activity
20142025
most citedBulge-forming galaxies with an extended rotating disk at z~2

130 citations · 590 across the 17 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2023

Spatial extent of molecular gas, dust, and stars in massive galaxies at z=2-2.5 determined with ALMA and JWST

Ken-ichi Tadaki, Tadayuki Kodama, Yusei Koyama +3

We present the results of 0.6"-resolution observations of CO J=3-2 line emission in 10 massive star-forming galaxies at z=2.2-2.5 with the Atacama Large Millimeter/submillimeter Ar…

astro-ph.GA2023

GALAXY CRUISE: Deep Insights into Interacting Galaxies in the Local Universe

Masayuki Tanaka, Michitaro Koike, Sei'ichiro Naito +15

We present the first results from GALAXY CRUISE, a community (or citizen) science project based on data from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). The current p…

astro-ph.CO2023

GREX-PLUS Science Book

PLUS Science Team, Akio K. Inoue, Yuichi Harikane +28

GREX-PLUS (Galaxy Reionization EXplorer and PLanetary Universe Spectrometer) is a mission candidate for a JAXA's strategic L-class mission to be launched in the 2030s. Its primary…

astro-ph.IM202321 cited

Estimating the statistical uncertainty due to spatially correlated noise in interferometric images

Takafumi Tsukui, Satoru Iguchi, Ikki Mitsuhashi +1

Interferometers (e.g. ALMA and NOEMA) allow us to obtain the detailed brightness distribution of astronomical sources in 3 dimensions (R.A., Dec., frequency). However, the spatial…

astro-ph.IM2022

Proper evaluation of spatially correlated noise in interferometric images

Takafumi Tsukui, Satoru Iguchi, Ikki Mitsuhashi +1

Recent interferometers (e.g. ALMA and NOEMA) allow us to obtain the detailed brightness distribution of the astronomical sources in 3 dimension (R.A., Dec., frequency). However, th…

astro-ph.GA2016108 cited

Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2

M. Fossati, D. J. Wilman, J. T. Mendel +25

We make publicly available a catalog of calibrated environmental measures for galaxies in the five 3D-HST/CANDELS deep fields. Leveraging the spectroscopic and grism redshifts from…