most citedMulti-molecule ALMA observations towards the Seyfert 1 galaxy NGC 1097

86 citations · 240 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA20245 cited

Measuring 60-pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA

Yuzuki Nagashima, Toshiki Saito, Soh Ikarashi +7

Star formation rate (SFR) is a fundamental parameter for describing galaxies and inferring their evolutionary course. HII regions yield the best measure of instantaneous SFR in gal…

astro-ph.IM2024

A 10.24-GHz-wide digital spectrometer array system for LMT-FINER: system design and laboratory performance verification

Masato Hagimoto, Akio Taniguchi, Yoichi Tamura +10

For efficient spectroscopic redshift identification of early galaxies in the northern hemisphere, we aim to combine the Large Millimeter Telescope (LMT) with a wide-band heterodyne…

astro-ph.IM2024

FINER: Far-Infrared Nebular Emission Receiver for the Large Millimeter Telescope

Yoichi Tamura, Takeshi Sakai, Ryohei Kawabe +34

Unveiling the emergence and prevalence of massive/bright galaxies during the epoch of reionization and beyond, within the first 600 million years of the Universe, stands as a pivot…

astro-ph.GA202220 cited

AGN-driven Cold Gas Outflow of NGC 1068 Characterized by Dissociation-Sensitive Molecules

Toshiki Saito, Shuro Takano, Nanase Harada +11

Recent developments in (sub-)millimeter facilities have drastically changed the amount of information obtained from extragalactic spectral scans. In this paper, we present a featur…

astro-ph.GA201486 cited

Multi-molecule ALMA observations towards the Seyfert 1 galaxy NGC 1097

S. Martin, K. Kohno, T. Izumi +17

The nearby Sy 1 galaxy NGC 1097 represents an ideal laboratory to explore the molecular chemistry in the presence and surroundings of an active galactic nucleus. Exploring the dist…

astro-ph.SR201479 cited

Cluster Formation Triggered by Filament Collisions in Serpens South

Fumitaka Nakamura, Koji Sugitani, Tomohiro Tanaka +24

The Serpens South infrared dark cloud consists of several filamentary ridges, some of which fragment into dense clumps. On the basis of CCS (), HCN (), N$_2…