activity
20192022
most citedBalmer Break Galaxy Candidates at : a Potential View on the Star-Formation Activity at

29 citations · 72 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202212 cited

CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC

Takehiro Yoshioka, Nobunari Kashikawa, Akio K. Inoue +11

The spatial inhomogeneity is one of the important features for understanding the reionization process; however, it has not yet been fully quantified. To map this inhomogeneous dist…

astro-ph.GA2021

SILVERRUSH X: Machine Learning-Aided Selection of LAEs at , , , , , and from the HSC SSP and CHORUS Survey Data

Yoshiaki Ono, Ryohei Itoh, Takatoshi Shibuya +25

We present a new catalog of Ly emitter (LAE) candidates at , , , , , and that are photometrically selected by the SILVERRUSH program wi…

astro-ph.GA202018 cited

CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview

Akio K. Inoue, Satoshi Yamanaka, Masami Ouchi +28

To determine the dominant sources for cosmic reionization, the evolution history of the global ionizing fraction, and the topology of the ionized regions, we have conducted a deep…

astro-ph.GA2020

Testing an indirect method for identifying galaxies with high levels of Lyman continuum leakage

Satoshi Yamanaka, Akio K. Inoue, Toru Yamada +6

Using a sample of galaxies at with detected Lyman Continuum (LyC) leakage in the SSA22 field, we attempt to verify a proposed indirect method for identifying cases wit…

astro-ph.GA201929 cited

Balmer Break Galaxy Candidates at : a Potential View on the Star-Formation Activity at

Ken Mawatari, Akio K. Inoue, Takuya Hashimoto +15

We search for galaxies with a strong Balmer break (Balmer Break Galaxies; BBGs) at over a 0.41 deg effective area in the COSMOS field. Based on rich imaging data, in…

astro-ph.GA201913 cited

The UV spectral slope beta and stellar population of most active star-forming galaxies at z~4

Satoshi Yamanaka, Toru Yamada

We investigate the stellar population of star-forming galaxies at by focusing on their slope of rest-frame ultraviolet (UV) continuum, where . We in…