The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. the North Galactic Cap Sample

Jan Torge Schindler, Xiaohui Fan, Ian D. McGreer, Jinyi Yang, Feige Wang, Richard Green, Nicolas Garavito-Camargo, Yun Hsin Huang, Christine O'Donnell, Anna Patej, Ragadeepika Pucha, Jon M. Rees, Eckhart Spalding

Research output: Contribution to journalArticle

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Abstract

We present the North Galactic Cap sample of the Extremely Luminous Quasar Survey (ELQS-N), which targets quasars with M 1450 < -27 at 2.8 ≤ z < 5 in an area of ∼7600 deg2 of the Sloan Digital Sky Survey (SDSS) footprint with 90° < R.A. < 270°. Based on a near-infrared/infrared JKW2 color cut, the ELQS selection efficiently uses random forest methods to classify quasars and to estimate photometric redshifts; this scheme overcomes some of the difficulties of pure optical quasar selection at z ≈ 3. As a result, we retain a completeness of >70% over z ∼ 3.0-5.0 at m i ≲ 17.5, limited toward fainter magnitudes by the depth of the Two Micron All Sky Survey. The presented quasar catalog consists of a total of 270 objects, of which 39 are newly identified in this work with spectroscopy obtained at the Vatican Advanced Technology Telescope and the MMT 6.5 m telescope. In addition to the high completeness, which allowed us to discover new quasars in the already well-surveyed SDSS North Galactic Cap, the efficiency of our selection is relatively high at ∼79%. Using 120 objects of this quasar sample we are able to extend the previously measured optical quasar luminosity function (QLF) by one magnitude toward the bright end at 2.8 ≤ z ≤ 4.5. A first analysis of the QLF suggests a relatively steep bright-end slope of β ≈ -4 for this sample. This result contrasts with previous results in the same redshift range, which find a much flatter slope around β ∼ -2.5, but agrees with recent measurements of the bright-end slope at lower and higher redshifts. Our results constrain the bright-end slope at z = 2.8-4.5 to β < -2.94 with a 99% confidence.

Original languageEnglish (US)
Article number144
JournalAstrophysical Journal
Volume863
Issue number2
DOIs
StatePublished - Aug 20 2018

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footprints
caps
footprint
quasars
slopes
advanced technology
luminosity
telescopes
spectroscopy
completeness
catalogs
confidence

Keywords

  • galaxies: active
  • galaxies: high-redshift
  • galaxies: nuclei
  • quasars: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. the North Galactic Cap Sample. / Schindler, Jan Torge; Fan, Xiaohui; McGreer, Ian D.; Yang, Jinyi; Wang, Feige; Green, Richard; Garavito-Camargo, Nicolas; Huang, Yun Hsin; O'Donnell, Christine; Patej, Anna; Pucha, Ragadeepika; Rees, Jon M.; Spalding, Eckhart.

In: Astrophysical Journal, Vol. 863, No. 2, 144, 20.08.2018.

Research output: Contribution to journalArticle

Schindler, JT, Fan, X, McGreer, ID, Yang, J, Wang, F, Green, R, Garavito-Camargo, N, Huang, YH, O'Donnell, C, Patej, A, Pucha, R, Rees, JM & Spalding, E 2018, 'The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. the North Galactic Cap Sample', Astrophysical Journal, vol. 863, no. 2, 144. https://doi.org/10.3847/1538-4357/aad2dd
Schindler, Jan Torge ; Fan, Xiaohui ; McGreer, Ian D. ; Yang, Jinyi ; Wang, Feige ; Green, Richard ; Garavito-Camargo, Nicolas ; Huang, Yun Hsin ; O'Donnell, Christine ; Patej, Anna ; Pucha, Ragadeepika ; Rees, Jon M. ; Spalding, Eckhart. / The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. the North Galactic Cap Sample. In: Astrophysical Journal. 2018 ; Vol. 863, No. 2.
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AU - Wang, Feige

AU - Green, Richard

AU - Garavito-Camargo, Nicolas

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