First Discoveries of z > 6 Quasars with the DECam Legacy Survey and UKIRT Hemisphere Survey
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Author
Wang, FeigeFan, Xiaohui
Yang, Jinyi
Wu, Xue-Bing
Yang, Qian
Bian, Fuyan
McGreer, Ian D.
Li, Jiang-Tao
Li, Zefeng
Ding, Jiani
Dey, Arjun
Dye, Simon
Findlay, Joseph R.
Green, Richard
James, David
Jiang, Linhua
Lang, Dustin
Lawrence, Andy
Myers, Adam D.
Ross, Nicholas P.
Schlegel, David J.
Shanks, Tom
Affiliation
Univ Arizona, Steward ObservIssue Date
2017-04-11
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First Discoveries of z > 6 Quasars with the DECam Legacy Survey and UKIRT Hemisphere Survey 2017, 839 (1):27 The Astrophysical JournalJournal
The Astrophysical JournalRights
© 2017. The American Astronomical Society. All rights reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We present the first discoveries from a survey of z greater than or similar to 6 quasars using imaging data from the DECam Legacy Survey (DECaLS) in the optical, the UKIRT Deep Infrared Sky Survey (UKIDSS) and a preliminary version of the UKIRT Hemisphere Survey (UHS) in the near-IR, and ALLWISE in the mid-IR. DECaLS will image 9000 deg(2) of sky down to z(AB) similar to 23.0, and UKIDSS and UHS will map the northern sky at 0 < decl. < + 60 degrees, reaching J(VEGA) similar to 19.6 (5-sigma). The combination of these data sets allows us to discover quasars at redshift z greater than or similar to 7 and to conduct a complete census of the faint quasar population at z greater than or similar to 6. In this paper, we report on the selection method of our search, and on the initial discoveries of two new, faint z greater than or similar to 6 quasars and one new z = 6.63 quasar in our pilot spectroscopic observations. The two new z similar to 6 quasars are at z = 6.07 and z = 6.17 with absolute magnitudes at rest-frame wavelength 1450 angstrom being M-1450 = -25.83 and M-1450 = -25.76, respectively. These discoveries suggest that we can find quasars close to or fainter than the break magnitude of the Quasar Luminosity Function (QLF) at z greater than or similar to 6. The new z = 6.63 quasar has an absolute magnitude of M-1450 = -25.95. This demonstrates the potential of using the combined DECaLS and UKIDSS/UHS data sets to find z greater than or similar to 7 quasars. Extrapolating from previous QLF measurements, we predict that these combined data sets will yield similar to 200 z similar to 6 quasars to z(AB) < 21.5, similar to 1000 z similar to 6 quasars to z(AB) < 23, and similar to 30 quasars at z > 6.5 to J(VEGA) < 19.5.ISSN
1538-4357Version
Final published versionSponsors
NSFC [11373008, 11533001]; National Key Basic Research Program of China [2014CB845700]; US NSF [AST 15-15115]; Ministry of Science and Technology of China [2016YFA0400703]; STFC; Ernest Rutherford Fellowship scheme; Strategic Priority Research Program "The Emergence of Cosmological Structures", National Astronomical Observatories, Chinese Academy of Sciences [XDB09000000]; Special Fund for Astronomy from the Ministry of FinanceAdditional Links
http://stacks.iop.org/0004-637X/839/i=1/a=27?key=crossref.659d362b0d97bc805aa686437a5fa0c6ae974a485f413a2113503eed53cd6c53
10.3847/1538-4357/aa689f