# Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$

**Authors:** Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue, Takuma Izumi, Michael A. Strauss, Masayuki Akiyama, Kentaro Aoki, Junya Arita, Xuheng Ding, Masatoshi Imanishi, Nobunari Kashikawa, Toshihiro Kawaguchi, Satoshi Kikuta, Kotaro Kohno, Chien-Hsiu Lee, Tohru Nagao, Camryn L. Phillips, Mahoshi Sawamura, John D. Silverman, Ayumi Takahashi, and Yoshiki Toba

arXiv: 2508.21229 · 2025-09-08

## TL;DR

This paper reports the discovery and spectroscopic confirmation of 54 new quasars and candidate obscured quasars at redshifts between 5.71 and 7.02, advancing understanding of the early universe during the epoch of reionization.

## Contribution

It presents the final major results from the SHELLQs project, identifying new low-luminosity quasars and candidates at high redshift using Subaru's Hyper Suprime-Cam survey.

## Key findings

- 54 new quasars and candidate obscured quasars identified at z=5.71-7.02
- Detection of additional objects including galaxies, brown dwarfs, and line emitters
- Spectroscopic confirmation of high-redshift quasars

## Abstract

We present spectroscopic identification of 43 quasars and 11 candidate obscured quasars in the epoch of reionization (EoR) at $5.71 \le z \le 7.02$, along with 29 galaxies at similar redshifts. This is the 24th publication from the Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs) project, which exploits the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) imaging survey to search for EoR quasars. The HSC-SSP survey has completed, and this paper is likely the final installment of major (unobscured) quasar discoveries from the SHELLQs project. In addition to the EoR objects, we identified five strong [O III] line emitters at $z < 1$, 30 Galactic brown dwarfs, and 14 passive galaxies at $z \sim 2$, which contaminated our sample of photometric quasar candidates. The present paper focuses on describing the immediate outcome of the spectroscopic observations, while a statistical analysis of the full SHELLQs sample will be presented in our next publication.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/2508.21229/full.md

## References

48 references — full list in the complete paper: https://tomesphere.com/paper/2508.21229/full.md

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Source: https://tomesphere.com/paper/2508.21229