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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…
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…
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…
A Planck-selected dusty proto-cluster at z=2.16 associated with a strong over-density of massive H emitting galaxies
Yusei Koyama, Maria del Carmen Polletta, Ichi Tanaka +6
We discovered an over-density of H-alpha-emitting galaxies associated with a Planck compact source in the COSMOS field (PHzG237.0+42.5) through narrow-band imaging observations wit…
A 16 deg survey of emission-line galaxies at z<1.6 from HSC-SSP PDR2 and CHORUS
Masao Hayashi, Rhythm Shimakawa, Masayuki Tanaka +7
We have conducted a comprehensive survey of emission-line galaxies at based on narrowband (NB) imaging data taken with Hyper Suprime-Cam (HSC) on the Subaru telescop…
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…