activity
20142025
most citedUpper limits on the mass and luminosity of Population III-dominated galaxies

26 citations · 87 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023

FOREVER22: Gas and metal outflow from massive galaxies in protocluster regions

Naoki Harada, Hidenobu Yajima, Makito Abe

We study gas and metal outflow from massive galaxies in protocluster regions at by using the results of the FOREVER22 simulation project. Our simulations contain massive ha…

astro-ph.GA20236 cited

Detections of [C II] 158 m and [O III] 88 m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies

Ryota Ura, Takuya Hashimoto, Akio K. Inoue +17

We present integral field, far-infrared (FIR) spectroscopy of Mrk 54, a local Lyman Continuum Emitter (LCE), obtained with FIFI-LS on the Stratospheric Observatory for Infrared Ast…

astro-ph.CO202317 cited

Exploring the cosmic dawn and epoch of reionization with 21cm line

Hayato Shimabukuro, Kenji Hasegawa, Akira Kuchinomachi +2

The dark age of the universe, when no luminous object had existed, ended with the birth of the first stars, galaxies, and blackholes. This epoch is called cosmic dawn. Cosmic reion…

astro-ph.GA20239 cited

UV & Ly halos of Ly emitters across environments at z=2.84

Satoshi Kikuta, Yuichi Matsuda, Shigeki Inoue +7

We present UV and Ly radial surface brightness (SB) profiles of Ly emitters (LAEs) at detected with the Hyper Suprime-Cam (HSC) on the Subaru Telescope. The depth of…

astro-ph.GA201626 cited

Upper limits on the mass and luminosity of Population III-dominated galaxies

Hidenobu Yajima, Sadegh Khochfar

We here derive upper limits on the mass and luminosity of Population III (POPIII) dominated proto-galaxies based on the collapse of primordial gas under the effect of angular momen…

astro-ph.CO201422 cited

Can the 21 cm signal probe Population III and II star formation?

Hidenobu Yajima, Sadegh Khochfar

Using varying models for the star formation rate (SFR) of Population (Pop) III and II stars at z>6 we derive the expected redshift history of the global 21 cm signal from the inter…