2 color cut using Wide-field Infrared Survey Explorer mission (WISE) AllWISE and 2MASS all-sky photometry, to yield high completeness for very bright (mi < 18.0) quasars in the redshift range of 3.0 ≤ z ≤ 5.0. It effectively uses random forest machinelearning algorithms on SDSS and WISE photometry for quasar-star classification and photometric redshift estimation. The ELQS will spectroscopically follow-up ∼230 new quasar candidates in an area of ∼12,000 deg2 in the SDSS footprint to obtain a well-defined and complete quasar sample for an accurate measurement of the brightend quasar luminosity function (QLF) at 3.0 ≤ z ≤ 5.0. In this paper, we present the quasar selection algorithm and the quasar candidate catalog.

Original languageEnglish (US)
Article number13
JournalAstrophysical Journal
Volume851
Issue number1
DOIs
StatePublished - Dec 10 2017

Fingerprint

footprints
footprint
quasars
Wide-field Infrared Survey Explorer
photometry
luminosity
color
near infrared
galactic evolution
completeness
probe
catalogs
sky

Keywords

  • galaxies: nuclei
  • quasars: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

The Extremely Luminous Quasar Survey in the SDSS Footprint. I. Infrared-based Candidate Selection. / Schindler, Jan Torge; Fan, Xiaohui; McGreer, Ian D.; Yang, Qian; Wu, Jin; Jiang, Linhua; Green, Richard.

In: Astrophysical Journal, Vol. 851, No. 1, 13, 10.12.2017.

Research output: Contribution to journalArticle

Schindler, Jan Torge ; Fan, Xiaohui ; McGreer, Ian D. ; Yang, Qian ; Wu, Jin ; Jiang, Linhua ; Green, Richard. / The Extremely Luminous Quasar Survey in the SDSS Footprint. I. Infrared-based Candidate Selection. In: Astrophysical Journal. 2017 ; Vol. 851, No. 1.
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