activity
20152022
most citedMAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5

85 citations · 457 across the 14 of their papers we have counts for

collaborators

18 papers

astro-ph.GA202244 cited

Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z=2.16

Jose Manuel Pérez-Martínez, Helmut Dannerbauer, Tadayuki Kodama +11

We use multi-object near-infrared (NIR) spectroscopy with VLT/KMOS to investigate the role of the environment in the evolution of the ionized gas properties of narrow-band selected…

astro-ph.GA20211 cited

Environmental dependence of gas properties in a protocluster at z~2.5

Kohei Aoyama, Tadayuki Kodama, Tomoko L. Suzuki +5

In a protocluster USS1558-003 at z=2.53, galaxies in the dense cores show systematically elevated star-forming activities than those in less dense regions. To understand its origin…

astro-ph.GA202019 cited

Dust, gas, and metal content in star-forming galaxies at revealed with ALMA and Near-IR spectroscopy

Tomoko L. Suzuki, Masato Onodera, Tadayuki Kodama +8

We conducted sub-millimeter observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) of star-forming galaxies at , whose gas-phase metallicities have be…

astro-ph.GA2020

Broad-band selection, spectroscopic identification, and physical properties of a population of extreme emission line galaxies at 3<z<3.7

Masato Onodera, Rhythm Shimakawa, Tomoko L. Suzuki +7

We present the selection, spectroscopic identification, and physical properties of extreme emission line galaxies (EELGs) at aiming at studying physical properties of an…

astro-ph.GA202082 cited

Structural evolution in massive galaxies at z~2

Ken-ichi Tadaki, Sirio Belli, Andreas Burkert +18

We present 0.2arcsec-resolution Atacama Large Millimeter/submillimeter Array observations at 870 m in a stellar mass-selected sample of 85 massive ($M_\mathrm{star}>10^{11}~M_\o…

astro-ph.GA20204 cited

Environmental impact on star-forming galaxies in a cluster during course of galaxy accretion

Tetsuro Asano, Tadayuki Kodama, Kentaro Motohara +18

Galaxies change their properties as they assemble into clusters. In order to understand the physics behind that, we need to go back in time and observe directly what is occurring i…