activity
19982026
most citedThe Arecibo Legacy Fast ALFA Survey: I. Science Goals, Survey Design and Strategy

830 citations · 10k across the 131 of their papers we have counts for

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67 papers · 1 filter

astro-ph.GA2026

Too Big to Quench? I. Constraining ISM Stripping of Dwarf Satellites in Milky Way-like Halos

Jingyao Zhu, Stephanie Tonnesen, Greg L. Bryan +1

Galaxy environment plays a crucial role in quenching star formation in dwarf galaxies. In Milky Way (MW)-like environments, dwarf satellite quenching is primarily driven by ram pre…

astro-ph.GA2025

Baryonic Masses and Properties of Gaseous Satellite Galaxies

Jingyao Zhu, Yasmeen Asali, Mary Putman +12

We present a sample of 127 gas-bearing dwarf galaxies around 56 late-type host galaxies within 30 Mpc using 21-cm HI data from the WALLABY, MHONGOOSE, and ALFALFA surveys. We chara…

astro-ph.GA2025

WALLABY Pilot Survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster

L. Staveley-Smith, K. Bekki, A. Boselli +16

As part of the pilot survey of the Widefield ASKAP L-band Legacy All-sky Survey (WALLABY), high-resolution neutral atomic hydrogen (HI) observations of the dwarf galaxy pair NGC 45…

astro-ph.GA2024★ 17 cited

It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip

Jingyao Zhu, Stephanie Tonnesen, Greg L. Bryan +1

The circumgalactic medium (CGM) of star-forming dwarf galaxies plays a key role in regulating the galactic baryonic cycle. We investigate how susceptible the CGM of dwarf satellite…

astro-ph.GA2024

The Plane Quasar Survey: First Data Release

Jessica Werk, Kirill Tchernyshyov, Hannah Bish +4

We present a sample of 305 QSO candidates having , the majority with GALEX magnitudes NUV < 18.75. To generate this sample, we apply UV-IR color selection criteri…

astro-ph.GA2024

Identifying HI Emission and UV Absorber Associations Near the Magellanic Stream

Doyeon A. Kim, Yong Zheng, Mary E. Putman

We present a new technique to identify associations of HI emission in the Magellanic Stream (MS) and ultraviolet (UV) absorbers from 92 QSO sight lines near the MS. We quantify the…

astro-ph.GA2024★ 7 cited

Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES

Yong Zheng, Kirill Tchernyshyov, Knut Olsen +11

The Large Magellanic Cloud (LMC) is home to many HII regions, which may lead to significant outflows. We examine the LMC's multiphase gas ( K) in HI, SII, SiIV, and…

astro-ph.GA2023★ 5 cited

Properties of 3D HI Filaments in the Smith High Velocity Cloud

Colin Holm-Hansen, M. E. Putman, D. A. Kim

We present findings of 3D filamentary structures in the Smith Cloud, a high-velocity cloud (HVC) located at , . We use data from the Galactic Arecibo L…

astro-ph.GA2023★ 9 cited

The Kinematic Structure of Magnetically Aligned HI Filaments

Doyeon Avery Kim, Susan E Clark, Mary E Putman +1

We characterize the kinematic and magnetic properties of HI filaments located in a high Galactic latitude region ( and ). We extra…

astro-ph.GA2023★ 10 cited

Census of Gaseous Satellites around Local Spiral Galaxies

Jingyao Zhu, Mary E Putman

We present a search for gas-containing dwarf galaxies as satellite systems around nearby spiral galaxies using 21 cm neutral hydrogen (HI) data from the Arecibo Legacy Fast ALFA (A…

astro-ph.GA2023★ 9 cited

HI filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-HI filaments

Y. K. Ma, N. M. McClure-Griffiths, S. E. Clark +12

High-spatial-resolution HI observations have led to the realisation that the nearby (within few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the amb…

astro-ph.GA2023

A Comprehensive Investigation of Metals in the Circumgalactic Medium of Nearby Dwarf Galaxies

Yong Zheng, Yakov Faerman, Benjamin D. Oppenheimer +7

Dwarf galaxies are found to have lost most of their metals via feedback processes; however, there still lacks consistent assessment on the retention rate of metals in their circumg…

astro-ph.GA2021★ 7 cited

Investigating the Baryon Cycle in Interacting Dwarfs with the Very Large Array and Pan-STARRS

Nicholas Luber, Sarah Pearson, Mary Putman +3

We present resolved HI synthesis maps from the Very Large Array (VLA) of three interacting dwarf systems: the NGC 3664 dwarf pair, the NGC 3264 dwarf pair, and the UGC 4638 dwarf t…

astro-ph.GA2021★ 30 cited

The Cosmic Ultraviolet Baryon Survey (CUBS) IV: The Complex Multiphase Circumgalactic Medium as Revealed by Partial Lyman Limit Systems

Thomas J. Cooper, Gwen C. Rudie, Hsiao-Wen Chen +18

We present a detailed study of two partial Lyman limit systems (pLLSs) of neutral hydrogen column density discovered at…

astro-ph.GA2021★ 51 cited

The Cosmic Ultraviolet Baryon Survey (CUBS) -- III. Physical properties and elemental abundances of Lyman limit systems at

Fakhri S. Zahedy, Hsiao-Wen Chen, Thomas M. Cooper +18

(Abridged) We present a systematic investigation of physical conditions and elemental abundances in four optically thick Lyman-limit systems (LLSs) at discovered withi…

astro-ph.GA2021★ 140 cited

The Gas Content and Stripping of Local Group Dwarf Galaxies

Mary E. Putman, Yong Zheng, Adrian M. Price-Whelan +4

The gas content of the complete compilation of Local Group dwarf galaxies (119 within 2 Mpc) is presented using HI survey data. Within the virial radius of the Milky Way (224 kpc h…

astro-ph.GA2020★ 19 cited

Discovery of Magellanic Stellar Debris in the H3 Survey

Dennis Zaritsky, Charlie Conroy, Rohan P. Naidu +9

We report the discovery of 15 stars in the H3 survey that lie, in projection, near the tip of the trailing gaseous Magellanic Stream (MS). The stars have Galactocentric velocities…

astro-ph.GA2020★ 17 cited

Characterizing the Circumgalactic Medium of the Lowest-Mass Galaxies: A Case Study of IC 1613

Yong Zheng, Andrew Emerick, Mary E. Putman +3

Using 10 sightlines observed with the Hubble Space Telescope/Cosmic Origins Spectrograph, we study the circumgalactic medium (CGM) and outflows of IC1613, which is a low-mass ($M_*…

astro-ph.GA2020★ 17 cited

The Cosmic Ultraviolet Baryon Survey (CUBS) II: Discovery of an H-Bearing DLA in the Vicinity of an Early-Type Galaxy at z = 0.576

Erin Boettcher, Hsiao-Wen Chen, Fakhri S. Zahedy +18

We report the serendipitous detection of an H-bearing damped Lyman- absorber at z = 0.576 in the spectrum of the QSO J0111-0316 in the Cosmic Ultraviolet Baryon Survey. Sp…

astro-ph.GA2020★ 18 cited

The QuaStar Survey: Detecting Hidden Low-Velocity Gas in the Milky Way's Circumgalactic Medium

Hannah V. Bish, Jessica K. Werk, Joshua Peek +2

From our position embedded within the Milky Way's interstellar medium (ISM), we have limited ability to detect gas at low relative velocities in the extended Galactic halo because…

astro-ph.GA2020★ 6 cited

The HI Structure of the Local Volume Dwarf Galaxy Pisces A

Luca Beale, Jennifer Donovan Meyer, Erik J. Tollerud +2

Dedicated HI surveys have recently led to a growing category of low-mass galaxies found in the Local Volume. We present synthesis imaging of one such galaxy, Pisces A, a low-mass d…

astro-ph.GA2020★ 74 cited

The Cosmic Ultraviolet Baryon Survey (CUBS) I. Overview and the diverse environments of Lyman limit systems at z<1

Hsiao-Wen Chen, Fakhri S. Zahedy, Erin Boettcher +19

We present initial results from the Cosmic Ultraviolet Baryon Survey (CUBS). CUBS is designed to map diffuse baryonic structures at redshift z<~1 using absorption-line spectroscopy…

astro-ph.GA2020★ 230 cited

WALLABY -- An SKA Pathfinder HI Survey

B. S. Koribalski, L. Staveley-Smith, T. Westmeier +67

The Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) is a next-generation survey of neutral hydrogen (HI) in the Local Universe. It uses the widefield, high-resolution…

astro-ph.GA2019★ 14 cited

Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM

Y. Zheng, M. E. Putman, A. Emerick +7

We report a tentative detection of the circumgalactic medium (CGM) of WLM, an isolated, low-mass (log), dwarf irregular galaxy in the Local Group (LG). We an…