Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0

Author:

Matsuoka YoshikiORCID,Iwasawa KazushiORCID,Onoue MasafusaORCID,Izumi TakumaORCID,Kashikawa NobunariORCID,Strauss Michael A.ORCID,Imanishi MasatoshiORCID,Nagao TohruORCID,Akiyama MasayukiORCID,Silverman John D.ORCID,Asami Naoko,Bosch JamesORCID,Furusawa HisanoriORCID,Goto Tomotsugu,Gunn James E.,Harikane YuichiORCID,Ikeda HiroyukiORCID,Ishimoto RikakoORCID,Kawaguchi ToshihiroORCID,Kato Nanako,Kikuta SatoshiORCID,Kohno KotaroORCID,Komiyama YutakaORCID,Lee Chien-HsiuORCID,Lupton Robert H.ORCID,Minezaki TakeoORCID,Miyazaki SatoshiORCID,Murayama HitoshiORCID,Nishizawa Atsushi J.ORCID,Oguri MasamuneORCID,Ono YoshiakiORCID,Ouchi MasamiORCID,Price Paul A.ORCID,Sameshima HiroakiORCID,Sugiyama Naoshi,Tait Philip J.,Takada MasahiroORCID,Takahashi Ayumi,Takata TadafumiORCID,Tanaka MasayukiORCID,Toba YoshikiORCID,Utsumi YousukeORCID,Wang Shiang-YuORCID,Yamashita TakujiORCID

Abstract

Abstract We present the spectroscopic discovery of 69 quasars at 5.8 < z < 7.0, drawn from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) imaging survey data. This is the 16th publication from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, and it completes identification of all but the faintest candidates (i.e., i-band dropouts with z AB < 24 and y-band detections, and z-band dropouts with y AB < 24) with Bayesian quasar probability P Q B > 0.1 in the HSC-SSP third public data release (PDR3). The sample reported here also includes three quasars with P Q B < 0.1 at z ∼ 6.6, which we selected in an effort to completely cover the reddest point sources with simple color cuts. The number of high-z quasars discovered in SHELLQs has now grown to 162, including 23 type II quasar candidates. This paper also presents identification of seven galaxies at 5.6 < z < 6.7, an [O iii] emitter at z = 0.954, and 31 Galactic cool stars and brown dwarfs. High-z quasars and galaxies compose 75% and 16%, respectively, of all the spectroscopic SHELLQs objects that pass our latest selection algorithm with the PDR3 photometry. That is, a total of 91% of the objects lie at z > 5.6. This demonstrates that the algorithm has very high efficiency, even though we are probing an unprecedentedly low luminosity population down to M 1450 ∼ −21 mag.

Funder

MEXT ∣ Japan Society for the Promotion of Science

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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