activity
19982023
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 914 across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.GA2023★ 10 cited

X3: a high-mass Young Stellar Object close to the supermassive black hole Sgr~A*

Florian Peißker, Michal Zajacek, Nadeen B. Sabha +10

To date, the proposed observation of Young Stellar Objects (YSOs) in the Galactic center (GC) still raises the question where and how these objects could have formed due to the vio…

astro-ph.GA2022★ 6 cited

ALMA Astrometry of the Objects within 0.5 pc of Sagittarius A

Masato Tsuboi, Takahiro Tsutsumi, Atsushi Miyazaki +2

Atacama Large Millimeter/Submillimeter Array (ALMA) is promising to be a powerful tool for precision astrometry of the area around Sagittarius A (Sgr A) because it ha…

astro-ph.GA2021★ 5 cited

Hot Molecular Core Candidates in the Galactic Center 50 km/s Molecular Cloud

Ryosuke Miyawaki, Masato Tsuboi, Kenta Uehara +1

We present the results based on the 2.5 arcsec-resolution observations using Atacama Large Millimeter/submillimeter Array (ALMA) of the Galactic Center Molecular Cloud G-0.02-0.07,…

astro-ph.GA2020★ 3 cited

Cloud-Cloud Collision in the Galactic Center Arc

Masato Tsuboi, Yoshimi Kitamura, Kenta Uehara +4

We performed a search of cloud-cloud collision (CCC) sites in the Sagittarius A molecular cloud (SgrAMC) based on the survey observations using the Nobeyama 45-m telescope in the C…

astro-ph.GA2020★ 9 cited

Where is the Western Part of the Galactic Center Lobe Located really?

Masato Tsuboi, Takahiro Tsutsumi, Yoshimi Kitamura +3

The Galactic Center Lobe (GCL) is a peculiar object widely protruding from the Galactic plane toward the positive Galactic latitude, which had been found toward the Galactic Center…

astro-ph.HE2020★ 28 cited

Time Variations in the Flux Density of Sgr A* at 230 GHz Detected with ALMA

Yuhei Iwata, Tomoharu Oka, Masato Tsuboi +2

A radio source at the Galactic center Sgr A* is a prime supermassive black hole candidate and therefore key to developing our understanding of them. Time variations in the 230 GHz…