311 citations · 2.3k across the 89 of their papers we have counts for
11 papers · 1 filter
The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of star-forming galaxies
R. S. Bagge, C. Foster, A. Battisti +17
Galaxy gas kinematics are sensitive to the physical processes that contribute to a galaxy's evolution. It is expected that external processes will cause more significant kinematic…
ProPane: Image Warping with Fire
A. S. G. Robotham, R. Tobar, S. Bellstedt +7
In this paper we introduce the software package ProPane, written for the R data analysis language. ProPane combines the full range of wcslib projections with the C++ image manipula…
The Hyper Suprime-Cam extended Point Spread Functions and applications
L. P. Garate-Nuñez, A. S. G. Robotham, S. Bellstedt +2
We present extended point spread function (PSF) models for the Hyper Suprime-Cam Subaru Strategic Program Public Data Release 3 (HSC-SSP PDR3) in all and $\texti…
Resolving cosmic star formation histories of present-day bulges, disks, and spheroids with ProFuse
Sabine Bellstedt, Aaron S. G. Robotham, Simon P. Driver +3
We present the first look at star formation histories of galaxy components using ProFuse, a new technique to model the 2D distribution of light across multiple wavelengths using si…
GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
Jordan C. J. D'Silva, Simon P. Driver, Claudia D. P. Lagos +11
We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy Survey (DEVILS) observational data sets to calculate the cosmic star formation rate (SFR) and a…
The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
Caro Derkenne, Richard M. McDermid, Adriano Poci +20
We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey. We u…
The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting
Jessica E. Thorne, Aaron S. G. Robotham, Sabine Bellstedt +1
Traditionally, the far ultraviolet (FUV) to far-infrared (FIR) and radio spectral energy distributions (SEDs) of galaxies have been considered separately despite the common physica…
Dynamic Wisp Removal in JWST NIRCam Images
A. S. G. Robotham, J. C. J. D'Silva, R. A. Windhorst +5
The James Webb Space Telescope (JWST) near-infrared camera (NIRCam) has been found to exhibit serious wisp-like structures in four of its eight short-wavelength detectors. The exac…
Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gy
Francesco D'Eugenio, Arjen van der Wel, Joanna M. Piotrowska +37
We present the first study of spatially integrated higher-order stellar kinematics over cosmic time. We use deep rest-frame optical spectroscopy of quiescent galaxies at redshifts…
A New WISE Calibration of Stellar Mass
T. H. Jarrett, M. E. Cluver, Edward N. Taylor +3
We derive new empirical scaling relations between WISE mid-infrared galaxy photometry and well-determined stellar masses from SED modeling of a suite of optical-infrared photometry…
Galaxy quenching timescales from a forensic reconstruction of their colour evolution
Matías Bravo, Aaron S. G. Robotham, Claudia del P. Lagos +3
The timescales on which galaxies move out of the blue cloud to the red sequence () provide insight into the mechanisms driving quenching. Here, we build upon previ…