Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9
Yoshiki Matsuoka, Masafusa Onoue, Nobunari Kashikawa, Kazushi Iwasawa,, Michael A. Strauss, Tohru Nagao, Masatoshi Imanishi, Mana Niida, Yoshiki, Toba, Masayuki Akiyama, Naoko Asami, James Bosch, S\'ebastien Foucaud,, Hisanori Furusawa, Tomotsugu Goto, James E. Gunn

TL;DR
This paper reports the discovery of 15 high-redshift quasars and galaxies at z > 5.7 using Subaru HSC data, demonstrating the effectiveness of their selection method and revealing the faint end of the early universe's luminosity function.
Contribution
First discovery of low-luminosity quasars and bright galaxies at z > 5.7 using Subaru HSC data, with a high success rate and implications for the early universe's luminosity function.
Findings
Discovered 15 high-z objects, including quasars and galaxies.
High photometric selection success rate (~100% at bright magnitudes).
Evidence for the steep rise of the galaxy luminosity function at z > 6.
Abstract
We report the discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9. This is the initial result from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, which exploits the exquisite multiband imaging data produced by the Subaru Hyper Suprime-Cam (HSC) Strategic Program survey. The candidate selection is performed by combining several photometric approaches including a Bayesian probabilistic algorithm to reject stars and dwarfs. The spectroscopic identification was carried out with the Gran Telescopio Canarias and the Subaru Telescope for the first 80 deg2 of the survey footprint. The success rate of our photometric selection is quite high, approaching 100 % at the brighter magnitudes (zAB < 23.5 mag). Our selection also recovered all the known high-z quasars on the HSC images. Among the 15 discovered objects, six are likely quasars, while the other six with…
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