THE PAN-STARRS1 DISTANT z > 5.6 QUASAR SURVEY: MORE THAN 100 QUASARS WITHIN THE FIRST GYR OF THE UNIVERSE
Venemans, B. P.
Farina, E. P.
Chambers, K. C.
Rosa, G. De
Burgett, W. S.
Draper, P. W.
Hodapp, K. W.
Jun, H. D.
Tonry, J. L.
Wainscoat, R. J.
AffiliationUniv Arizona, Steward Observ
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PublisherIOP PUBLISHING LTD
CitationTHE PAN-STARRS1 DISTANT z > 5.6 QUASAR SURVEY: MORE THAN 100 QUASARS WITHIN THE FIRST GYR OF THE UNIVERSE 2016, 227 (1):11 The Astrophysical Journal Supplement Series
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AbstractLuminous quasars at z > 5.6 can be studied in detail with the current generation of telescopes and provide us with unique information on the first gigayear of the universe. Thus far, these studies have been statistically limited by the number of quasars known at these redshifts. Such quasars are rare, and therefore, wide-field surveys are required to identify them, and multiwavelength data are required to separate them efficiently from their main contaminants, the far more numerous cool dwarfs. In this paper, we update and extend the selection for the z similar to 6 quasars presented in Banados et al. (2014) using the Pan- STARRS1 (PS1) survey. We present the PS1 distant quasar sample, which currently consists of 124 quasars in the redshift range 5.6 less than or similar to z less than or similar to 6.7 that satisfy our selection criteria. Of these quasars, 77 have been discovered with PS1, and 63 of them are newly identified in this paper. We present the composite spectra of the PS1 distant quasar sample. This sample spans a factor of similar to 20 in luminosity and shows a variety of emission line properties. The number of quasars at z > 5.6 presented in this work almost doubles the previously known quasars at these redshifts, marking a transition phase from studies of individual sources to statistical studies of the high-redshift quasar population, which was impossible with earlier, smaller samples.
VersionFinal published version
SponsorsNSF [AST-9987045]; NSF Telescope System Instrumentation Program; Ohio Board of Regents; Ohio State University Office of Research; Leibniz Prize (DFG) [HA 1850/28-1]; National Aeronautics and Space Administration