T. Westmeier
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View article: WALLABY Pilot Survey: Characterizing Low-rotation Kinematically Modeled Galaxies
WALLABY Pilot Survey: Characterizing Low-rotation Kinematically Modeled Galaxies Open
Many of the tensions in cosmological models of the Universe lie in the low-mass, low-velocity regime. Probing this regime requires a statistically significant sample of galaxies with well-measured kinematics and robustly measured uncertain…
View article: WALLABY: an untargeted search for H <scp>i</scp> -bearing ultra-diffuse galaxies uncovers the first known ultra-diffuse galaxy pair
WALLABY: an untargeted search for H <span>i</span> -bearing ultra-diffuse galaxies uncovers the first known ultra-diffuse galaxy pair Open
Using the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY), we performed an untargeted search for H i-bearing ultra-diffuse galaxies (UDGs). We identified a core sample of 10 UDGs defined by $\mu _{0,g}\ge 24$ mag arcsec$^{-2}$…
View article: WALLABY Pilot Survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster
WALLABY Pilot Survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster Open
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 4532/DDO 137 (WALLABY J123424+062511) have revealed a huge (4…
View article: WALLABY pilot survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster
WALLABY pilot survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster Open
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 4532/DDO 137 (WALLABY J123424+062511) have revealed a huge (4…
View article: WALLABY pilot survey: properties of HI-selected dark sources and low surface brightness galaxies
WALLABY pilot survey: properties of HI-selected dark sources and low surface brightness galaxies Open
We examine the optical counterparts of the 1829 neutral hydrogen (HI) detections in three pilot fields in the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) using data from the Dark Energy Spectroscopic Instrument (DESI) Lega…
View article: Looking at the Distant Universe with the MeerKAT Array: The H <scp>i</scp> Mass Function in the Local Universe
Looking at the Distant Universe with the MeerKAT Array: The H <span>i</span> Mass Function in the Local Universe Open
We present measurements of the neutral atomic hydrogen (H i ) mass function (H i MF) and cosmic H i density (Ω H I ) at 0 ≤ z ≤ 0.088 from the Looking at the Distant Universe with MeerKAT Array (LADUMA) survey. Using LADUMA Data Release 1 …
View article: WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation
WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation Open
An avenue for understanding cosmological galaxy formation is to compare morphometric parameters in observations and simulations of galaxy assembly. In this second paper of the ASymba: Asymmetries of H i in SIMBA Galaxies series, we measure…
View article: WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs
WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs Open
Galaxy interactions can significantly affect the star formation in galaxies, but it remains a challenge to achieve a consensus on the star formation rate (SFR) enhancement in galaxy pairs. Here, we investigate the SFR enhancement of gas-ri…
View article: WALLABY Pilot Survey: kNN identification of perturbed galaxies through HI morphometrics
WALLABY Pilot Survey: kNN identification of perturbed galaxies through HI morphometrics Open
Galaxy morphology in stellar light can be described by a series of "non-parametric" or "morphometric" parameters, such as concentration-asymmetry-smoothness, Gini, $M_{20}$, and Sersic fit. These parameters can be applied to column density…
View article: The CRAFT coherent (CRACO) upgrade I: System description and results of the 110-ms radio transient pilot survey
The CRAFT coherent (CRACO) upgrade I: System description and results of the 110-ms radio transient pilot survey Open
We present the first results from a new backend on the Australian Square Kilometre Array Pathfinder, the Commensal Realtime ASKAP Fast Transient COherent (CRACO) upgrade. CRACO records millisecond time resolution visibility data, and searc…
View article: WALLABY Pilot Survey: kNN identification of perturbed galaxies through H <scp>1</scp> morphometrics
WALLABY Pilot Survey: kNN identification of perturbed galaxies through H <span>1</span> morphometrics Open
Galaxy morphology in stellar light can be described by a series of ‘non-parametric’ or ‘morphometric’ parameters, such as concentration-asymmetry-smoothness, Gini, $M_{20}$ , and Sérsic fit. These parameters can be applied to column densit…
View article: WALLABY Pilot Survey: HI source-finding with a machine learning framework
WALLABY Pilot Survey: HI source-finding with a machine learning framework Open
The data volumes generated by theWidefield ASKAP L-band Legacy All-sky Blind surveY atomic hydrogen ( Hi ) survey using the Australian Square Kilometre Array Pathfinder (ASKAP) necessitate greater automation and reliable automation in the …
View article: WALLABY pilot survey: Properties of H <scp>i</scp>-selected dark sources and low surface brightness galaxies
WALLABY pilot survey: Properties of H <span>i</span>-selected dark sources and low surface brightness galaxies Open
We examine the optical counterparts of the 1 829 neutral hydrogen (H i ) detections in three pilot fields in the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) using data from the Dark Energy Spectroscopic Instrument (DESI) L…
View article: WALLABY pilot survey: Spatially resolved gas scaling relations within the stellar discs of nearby galaxies
WALLABY pilot survey: Spatially resolved gas scaling relations within the stellar discs of nearby galaxies Open
The scatter in global atomic hydrogen (H i ) scaling relations is partly attributed to differences in how H i and stellar properties are measured, with H i reservoirs typically extending beyond the inner regions of galaxies where star form…
View article: The first large absorption survey in H <scp>i</scp> (FLASH): II. Pilot survey data release and first results
The first large absorption survey in H <span>i</span> (FLASH): II. Pilot survey data release and first results Open
The First Large Absorption Survey in H i (FLASH) is a large-area radio survey for neutral hydrogen in and around galaxies in the intermediate redshift range $0.4\lt z\lt1.0$ , using the 21-cm H i absorption line as a probe of cold neutral …
View article: Looking At the Distant Universe with the MeerKAT Array: the HI Mass Function in the Local Universe
Looking At the Distant Universe with the MeerKAT Array: the HI Mass Function in the Local Universe Open
We present measurements of the neutral atomic hydrogen (HI) mass function (HIMF) and cosmic HI density ($Ω_{\rm HI}$) at $0 \leq z \leq 0.088$ from the Looking at the Distant Universe with MeerKAT Array (LADUMA) survey. Using LADUMA Data R…
View article: WALLABY Pilot Survey: Gas-rich Galaxy Scaling Relations from Marginally Resolved Kinematic Models
WALLABY Pilot Survey: Gas-rich Galaxy Scaling Relations from Marginally Resolved Kinematic Models Open
We present the first set of galaxy scaling relations derived from kinematic models of the Widefield Australian Square Kilometer Array Pathfinder (ASKAP) L -band Legacy All-sky Blind surveY (WALLABY) pilot phase observations. Combining the …
View article: WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs
WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs Open
Galaxy interactions can significantly affect the star formation in galaxies, but it remains a challenge to achieve a consensus on the star formation rate (SFR) enhancement in galaxy pairs. Here, we investigate the SFR enhancement of gas-ri…
View article: WALLABY Pilot Survey: HI source-finding with a machine learning framework
WALLABY Pilot Survey: HI source-finding with a machine learning framework Open
The data volumes generated by the WALLABY atomic Hydrogen (HI) survey using the Australiian Square Kilometre Array Pathfinder (ASKAP) necessitate greater automation and reliable automation in the task of source-finding and cataloguing. To …
View article: The First Large Absorption Survey in HI (FLASH): II. Pilot Survey data release and first results
The First Large Absorption Survey in HI (FLASH): II. Pilot Survey data release and first results Open
The First Large Absorption Survey in HI (FLASH) is a large-area radio survey for neutral hydrogen in the redshift range 0.41$, and appear to be a mixture of intervening and associated systems. Interestingly, around two-thirds of the lines …
View article: MHONGOOSE: A MeerKAT nearby galaxy H I survey
MHONGOOSE: A MeerKAT nearby galaxy H I survey Open
The MHONGOOSE (MeerKAT H I Observations of Nearby Galactic Objects: Observing Southern Emitters) survey maps the distribution and kinematics of the neutral atomic hydrogen (H I ) gas in and around 30 nearby star-forming spiral and dwarf ga…
View article: WALLABY pilot survey: an ‘almost’ dark cloud near the Hydra cluster
WALLABY pilot survey: an ‘almost’ dark cloud near the Hydra cluster Open
We explore the properties of an ‘almost’ dark cloud of neutral hydrogen (H i) using data from the Widefield ASKAP L-band Legacy All-sky Survey (WALLABY). Until recently, WALLABY J103508 − 283427 (also known as H1032 − 2819 or LEDA 2793457)…
View article: WALLABY Pilot Survey: An 'Almost' Dark Cloud near the Hydra Cluster
WALLABY Pilot Survey: An 'Almost' Dark Cloud near the Hydra Cluster Open
We explore the properties of an 'almost' dark cloud of neutral hydrogen (HI) using data from the Widefield ASKAP L-band Legacy All-sky Survey (WALLABY). Until recently, WALLABY J103508-283427 (also known as H1032-2819 or LEDA 2793457) was …
View article: WALLABY Pilot Survey: Public data release of ∼ 1800 H <scp>i</scp> sources and high-resolution cut-outs from Pilot Survey Phase 2
WALLABY Pilot Survey: Public data release of ∼ 1800 H <span>i</span> sources and high-resolution cut-outs from Pilot Survey Phase 2 Open
We present the Pilot Survey Phase 2 data release for the Wide-field ASKAP L-band Legacy All-sky Blind surveY (WALLABY), carried-out using the Australian SKA Pathfinder (ASKAP). We present 1760 H i detections (with a default spatial resolut…
View article: The Detection of an Extremely Bright Fast Radio Burst in a Phased Array Feed Survey
The Detection of an Extremely Bright Fast Radio Burst in a Phased Array Feed Survey Open
We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly's-eye configuration using the phased-…
View article: FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group Open
Combining new H i data from a synergetic survey of Australian Square Kilometre Array Pathfinder (ASKAP) Widefield ASKAP L -band Legacy All-sky Blind surveY and Five-hundred-meter Aperture Spherical radio Telescope with the Arecibo Legacy F…
View article: WALLABY pre-pilot survey: ultra-diffuse galaxies in the Eridanus supergroup
WALLABY pre-pilot survey: ultra-diffuse galaxies in the Eridanus supergroup Open
We present a pilot study of the atomic neutral hydrogen gas (H i) content of ultra-diffuse galaxy (UDG) candidates. In this paper, we use the pre-pilot Eridanus field data from the Widefield ASKAP L-band Legacy All-sky Blind Survey to sear…
View article: WALLABY Pre-Pilot Survey: Ultra-Diffuse Galaxies in the Eridanus Supergroup
WALLABY Pre-Pilot Survey: Ultra-Diffuse Galaxies in the Eridanus Supergroup Open
We present a pilot study of the atomic neutral hydrogen gas (HI) content of ultra-diffuse galaxy (UDG) candidates. In this paper, we use the pre-pilot Eridanus field data from the Widefield ASKAP L-band Legacy All-sky Blind Survey (WALLABY…
View article: WALLABY pilot survey: the potential polar ring galaxies NGC 4632 and NGC 6156
WALLABY pilot survey: the potential polar ring galaxies NGC 4632 and NGC 6156 Open
We report on the discovery of two potential polar ring galaxies (PRGs) in the WALLABY Pilot Data Release 1 (PDR1). These untargeted detections, cross-matched to NGC 4632 and NGC 6156, are some of the first galaxies where the H i observatio…
View article: On the origin of the anomalous gas, non-declining rotation curve, and disc asymmetries in NGC 253
On the origin of the anomalous gas, non-declining rotation curve, and disc asymmetries in NGC 253 Open
We present a multiwavelength (from far-ultraviolet to ${\rm H}\, \rm {\small I}$ emission) study of star formation feedback on the kinematics of the interstellar medium in the Sculptor galaxy, NGC 253. Its three well-known features (a disr…