activity
20182021
most citedBlack Hole Mass Measurements of Radio Galaxies NGC 315 and NGC 4261 Using ALMA CO Observations

65 citations · 103 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.GA20241 cited

Modeling ALMA Observations of the Warped Molecular Gas Disk in the Red Nugget Relic Galaxy NGC 384

Jonathan H. Cohn, Maeve Curliss, Jonelle L. Walsh +9

We present 0-resolution CO(21) observations of the circumnuclear gas disk in the local compact galaxy NGC 384 with the Atacama Large Millimeter/submill…

astro-ph.GA2021

An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698

Jonathan H. Cohn, Jonelle L. Walsh, Benjamin D. Boizelle +9

We present 0\farcs{14}-resolution Atacama Large Millimeter/submillimeter Array (ALMA) CO(21) observations of the circumnuclear gas disk in UGC 2698, a local compact galaxy. The…

astro-ph.GA202065 cited

Black Hole Mass Measurements of Radio Galaxies NGC 315 and NGC 4261 Using ALMA CO Observations

Benjamin D. Boizelle, Jonelle L. Walsh, Aaron J. Barth +6

We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 5 and Cycle 6 observations of CO(21) and CO(32) emission at 0.2''0.3'' resolution in two radio-bright,…

astro-ph.GA202014 cited

A giant galaxy in the young Universe with a massive ring

Tiantian Yuan, Ahmed Elagali, Ivo Labbe +12

In the local (redshift z~0) Universe, collisional ring galaxies make up only ~0.01% of galaxies and are formed by head-on galactic collisions that trigger radially propagating dens…

astro-ph.GA202024 cited

MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3<z<4) from the ZFOURGE Survey

Kim-Vy H. Tran, Ben Forrest, Leo Y. Alcorn +13

To understand how strong emission line galaxies (ELGs) contribute to the overall growth of galaxies and star formation history of the universe, we target Strong ELGs (SELGs) from t…

astro-ph.GA2020

MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation

Anshu Gupta, Kim-Vy Tran, Jonathan Cohn +13

We use K-band spectroscopic data from the Multi-Object Spectroscopic Emission Line (MOSEL) survey to analyze the kinematic properties of galaxies at z>3. Our sample consists of 34…