# Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV.   Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.9

**Authors:** 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, T. Minezaki, S. Miyazaki, T., Morokuma, H. Murayama, M. Niida, A. J. Nishizawa, M. Oguri, Y. Ono, M. Ouchi,, P. A. Price, H. Sameshima, A. Schulze, H. Shirakata, J. D. Silverman, N., Sugiyama, P. J. Tait, M. Takada, T. Takata, M. Tanaka, J.-J. Tang, Y. Toba,, Y. Utsumi, S.-Y. Wang, and T. Yamashita

arXiv: 1803.01861 · 2018-07-18

## 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.

## Key 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 M1450 ~ -26 to -22 mag, and continue to populate a few magnitude lower luminosities than have been probed by previous wide-field surveys. In a companion paper, we derive the quasar luminosity function at z ~ 6 over an unprecedentedly wide range of M1450 ~ -28 to -21 mag, exploiting the SHELLQs and other survey outcomes.

## Full text

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## Figures

22 figures with captions in the complete paper: https://tomesphere.com/paper/1803.01861/full.md

## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1803.01861/full.md

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Source: https://tomesphere.com/paper/1803.01861