activity
20072026
most citedCO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project

61 citations · 717 across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2026

High-Resolution [CI] and CO Observations of Circumnuclear Disks in Nearby Seyfert Galaxies

Dragan Salak, Suphakorn Suphapolthaworn, Yusuke Miyamoto +3

We present [CI] , CO , and 800-GHz continuum observations of the circumnuclear disks (CNDs) in the Seyfert galaxies…

astro-ph.HE2026

Compact dusty starbursts at cosmic noon linked to high-energy neutrinos

Yuji Urata, Kuiyun Huang, Bunyo Hatsukade +7

The origin of high-energy astrophysical neutrinos remains unresolved, and secure electromagnetic counterparts to individual events are rare despite rapid follow-up. Dusty star-form…

astro-ph.GA2025

CO Multi-line Imaging of Nearby Galaxies (COMING). XI. Azimuthally averaged star formation rate and stellar mass relation with molecular gas amount

Ayumi Kajikawa, Kazuo Sorai, Kana Morokuma-Matsui +13

This study investigated the relation between the surface density of star formation rate (SFR) (), stellar mass (), and molecular gas mass ($Σ_{M_\ma…

astro-ph.GA2025★ 1 cited

Water Maser Disk and a Supermassive Black Hole at the Nucleus of the Active Galaxy NGC 7738

Rinka Ito, Yusuke Miyamoto, Naomasa Nakai +2

We present the results of very long baseline interferometry (VLBI) observations of water vapor masers in the nucleus of the LINER galaxy NGC 7738. The red- and blue-shifted and new…

astro-ph.GA2025★ 4 cited

Infrared bubble recognition in the Milky Way and beyond using deep learning

Shimpei Nishimoto, Toshikazu Onishi, Atsushi Nishimura +9

We propose a deep learning model that can detect Spitzer bubbles accurately using two-wavelength near-infrared data acquired by the Spitzer Space Telescope and JWST. The model is b…

astro-ph.GA2023

Predicting reliable H column density maps from molecular line data using machine learning

Yoshito Shimajiri, Yasutomo Kawanishi, Shinji Fujita +13

The total mass estimate of molecular clouds suffers from the uncertainty in the H-CO conversion factor, the so-called factor, which is used to convert the C…