activity
20172020
most citedGas clump formation via thermal instability in high-redshift dwarf galaxy mergers

16 citations · 16 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020

Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era

Shohei Arata, Hidenobu Yajima, Kentaro Nagamine +2

Recent observations have successfully detected [O III] and [C II] lines from galaxies in the early Universe with the Atacama Large Millimeter Arr…

astro-ph.GA2019

Galaxy evolution and radiative properties in the early Universe: multi-wavelength analysis in cosmological simulations

Shohei Arata, Hidenobu Yajima, Kentaro Nagamine +2

Recent observations have successfully detected UV or infrared flux from galaxies at the epoch of reionization. However, the origin of their radiative properties has not been fully…

astro-ph.GA2019

CHORUS. III. Photometric and Spectroscopic Properties of Ly Blobs at

Haibin Zhang, Masami Ouchi, Ryohei Itoh +20

We report the Subaru Hyper Suprime-Cam (HSC) discovery of two Ly blobs (LABs), dubbed z70-1 and z49-1 at and respectively, that are Ly emitters with a bri…

astro-ph.GA2019

First Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7

Seiji Fujimoto, Masami Ouchi, Andrea Ferrara +7

We report the discovery of 10-kpc scale [CII] 158um halos surrounding star-forming galaxies in the early Universe. We choose deep ALMA data of 18 galaxies each with a star-formatio…

astro-ph.GA2018

Radiative properties of the first galaxies: rapid transition between blue and red

Shohei Arata, Hidenobu Yajima, Kentaro Nagamine +2

Recent observations have successfully detected UV-bright and infrared-bright galaxies in the epoch of reionization. However, the origin of their radiative properties has not been u…

astro-ph.GA201716 cited

Gas clump formation via thermal instability in high-redshift dwarf galaxy mergers

Shohei Arata, Hidenobu Yajima, Kentaro Nagamine

Star formation in high-redshift dwarf galaxies is a key to understand early galaxy evolution in the early Universe. Using the three-dimensional hydrodynamics code GIZMO, we study t…