David V. Stark
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View article: Erratum: “The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs” (2016, ApJ, 832, 126)
Erratum: “The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs” (2016, ApJ, 832, 126) Open
Erratum to: “The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs”
View article: The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H i–Halo Mass Relation
The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H i–Halo Mass Relation Open
We present a four-step group-finding algorithm for the Gas in Galaxy Groups (G3) initiative, a spin-off of the z ∼ 0 REsolved Spectroscopy Of a Local VolumE (RESOLVE) and Environmental COntext (ECO) surveys. In preparation for future compa…
View article: Erratum: “The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H <scp>i</scp>–Halo Mass Relation” (2023, ApJ, 956, 51)
Erratum: “The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H <span>i</span>–Halo Mass Relation” (2023, ApJ, 956, 51) Open
View article: The RESOLVE and ECO G3 Initiative: Drivers of H <scp>i</scp> Content and X-Ray Emission in Galaxy Groups
The RESOLVE and ECO G3 Initiative: Drivers of H <span>i</span> Content and X-Ray Emission in Galaxy Groups Open
Adding to the RESOLVE and ECO Gas in Galaxy Groups (G3) initiative, we examine possible drivers of group-integrated H i -to-halo mass ratios ( M HI,grp / M halo ) and group X-ray emission, including group halo mass ( M halo ), virializatio…
View article: The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey
The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey Open
We study tidal features around galaxies in the REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey. Our sample consists of 1048 RESOLVE galaxies that overlap with the DECam Legacy Survey, which reaches an r-band 3σ depth of ∼27.9 mag …
View article: Erratum: “The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey” (2018, ApJ, 857, 144)
Erratum: “The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey” (2018, ApJ, 857, 144) Open
Erratum to “The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey”
View article: The Impacts of Bars, Spirals, and Bulge Size on Gas-phase Metallicity Gradients in MaNGA Galaxies
The Impacts of Bars, Spirals, and Bulge Size on Gas-phase Metallicity Gradients in MaNGA Galaxies Open
As galaxies evolve over time, the orbits of their constituent stars are expected to change in size and shape, moving stars away from their birth radius. Radial gas flows are also expected. Spiral arms and bars in galaxies are predicted to …
View article: The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies
The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies Open
As galaxies evolve over time, the orbits of their constituent stars are expected to change in size and shape, moving stars away from their birth radius. Radial gas flows are also expected. Spiral arms and bars in galaxies are predicted to …
View article: The Strength of Bisymmetric Modes in SDSS-IV/MaNGA Barred Galaxy Kinematics
The Strength of Bisymmetric Modes in SDSS-IV/MaNGA Barred Galaxy Kinematics Open
The Sloan Digital Sky Survey-IV/Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) Survey data provide an unprecedented opportunity to study the internal motions of galaxies and, in particular, represent the largest sample of barr…
View article: SatHub Panel: Satellite Interference in Observatories Around the World
SatHub Panel: Satellite Interference in Observatories Around the World Open
Satellite constellation interference occurs across astronomical disciplines. We present examples of interference from radio and $γ$-Ray astronomy to optical and spectroscopic interference in ground-based and space-borne facilities. In part…
View article: BreakBRD Galaxies: Evolutionary Clues through an Analysis of Gas Content
BreakBRD Galaxies: Evolutionary Clues through an Analysis of Gas Content Open
By combining newly obtained deep Green Bank Telescope 21 cm observations with optical spectroscopic data, we present an analysis of the gas content of break bulges in red disks (breakBRD) galaxies, a population denoted by their blue star-f…
View article: Finding Passive Galaxies in H i-MaNGA: The Impact of Star Formation Rate Indicator
Finding Passive Galaxies in H i-MaNGA: The Impact of Star Formation Rate Indicator Open
H i -rich galaxies typically have high star formation rates (SFRs), but there exist interesting H i -rich and low star-forming galaxies. Previous work on a sample of these galaxies identified from H i -Mapping Nearby Galaxies at Apache Poi…
View article: BreakBRD Galaxies: Evolutionary Clues Through an Analysis of Gas Content
BreakBRD Galaxies: Evolutionary Clues Through an Analysis of Gas Content Open
By combining newly obtained deep GBT 21cm observations with optical spectroscopic data, we present an analysis of the gas content of BreakBRD galaxies, a population denoted by their blue star-forming centers and red quenched disks that do …
View article: Identification and Quenching of Nugget Galaxies in the RESOLVE Survey at z = 0
Identification and Quenching of Nugget Galaxies in the RESOLVE Survey at z = 0 Open
We present a complete census of candidate nuggets, i.e., dense galaxies likely formed by compaction with intense gas influx, within the volume-limited redshift z ∼ 0 REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey. These nuggets s…
View article: The ALMaQUEST Survey XV: The Dependence of the Molecular-to-Atomic Gas Ratios on Resolved Optical Diagnostics
The ALMaQUEST Survey XV: The Dependence of the Molecular-to-Atomic Gas Ratios on Resolved Optical Diagnostics Open
The atomic-to-molecular gas conversion is a critical step in the baryon cycle of galaxies, which sets the initial conditions for subsequent star formation and influences the multi-phase interstellar medium. We compiled a sample of 94 nearb…
View article: The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys
The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys Open
Galaxy environment plays an important role in driving the transformation of galaxies from blue and star forming to red and quenched. Recent works have focused on the role of cosmic web filaments in galaxy evolution and have suggested that …
View article: The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys
The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys Open
Galaxy environment plays an important role in driving the transformation of galaxies from blue and star-forming to red and quenched. Recent works have focused on the role of cosmic web filaments in galaxy evolution and have suggested that …
View article: The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H <scp>i</scp>–Halo Mass Relation
The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H <span>i</span>–Halo Mass Relation Open
We present a four-step group-finding algorithm for the Gas in Galaxy Groups (G3) initiative, a spin-off of the z ∼ 0 REsolved Spectroscopy Of a Local VolumE (RESOLVE) and Environmental COntext (ECO) surveys. In preparation for future compa…
View article: HI Rich but Low Star Formation galaxies in MaNGA: Physical Properties and Comparison to Control Samples
HI Rich but Low Star Formation galaxies in MaNGA: Physical Properties and Comparison to Control Samples Open
Gas rich galaxies are typically star-forming. We make use of HI-MaNGA, a program of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey of the Sloan Digital Sky Surveys to construct a sample of unusual n…
View article: H <scp>i</scp>-rich but low star formation galaxies in MaNGA: physical properties and comparison to control samples
H <span>i</span>-rich but low star formation galaxies in MaNGA: physical properties and comparison to control samples Open
Gas-rich galaxies are typically star forming. We make use of H i-MaNGA, a programme of H i follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey of the Sloan Digital Sky Surveys, to construct a sample of unus…
View article: Erratum: “Testing Algorithms for Identifying Source Confusion in the HI-MaNGA Survey” (2022, RNAAS, 6, 1)
Erratum: “Testing Algorithms for Identifying Source Confusion in the HI-MaNGA Survey” (2022, RNAAS, 6, 1) Open
The first three authors regret an oversight which led to improper acknowledgment of the use of Apertif data in the initial publication and the omission of a co-author. In this Erratum we add the specific named co-author, as well as “the Ap…
View article: Post-starburst properties of post-merger galaxies
Post-starburst properties of post-merger galaxies Open
Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching, we investigate the incidence of PSBs and resolved PSB prope…
View article: Post-Starburst Properties of Post-Merger Galaxies
Post-Starburst Properties of Post-Merger Galaxies Open
Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching, we investigate the incidence of PSBs and resolved PSB prope…
View article: A comparison of the baryonic Tully–Fisher relation in MaNGA and IllustrisTNG
A comparison of the baryonic Tully–Fisher relation in MaNGA and IllustrisTNG Open
We compare an observed baryonic Tully–Fisher relation (BTFR) from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) and HI-MaNGA surveys to a simulated BTFR from the cosmological magnetohydrodynamical simulation, IllustrisTNG…
View article: A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants
A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants Open
We investigate the role of galaxy mergers in triggering active galactic nuclei (AGN) in the nearby universe. Our analysis is based on a sample of 79 post-merger remnant galaxies with deep X-ray observations from Chandra/XMM-Newton capable …
View article: The H <scp>i</scp> content of red geyser galaxies
The H <span>i</span> content of red geyser galaxies Open
Red geysers are a specific type of quiescent galaxy, denoted by twin jets emerging from their galactic centres. These bisymmetric jets possibly inject energy and heat into the surrounding material, effectively suppressing star formation by…
View article: The HI Content of Red Geyser Galaxies
The HI Content of Red Geyser Galaxies Open
Red geysers are a specific type of quiescent galaxy, denoted by twin jets emerging from their galactic centers. These bisymmetric jets possibly inject energy and heat into the surrounding material, effectively suppressing star formation by…
View article: Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past Open
Post-starburst (PSB) galaxies have recently and rapidly quenched their star formation; thus, they are an important way to understand how galaxies transition from star-forming late types to quiescent early types. The recent discovery of lar…
View article: Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past Open
Post-starburst galaxies (PSBs) have recently and rapidly quenched their star-formation, thus they are an important way to understand how galaxies transition from star-forming late-types to quiescent early-types. The recent discovery of lar…
View article: MaNGA 8313-1901: Gas Accretion Observed in a Blue Compact Dwarf Galaxy?
MaNGA 8313-1901: Gas Accretion Observed in a Blue Compact Dwarf Galaxy? Open
Gas accretion is an important process in the evolution of galaxies, but it has limited direct observational evidences. In this paper, we report the detection of a possible ongoing gas accretion event in a blue compact dwarf (BCD) galaxy, M…