The Extremely Luminous Quasar Survey (ELQS) in the Sloan Digital Sky Survey footprint. II. The North Galactic Cap Sample
arXiv:1806.03374 · doi:10.3847/1538-4357/aad2dd
Abstract
We present the North Galactic Cap sample of the Extremely Luminous Quasar Survey (ELQS-N), which targets quasars with at in an area of of the Sloan Digital Sky Survey (SDSS) footprint with . Based on a near-infrared/infrared \textit{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 . As a result, we retain a completeness of over at , limited toward fainter magnitudes by the depth of the Two Micron All Sky Survey (2MASS). 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 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 . 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 . A first analysis of the QLF suggests a relatively steep bright-end slope of for this sample. This result contrasts with previous results in the same redshift range, which find a much flatter slope around , but agrees with recent measurements of the bright-end slope at lower and higher redshifts. Our results constrain the bright-end slope at to with a 99\% confidence.
arXiv comment23 pages, 13 figures, submitted to ApJ
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