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

**Authors:** Feige Wang, Xiaohui Fan, Jinyi Yang, Xue-Bing Wu, Qian Yang, Fuyan, Bian, Ian D. McGreer, Jiang-Tao Li, Zefeng Li, Jiani Ding, Arjun Dey, Simon, Dye, Joseph R. Findlay, Richard Green, David James, Linhua Jiang, Dustin, Lang, Andy Lawrence, Adam D. Myers, Nicholas P. Ross, David J. Schlegel, Tom, Shanks

arXiv: 1703.07490 · 2017-04-19

## TL;DR

This paper reports the initial discovery of faint quasars at redshifts greater than 6 using combined optical, near-infrared, and mid-infrared survey data, demonstrating the potential to identify quasars near the epoch of reionization.

## Contribution

It introduces a new survey method combining DECaLS, UKIDSS, and UHS datasets to efficiently find high-redshift quasars, including very faint ones, expanding the known quasar population at z>6.

## Key findings

- Discovered two new faint quasars at z~6.
- Identified a quasar at z=6.63 with significant luminosity.
- Predicted discovery of hundreds of z~6 quasars with future data.

## 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 $J_{\rm VEGA}<19.5$.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1703.07490/full.md

## References

53 references — full list in the complete paper: https://tomesphere.com/paper/1703.07490/full.md

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Source: https://tomesphere.com/paper/1703.07490