4.6 Article

THE FIRST HIGH-REDSHIFT QUASAR FROM Pan-STARRS

Journal

ASTRONOMICAL JOURNAL
Volume 143, Issue 6, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/143/6/142

Keywords

early Universe; quasars: individual (PSO J215.1512-16.0417); surveys

Funding

  1. National Aeronautics and Space Administration through the Planetary Science Division of the NASA Science Mission Directorate [NNX08AR22G]
  2. Deutsche Forschungsgemeinschaft [1177]
  3. Germany's national research center for aeronautics and space (DLR) [FKZ 50 OR 1104]
  4. Leibniz-Prize (DFG) [HA 1850/28-1]
  5. Division Of Astronomical Sciences
  6. Direct For Mathematical & Physical Scien [806861] Funding Source: National Science Foundation

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We present the discovery of the first high-redshift (z > 5.7) quasar from the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1 or PS1). This quasar was initially detected as an i(P1) dropout in PS1, confirmed photometrically with the SAO Wide-field InfraRed Camera at Arizona's Multiple Mirror Telescope (MMT) and the Gamma-Ray Burst Optical/Near-Infrared Detector at the MPG 2.2 m telescope in La Silla. The quasar was verified spectroscopically with the MMT Spectrograph, Red Channel and the Cassegrain Twin Spectrograph at the Calar Alto 3.5 m telescope. Its near-infrared spectrum was taken at the Large Binocular Telescope Observatory (LBT) with the LBT Near-Infrared Spectroscopic Utility with Camera and Integral Field Unit for Extragalactic Research. It has a redshift of 5.73, an AB z(P1) magnitude of 19.4, a luminosity of 3.8 x 10(47) erg s(-1), and a black hole mass of 6.9 x 10(9) M-circle dot. It is a broad absorption line quasar with a prominent Ly beta peak and a very blue continuum spectrum. This quasar is the first result from the PS1 high-redshift quasar search that is projected to discover more than 100 i(P1) dropout quasars and could potentially find more than 10 z(P1) dropout (z > 6.8) quasars.

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