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First Discoveries of z>6 Quasars with the DECam Legacy Survey and UKIRT Hemisphere Survey

Authors :
Wang, Feige
Fan, 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
Publication Year :
2017

Abstract

We present the first discoveries from a survey of $z\gtrsim6$ 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 $z_{\rm AB}\sim23.0$, and UKIDSS and UHS, which will map the northern sky at $0<DEC<+60^{\circ}$, reaching $J_{\rm VEGA}\sim19.6$ (5-$\sigma$). The combination of these datasets allows us to discover quasars at redshift $z\gtrsim7$ and to conduct a complete census of the faint quasar population at $z\gtrsim6$. In this paper, we report on the selection method of our search, and on the initial discoveries of two new, faint $z\gtrsim6$ quasars and one new $z=6.63$ quasar in our pilot spectroscopic observations. The two new $z\sim6$ quasars are at $z=6.07$ and $z=6.17$ with absolute magnitudes at rest-frame wavelength 1450 \AA\ 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 $z\gtrsim6$. 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 datasets to find $z\gtrsim7$ quasars. Extrapolating from previous QLF measurements, we predict that these combined datasets will yield $\sim200$ $z\sim6$ quasars to $z_{\rm AB} < 21.5$, $\sim1{,}000$ $z\sim6$ quasars to $z_{\rm AB}<23$, and $\sim 30$ quasars at $z>6.5$ to $J_{\rm VEGA}<19.5$.<br />Comment: 8 pages, 5 figures, accepted for publication in The Astrophysical Journal

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1703.07490
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-4357/aa689f