18.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- J. Bland-Hawthorn3 profiles269 · h 100
- Q. Parker2 profiles146 · h 52
- A. Hopkins2 profiles140 · h 66
- S. Brough129 · h 65
- S. Croom127 · h 55
- M. Colless2 profiles92 · h 70
- K. Glazebrook85 · h 106
- M. Owers85 · h 54
- S. Driver85 · h 94
- J. Lawrence2 profiles77 · h 40
- C. Tinney76 · h 60
- Á. López-Sánchez2 profiles70 · h 68
- Macquarie UniversityAU873 papers
- The University of SydneyAU617 papers
- Australian National UniversityAU525 papers
- Centre National de la Recherche ScientifiqueFR516 papers
- University of CambridgeGB449 papers
- University College LondonGB423 papers
- Swinburne University of TechnologyAU371 papers
- University of SussexGB345 papers
- University of PortsmouthGB331 papers
- University of ChicagoUS328 papers
- University of MichiganUS327 papers
- Centro de Investigaciones Energéticas, Medioambientales y TecnológicasES324 papers
37 papers · 2 filters
SAMI-HI: the connection between global asymmetry in the ionised and neutral atomic hydrogen gas in galaxies
Adam B. Watts, Luca Cortese, Barbara Catinella +7
Observations of the neutral atomic hydrogen (HI) gas in galaxies are predominantly spatially unresolved, in the form of a global HI spectral line. There has been substantial work o…
SAMI-HI: The HI view of the H Tully-Fisher relation and data release
Barbara Catinella, Luca Cortese, Alfred L. Tiley +15
We present SAMI-HI, a survey of the atomic hydrogen content of 296 galaxies with integral field spectroscopy available from the SAMI Galaxy Survey. The sample spans nearly 4 dex in…
Timing the r-Process Enrichment of the Ultra-Faint Dwarf Galaxy Reticulum II
Joshua D. Simon, Thomas M. Brown, Burçin Mutlu-Pakdil +65
The ultra-faint dwarf galaxy Reticulum II (Ret II) exhibits a unique chemical evolution history, with 72 +10/-12% of its stars strongly enhanced in r-process elements. We present d…
A Search for Missing Radio Sources at Using Lyman Dropouts
Devika Shobhana, Ray P. Norris, Miroslav D. Filipović +5
Using the Lyman Dropout technique, we identify 148 candidate radio sources at from the 887.5 MHz Australian Square Kilometer Array Pathfinder (ASKAP) observations…
Dissecting the interstellar medium of a z=6.3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
A. Saccardi, S. D. Vergani, A. De Cia +35
The study of the properties of galaxies in the first billion years after the Big Bang is one of the major topic of current astrophysics. Optical/near-infrared spectroscopy of the a…
Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
Jonghwan Rhee, Martin Meyer, Attila Popping +19
We present early science results from Deep Investigation of Neutral Gas Origins (DINGO), an HI survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP su…
The SAMI Galaxy Survey: Physical drivers of stellar-gas kinematic misalignments in the nearby Universe
A. Ristea, L. Cortese, A. Fraser-McKelvie +10
Misalignments between the rotation axis of stars and gas are an indication of external processes shaping galaxies throughout their evolution. Using observations of 3068 galaxies fr…
Identification of Galaxy-Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
E. A. Zaborowski, A. Drlica-Wagner, F. Ashmead +88
We perform a search for galaxy-galaxy strong lens systems using a convolutional neural network (CNN) applied to imaging data from the first public data release of the DECam Local V…
Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
I. Millan-Irigoyen, M. G. del Valle-Espinosa, R. Fernández-Aranda +5
We present a summary of our project that studies galaxies hosting type Ia supernova (SN Ia) at different redshifts. We present Gran Telescopio de Canarias (GTC) optical spectroscop…
Characterising the Intracluster Light over the Redshift Range in the DES-ACT Overlap
Jesse B. Golden-Marx, Y. Zhang, R. L. C. Ogando +66
We characterise the properties and evolution of Bright Central Galaxies (BCGs) and the surrounding intracluster light (ICL) in galaxy clusters identified in overlapping regions of…
Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks
Ting-Yun Cheng, H. Domínguez Sánchez, J. Vega-Ferrero +54
We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised…
The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
Di Wang, Scott M. Croom, Julia J. Bryant +16
We study environmental quenching using the spatial distribution of current star-formation and stellar population ages with the full SAMI Galaxy Survey. By using a star-formation co…
Discovery of Peculiar Radio Morphologies with ASKAP using Unsupervised Machine Learning
Nikhel Gupta, Minh Huynh, Ray P. Norris +5
We present a set of peculiar radio sources detected using an unsupervised machine learning method. We use data from the Australian Square Kilometre Array Pathfinder (ASKAP) telesco…
Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
Sarah Casura, Jochen Liske, Aaron S. G. Robotham +10
We derive single Sérsic fits and bulge-disk decompositions for 13096 galaxies at redshifts z < 0.08 in the GAMA II equatorial survey regions in the Kilo-Degree Survey (KiDS) g, r a…
The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship
Sam P. Vaughan, Tania M. Barone, Scott M. Croom +14
In this work, we investigate how the central stellar metallicity ([Z/H]) of 1363 galaxies from the SAMI galaxy survey is related to their stellar mass and a proxy for the gravitati…
Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
R. Porter-Temple, B. W. Holwerda, A. M. Hopkins +6
Understanding the effect spiral structure has on star formation properties of galaxies is important to completing our picture of spiral structure evolution. Previous studies have i…
Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity
H. F. M. Yao, M. E. Cluver, T. H. Jarrett +10
The identification of AGN in large surveys has been hampered by seemingly discordant classifications arising from differing diagnostic methods, usually tracing distinct processes s…
Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
Pablo Corcho-Caballero, Yago Ascasibar, Sebastián F. Sánchez +1
We study recent changes on the star formation history (SFH) of galaxies by means of the ageing diagram (AD), tracing the fraction of stars formed during the last Myr thro…
OzDES Reverberation Mapping Program: Mg II Lags and R-L relation
Zhefu Yu, Paul Martini, A. Penton +55
The correlation between the broad line region radius and continuum luminosity ( relation) of active galactic nuclei (AGN) is critical for single-epoch mass estimates of superm…
Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA
C. J. Riseley, E. Bonnassieux, T. Vernstrom +21
Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant substructure. We present new, highly sensitive radio continuum observations of Abell 3266 perfo…
The VMC Survey -- XLIX. Discovery of a population of quasars dominated by nuclear dust emission behind the Magellanic Clouds
Clara M. Pennock, Jacco Th. van Loon, Joy O. Anih +14
Following the discovery of SAGE0536AGN ( 0.14), with the strongest 10-m silicate emission ever observed for an Active Galactic Nucleus (AGN), we discovered SAGE0534AGN (…
The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
Yifan Mai, Sam P. Vaughan, Scott M. Croom +12
Using data from the SAMI Galaxy Survey, we investigate the correlation between the projected stellar kinematic spin vector of 1397 SAMI galaxies and the line-of-sight motion of the…
Low star-formation activity and low gas content of quiescent galaxies at 3.5-4.0 constrained with ALMA
Tomoko L. Suzuki, Karl Glazebrook, Corentin Schreiber +10
The discovery in deep near-infrared surveys of a population of massive quiescent galaxies at has given rise to the question of how they came to be quenched so early in the hi…
The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies
L. Cortese, A. Fraser-McKelvie, J. Woo +8
The stellar surface density within the inner 1 kpc () has become a popular tool for understanding the growth of galaxies and its connection with the quenching of star format…