Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.9
Y. Matsuoka, K. Iwasawa, M. Onoue, N. Kashikawa, M. A. Strauss, C.-H., Lee, M. Imanishi, T. Nagao, M. Akiyama, N. Asami, J. Bosch, H. Furusawa, T., Goto, J. E. Gunn, Y. Harikane, H. Ikeda, T. Izumi, T. Kawaguchi, N. Kato, S., Kikuta, K. Kohno, Y. Komiyama, R. H. Lupton

TL;DR
This paper reports the discovery of 41 new high-redshift quasars and luminous galaxies, expanding the known population at 5.7 < z < 6.9 and probing lower luminosities than previous surveys, based on deep imaging and follow-up spectroscopy.
Contribution
It presents a large, spectroscopically confirmed sample of high-z quasars and galaxies, utilizing a Bayesian selection method and deep imaging data from the SHELLQs project, with implications for the quasar luminosity function.
Findings
Discovery of 41 new high-z quasars and luminous galaxies.
Sample spans a wide luminosity range, including lower luminosities.
Provides data for deriving the quasar luminosity function at z ~ 6.
Abstract
We report discovery of 41 new high-z quasars and luminous galaxies, which were spectroscopically identified at 5.7 < z < 6.9. This is the fourth in a series of papers from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, based on the deep multi-band imaging data collected by the Hyper Suprime-Cam (HSC) Subaru Strategic Program survey. We selected the photometric candidates by a Bayesian probabilistic algorithm, and then carried out follow-up spectroscopy with the Gran Telescopio Canarias and the Subaru Telescope. Combined with the sample presented in the previous papers, we have now spectroscopically identified 137 extremely-red HSC sources over about 650 deg2, which include 64 high-z quasars, 24 high-z luminous galaxies, 6 [O III] emitters at z ~ 0.8, and 43 Galactic cool dwarfs (low-mass stars and brown dwarfs). The new quasars span the luminosity range from…
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