activity
20142026
most citedClumps as multiscale structures in cosmic noon galaxies

15 citations · 19 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

An AGN in the Antennae galaxies ?

Shinya Komugi, Toshiki Saito, Tomonari Michiyama +5

Time variability is a strong probe of energetic phenomena which occur at small spatial scales, like Active Galactic Nuclei (AGN). We use ALMA observations at 100 GHz executed over…

astro-ph.GA2026

Cloud-Cloud Collisions Induce Filament-Mediated Super Star Cluster Formation in the Antennae Overlap Region: Evidence from ALMA and JWST

Tomonari Michiyama, Toshiki Saito, Kouichiro Nakanishi +5

The formation of super star clusters (SSCs) in galaxies remains a fundamental yet unresolved problem. Among the proposed mechanisms, cloud-cloud collisions (CCCs) have been suggest…

astro-ph.GA2025★ 3 cited

Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies

Ryota Ikeda, Daisuke Iono, Ken-ichi Tadaki +19

We present an analysis of rest-frame optical and far-infrared continuum emission in three luminous submillimeter galaxies (SMGs) at . The SMGs are spatial…

astro-ph.GA2025★ 1 cited

Low dust mass and high star-formation efficiency at from deep ALMA observations

Ikki Mitsuhashi, Jorge A. Zavala, Tom J. L. C. Bakx +15

We investigate the dust mass build-up and star formation efficiency of two galaxies at , GHZ2 and GS-z14-0, by combining ALMA and JWST observations with an analytical model t…

astro-ph.GA2025★ 15 cited

Clumps as multiscale structures in cosmic noon galaxies

Boris S Kalita, Tomoko L Suzuki, Daichi Kashino +31

Star-forming clumps have been found to significantly influence the star formation of gas-rich galaxies. Using public data from JWST/NIRCam (COSMOS-Web) and ALMA (FMOS-COSMOS)…

astro-ph.GA2014

Molecular Gas and Star Formation in Voids

M. Das, T. Saito, D. Iono +2

We present the detection of molecular gas using CO(1-0) line emission and follow up Halpha imaging observations of galaxies located in nearby voids. The CO(1-0) observations were d…