activity
20122026
most citedQuiescent galaxies 1.5 billion years after the Big Bang and their progenitors

206 citations · 1.9k across the 52 of their papers we have counts for

collaborators

52 papers

astro-ph.GA2026

DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Overdensities

Takumi Kakimoto, Masayuki Tanaka, Kei Ito +20

We report on the spectroscopic confirmation of overdense regions of massive quiescent galaxies (QGs) in the early Universe with JWST/NIRSpec. Based on data from the DeepDive NIRSpe…

astro-ph.GA2026

The role of small-scale environments in the quenching of massive galaxies at

Takumi Kakimoto, Masayuki Tanaka, Makoto Ando +10

Massive quiescent galaxies (QGs) at high redshifts are likely progenitors of massive elliptical galaxies in the local Universe. Recent discoveries of high-redshift QGs in overdensi…

astro-ph.GA2026

The ionised interstellar medium of DSFGs revealed by JWST/NIRSpec and ALMA: Super-solar metallicity, low ionisation parameters and, typical electron densities

Steven Gillman, Kei Ito, Francesco Valentino +25

We present a detailed study of near-infrared (2-4m) JWST/NIRSpec spectra of 48 high-redshift () galaxies detected with ALMA at . From a multi-wa…

astro-ph.GA2025★ 2 cited

Environment of SDSS quasars at explored by Subaru HSC

Kohei Shibata, Tohru Nagao, Hisakazu Uchiyama +5

The relationship between quasars and their galaxy environment is important for understanding the evolution of galaxies and supermassive black holes, but it is not fully understood.…

astro-ph.GA2024

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X. The Massive and Passive Nature of Radio Galaxies at

Yuta Yamamoto, Tohru Nagao, Takuji Yamashita +8

High- radio galaxies (HzRGs) are considered important objects for understanding the formation and evolution of massive galaxies in the early universe. However, till date, detail…

astro-ph.GA2024

Mining for Protoclusters at from Photometric Datasets with Deep Learning

Yoshihiro Takeda, Nobunari Kashikawa, Kei Ito +9

Protoclusters are high- overdense regions that will evolve into clusters of galaxies by , making them ideal for studying galaxy evolution expected to be accelerated by envi…

astro-ph.GA2024

ADF22-WEB: A giant barred spiral starburst galaxy in the z = 3.1 SSA22 protocluster core

H. Umehata, C. C. Steidel, I. Smail +15

In the present-day universe, the most massive galaxies are ellipticals located in the cores of galaxy clusters, harboring the heaviest super-massive black holes (SMBHs). However th…

astro-ph.GA2024

Galaxy properties from the outskirts to the core of a protocluster at z=3.699

Jun Toshikawa, Stijn Wuyts, Nobunari Kashikawa +6

We present follow-up spectroscopy on a protocluster candidate selected from the wide-field imaging of the Hyper SuprimeCam Subaru Strategic Programme. The target protocluster candi…

astro-ph.GA2023★ 1 cited

A proto-cluster of massive quiescent galaxies at z=4

Masayuki Tanaka, Masato Onodera, Rhythm Shimakawa +7

We report on discovery of a concentration of massive quiescent galaxies located at z=4. The concentration is first identified using high-quality photometric redshifts based on deep…

astro-ph.GA2023

New technique to select recent fast-quenching galaxies at using the optical colors

Mariko Kubo, Tohru Nagao, Hisakazu Uchiyama +4

Many massive quiescent galaxies have been discovered at thanks to multi-wavelength deep and wide surveys, however, substantial deep near-infrared spectroscopic observations a…

astro-ph.GA2023

An enhanced abundance of bright galaxies in protocluster candidates at z~3-5

Jun Toshikawa, Stijn Wuyts, Nobunari Kashikawa +11

We present a protocluster search covering to based on the combination of the Hyper SuprimeCam Subaru Strategic Programme and the CFHT Large Area -band Deep Sur…

astro-ph.GA2023★ 1 cited

A massive quiescent galaxy in a group environment at

Takumi Kakimoto, Masayuki Tanaka, Masato Onodera +10

We report on the spectroscopic confirmation of a massive quiescent galaxy at in the COSMOS field. The object was first identified as a galaxy with suppressed…

astro-ph.GA2023★ 5 cited

Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at in Public Fields

Kei Ito, Francesco Valentino, Gabriel Brammer +19

We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at using the Near-Infrared Camera (NIRCam) onboard . Based…

astro-ph.GA2023★ 16 cited

Revisiting the Properties of X-ray AGN in the SSA22 Protocluster: Normal SMBH and Host-Galaxy Growth for AGN in a Overdensity

Erik B. Monson, Keith Doore, Rafael T. Eufrasio +6

We analyze the physical properties of 8 X-ray selected active galactic nuclei (AGN) and one candidate protoquasar system (ADF22A1) in the SSA22 protocluster by fitting t…

astro-ph.GA2023★ 204 cited

An Atlas of Color-selected Quiescent Galaxies at in Public Fields

Francesco Valentino, Gabriel Brammer, Katriona M. L. Gould +24

We present the results of a systematic search for candidate quiescent galaxies in the distant Universe in eleven fields with publicly available observations collected during…

astro-ph.GA2023★ 52 cited

COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at

Kei Ito, Masayuki Tanaka, Francesco Valentino +9

Protoclusters of galaxies have been found in the last quarter century. However, most of them have been found through the overdensity of star-forming galaxies, and there had been no…

astro-ph.GA2022★ 6 cited

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IX. The Most Overdense Region at z~5 Inhabited by a Massive Radio Galaxy

Hisakazu Uchiyama, Takuji Yamashita, Tohru Nagao +13

We report on the galaxy density environment around a high-z radio galaxy (HzRG) at z=4.72, HSC J083913.17+011308.1 (HSC J0839+0113), probed using an r-dropout Lyman break galaxy (L…

astro-ph.GA2022★ 25 cited

An AGN with an ionized gas outflow in a massive quiescent galaxy in a protocluster at

Mariko Kubo, Hideki Umehata, Yuichi Matsuda +13

We report the detection of an ionized gas outflow from an -ray active galactic nucleus (AGN) hosted in a massive quiescent galaxy in a protocluster at (J221737.29+00182…

astro-ph.GA2022★ 11 cited

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z=0.3-1.4

Hisakazu Uchiyama, Takuji Yamashita, Tohru Nagao +9

We examine the redshift evolution of density environments around 2,163 radio galaxies with the stellar masses of between redshifts of , base…

astro-ph.GA2021★ 12 cited

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4

Hisakazu Uchiyama, Takuji Yamashita, Jun Toshikawa +13

We present the environmental properties around high- radio galaxies (HzRGs) at , which have been poorly investigated because of their rarity. We use the largest samples…

astro-ph.GA2021★ 16 cited

ALMA Observations of Lyman-alpha Blob 1: Multiple major-mergers and widely distributed interstellar media

Hideki Umehata, Ian Smail, Charles C. Steidel +11

We present observations of a giant Lyman-alpha blob in the SSA22 proto-cluster at z=3.1, SSA22-LAB1, taken with the Atacama Large Millimeter/submillimeter Array (ALMA). Dust contin…

astro-ph.GA2021★ 4 cited

A massive quiescent galaxy confirmed in a protocluster at z=3.09

Mariko Kubo, Hideki Umehata, Yuichi Matsuda +10

We report a massive quiescent galaxy at spectroscopically confirmed at a protocluster in the SSA22 field by detecting the Balmer and Ca {\fo…

astro-ph.GA2021★ 21 cited

On the Nature of AGN and Star Formation Enhancement in the SSA22 Protocluster: The HST WFC3 IR View

Erik B. Monson, Bret D. Lehmer, Keith Doore +9

We examine possible environmental sources of the enhanced star formation and active galactic nucleus (AGN) activity in the SSA22 protocluster using Hubble WFC3 F160W ($\…

astro-ph.GA2021★ 16 cited

Interrelation of the environment of Ly emitters and massive galaxies at

Kei Ito, Nobunari Kashikawa, Masayuki Tanaka +7

We present a comparison of the spatial distributions of Ly emitters (LAEs) and massive star-forming and quiescent galaxies (SFGs and QGs) at . We use the photometric re…