activity
20162025
most citedThe Enigmatic (Almost) Dark Galaxy Coma P: Distance Measurement and Stellar Populations from HST Imaging

24 citations · 128 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025

Resolved ALMA [CII] 158 micron Observations at Cosmic Noon: ISM Structure and Dynamics of Starbursting QSO SDSSJ1000

Christopher Rooney, Bo Peng, Amit Vishwas +7

We present spatially resolved Alma Band-9 observations of the [CII] 158 m fine structure line from an optically selected quasar, SDSS J100038.01+020822.4 (J1000), at z=1.8275. B…

astro-ph.GA2022★ 8 cited

A Generalist, Automated ALFALFA Baryonic Tully-Fisher Relation

Catie J. Ball, Martha P. Haynes, Michael G. Jones +5

The Baryonic Tully-Fisher Relation (BTFR) has applications in galaxy evolution as a testbed for the galaxy-halo connection and in observational cosmology as a redshift-independent…

astro-ph.GA2022★ 5 cited

Parametrized Asymmetric Neutral hydrogen Disk Integrated Spectrum Characterization (PANDISC) I: Introduction to A Physically Motivated H I Model

Bo Peng, Martha P. Haynes, Catie J. Ball +1

Modelling the integrated H I spectra of galaxies has been a difficult task due to their diverse shapes, but more dynamical information is waiting to be explored in Hi line profiles…

astro-ph.GA2022★ 18 cited

Discovery of a Dusty, Chemically Mature Companion to a z4 Starburst Galaxy in JWST ERS Data

Bo Peng, Amit Vishwas, Gordon Stacey +6

We report the discovery of two companion sources to a strongly lensed galaxy SPT0418-47 ("ring") at redshift 4.225, targeted by the JWST Early Release Science program. We confirm t…

astro-ph.GA2021★ 21 cited

The ALFALFA Almost-Dark Galaxy AGC~229101: A Two Billion Solar Mass HI Cloud with a Very Low Surface Brightness Optical Counterpart

Lukas Leisman, Katherine L. Rhode, Catherine Ball +11

We present results from deep HI and optical imaging of AGC 229101, an unusual HI source detected at v = 7116 km/s in the ALFALFA survey. Initially classified as a can…

astro-ph.GA2020★ 20 cited

Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies

Bo Peng, Cody Lamarche, Gordon Stacey +8

The Nitrogen-to-Oxygen (N/O) abundance ratio is an important diagnostic of galaxy evolution since the ratio is closely tied to the growth of metallicity and the star formation hist…