activity
20192026
most citedCO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project

61 citations · 97 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

An Energetic Consistency Test for Feedback-Driven Gas Loss in Milky Way Dwarf Satellites

Sena A. Matsui, Tsutomu T. Takeuchi, Suchetha Cooray +1

Dwarf spheroidal galaxies (dSphs) contain little detectable cold gas, but the relative roles of stellar feedback, reionization, and environmental effects in their gas loss remain u…

astro-ph.GA2026

Interplay of Compaction, Quenching, and Black Hole Growth in the Most Massive Galaxies since : Insights from JWST and Chandra Data

Novan Saputra Haryana, Masayuki Akiyama, Abdurro'uf +16

The buildup of dense stellar cores is expected to mark an important transition in the star-formation and black-hole growth of massive galaxies. Using spatially resolved spectral en…

astro-ph.IM2026

A Path to an All-Sky Survey with Roman

Jiwon Jesse Han, Anirudh Chiti, Kai-Feng Chen +93

A deep, space-based, all-sky near-infrared survey carried out with the Nancy Grace Roman Space Telescope would constitute a foundational astronomical infrastructure for decades to…

cs.CL2025★ 1 cited

ReplicationBench: Can AI Agents Replicate Astrophysics Research Papers?

Christine Ye, Sihan Yuan, Suchetha Cooray +10

Frontier AI agents show increasing promise as scientific research assistants, and may eventually be useful for extended, open-ended research workflows. However, in order to use age…

astro-ph.GA2025

How does feedback affect the star formation histories of galaxies?

Kartheik G. Iyer, Tjitske K. Starkenburg, Greg L. Bryan +20

Star formation in galaxies is regulated by the interplay of a range of processes that shape the multiphase gas in the interstellar and circumgalactic media. Using the CAMELS suite…

astro-ph.GA2025★ 1 cited

Insights into the dependence of galaxy properties on the environment with explainable machine learning models

Shun-ya S. Uchida, Suchetha Cooray, Atsushi J. Nishizawa +2

Galaxies reside within dark matter halos, but their properties are influenced not only by their halo properties but also by the surrounding environment. We construct an interpretab…

astro-ph.CO2024★ 1 cited

sOPTICS: A Modified Density-Based Algorithm for Identifying Galaxy Groups/Clusters and Brightest Cluster Galaxies

Hai-Xia Ma, Tsutomu T. Takeuchi, Suchetha Cooray +1

A direct approach to studying the galaxy-halo connection is to analyze groups and clusters of galaxies that trace the underlying dark matter halos, emphasizing the importance of id…

astro-ph.GA2024

Katachi: Decoding the Imprints of Past Star Formation on Present Day Morphology in Galaxies with Interpretable CNNs

Juan Pablo Alfonzo, Kartheik G. Iyer, Masayuki Akiyama +8

The physical processes responsible for shaping how galaxies form and quench over time leave imprints on both the spatial (galaxy morphology) and temporal (star formation history; S…

astro-ph.GA2023★ 1 cited

Extracting an Informative Latent Representation of High-Dimensional Galaxy Spectra

Daiki Iwasaki, Suchetha Cooray, Tsutomu T. Takeuchi

To understand the fundamental parameters of galaxy evolution, we investigated the minimum set of parameters that explain the observed galaxy spectra in the local Universe. We ident…

astro-ph.GA2022★ 4 cited

Galaxy Manifold: Characterizing and understanding galaxies with two parameters

Suchetha Cooray, Tsutomu T. Takeuchi, Daichi Kashino +3

We report the discovery of a two-dimensional Galaxy Manifold within the multi-dimensional luminosity space of local galaxies. The multi-dimensional luminosity space is constructed…

astro-ph.GA2022

Estimating Galaxy Star Formation Rates from Murchison Widefield Array Radio Continuum Emission

Tsutomu T. Takeuchi, Suchetha Cooray, Luca Cortese +3

We investigate the frequency dependence of the low-frequency infrared (IR)--radio correlation for nearby galaxies drawn from the {\sl Herschel} Reference Survey (HRS), using radio…

astro-ph.IM2022★ 1 cited

High Dimensional Statistical Analysis and its Application to ALMA Map of NGC 253

Tsutomu T. Takeuchi, Kazuyoshi Yata, Kento Egashira +6

In astronomy, if we denote the dimension of data as and the number of samples as , we often meet a case with . Traditionally, such a situation is regarded as ill-po…

astro-ph.IM2021★ 3 cited

Wavelets and sparsity for Faraday tomography

Suchetha Cooray, Tsutomu T. Takeuchi, Shinsuke Ideguchi +3

Faraday tomography through broadband polarimetry can provide crucial information on magnetized astronomical objects, such as quasars, galaxies, or galaxy clusters. However, the lim…

astro-ph.IM2020★ 10 cited

An Iterative Reconstruction Algorithm for Faraday Tomography

Suchetha Cooray, Tsutomu T. Takeuchi, Takuya Akahori +4

Faraday tomography offers crucial information on the magnetized astronomical objects, such as quasars, galaxies, or galaxy clusters, by observing its magnetoionic media. The observ…

astro-ph.CO2020★ 10 cited

A Study on the Baryon Acoustic Oscillation with Topological Data Analysis

Kai T. Kono, Tsutomu T. Takeuchi, Suchetha Cooray +2

(abridged) The scale of the acoustic oscillation of baryons at the baryon-photon decoupling is imprinted on the spatial distribution of galaxies in the Universe, known as the baryo…

astro-ph.IM2020★ 4 cited

A Method for Unmasking Incomplete Astronomical Signals: Application to CO Multi-line Imaging of Nearby Galaxies Project

Suchetha Cooray, Tsutomu T. Takeuchi, Moe Yoda +1

Photometric surveys have provided incredible amounts of astronomical information in the form of images. However, astronomical images often contain artifacts that can critically hin…

astro-ph.GA2019★ 61 cited

CO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project

Kazuo Sorai, Nario Kuno, Kazuyuki Muraoka +36

Observations of the molecular gas in galaxies are vital to understanding the evolution and star-forming histories of galaxies. However, galaxies with molecular gas maps of their wh…