The Pan-STARRS1 distant z>5.6 quasar survey: more than 100 quasars within the first Gyr of the universe
arXiv:1608.03279 · doi:10.3847/0067-0049/227/1/11
Abstract
Luminous 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 needed to separate them efficiently from their main contaminants, the far more numerous cool dwarfs. In this paper, we update and extend the selection for z~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<z<6.7 that satisfy our selection criteria. Seventy-seven of these quasars have been discovered with PS1, and 63 of them are newly identified in this paper. We present composite spectra of the PS1 distant quasar sample. This sample spans a factor of ~20 in luminosity and shows a variety of emission line properties. The number of quasars at z>5.6 presented in this work almost double the quasars previously known 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.
arXiv commentAccepted by ApJS. Machine readable tables and an up-to-date census of z>5.6 quasars are available at https://users.obs.carnegiescience.edu/~ebanados/high-z-qsos.html
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- VEXAS: VISTA EXtension to Auxiliary Surveys -- Data Release 2: Machine-learning based classification of sources in the Southern Hemisphere
- Prospects for Observing High-redshift Radio-loud Quasars in the SKA Era: Paving the Way for 21-cm Forest Observations
- Possible evolution of the circum-galactic medium around QSOs with QSO age and cosmic time revealed by Ly halos
- The host galaxies of radio-loud quasars at z>5 with ALMA
- High Star Formation Rates of Low Eddington Ratio Quasars at
- A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
- Multi-wavelength properties of three new radio-powerful quasi-stellar objects discovered from RACS
- The benefit of simultaneous seven-filter imaging: 10 years of GROND observations
- A variable active galactic nucleus at triply-imaged by the galaxy cluster MACS J0035.4-2015
- When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data
- VEXAS: the VISTA EXtension to Auxiliary Surveys -- Data Release 1: the Southern Galactic Hemisphere
- The Infrared Medium-deep Survey. IX. Discovery of Two New Quasars and Space Density down to mag
- Structure of the super-Eddington outflow and itsimpact on the cosmological scale
- The Decoupled Kinematics of high-z QSO Host Galaxies and their Lya halos
- Optical and near-infrared spectroscopy of quasars at : public data release and composite spectrum
- Effects of the Hubble Parameter on the Cosmic Growth of the First Quasars
- Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
- Comprehensive view on a radio-loud QSO: from the radio to the optical/NIR to the X-ray band
- Strong Lensed QSOs with Variability Detectable by LSST: How many are there?
- Plausible association of distant late M dwarfs with low-frequency radio emission
- High- Universe probed via Lensing by QSOs (HULQ) I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
- Revealing new high redshift quasar populations through Gaussian mixture model selection
- An Optically Faint Quasar Survey at z~5 in the CFHTLS Wide Field: Estimates of the Black Hole Masses and Eddington Ratios
- High- radio Quasars in RACS I: Selection, identification, and multi-wavelength properties
- Astrophysics with the Laser Interferometer Space Antenna
- HYPERION: broad-band X-ray-to-near-infrared emission of Quasars in the first billion years of the Universe
- High-redshift quasar selection from the CFHQSIR survey
- Revealing faint compact radio jets at redshifts above 5 with very long baseline interferometry
- Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
- Euclid: The potential of slitless infrared spectroscopy: A z=5.4 quasar and new ultracool dwarfs
- Galaxies into the Dark Ages
- The Dawn of Black Holes
- JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system
- The quasar luminosity function at via deep learning and Bayesian information criterion
- Rapidly accreting black hole of the Lyα-luminous quasar PSO J006.1240+39.2219
- Searching for [CII] Emission from the First Sample of OI Absorption-Associated Galaxies with ALMA
- A method for checking high-redshift identification of radio AGNs
- Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
- Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
- Discovery of two quasars at from the OGLE Survey
- Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.1292
- Lensing in the Darkness: A Bayesian Analysis of 22 Chandra Sources at Shows No Evidence of Lensing
- The clustering of C IV and Si IV at the end of reionisation: A perspective from the E-XQR-30 survey
- 4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < < 7) selected with SED fitting
- Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4
- Gemini Near Infrared SpectrographDistant Quasar Survey: the Chandra View
- Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
- A Super-Eddington, Lensing-Magnified Quasar at observed with JWST
- Black Hole merger rates in the first billion years in light of JWST data
- X-Ray Evidence Against the Hypothesis that the Hyper-Luminous z=6.3 Quasar J0100+2802 is Lensed
- The Impact of Powerful Jets on the Far-infrared Emission of an Extreme Radio Quasar at z~6
- Quasar clustering at redshift 6
- High- Universe probed via Lensing by QSOs (HULQ) II. Deep GMOS spectroscopy of a QSO lens candidate
- ALMA Observations of the Sub-kpc Structure of the Host Galaxy of a z= 6.5 Lensed Quasar: A Rotationally-Supported Hyper-Starburst System at the Epoch of Reionization
- X-HESS: a large sample of highly accreting serendipitous AGN under the XMM-Newton microscope
- Can X-ray Observations Improve Optical-UV-based Accretion-Rate Estimates for Quasars?