ORCID as entered in ROS
https://orcid.org/0000-0002-9796-1363
Select Publications
Conference Papers
, 2015, 'LSST and Australia', in Lorente NPF; Shortridge K; Wayth R (eds.), ASTRONOMICAL DATA ANALYSIS SOFTWARE AND SYSTEMS XXV, ASTRONOMICAL SOC PACIFIC, AUSTRALIA, ARC Ctr Excellence All Sky Astrophys (CAASTRO), Sydney, pp. 667 - 669, presented at
, 2014, 'How do brightest cluster galaxies grow?', in Revista Mexicana De Astronomia Y Astrofisica Serie De Conferencias, pp. 87
, 2013, 'A framework to aid adoption of automated rehabilitation devices into clinical practice Synthesising and Interpreting Language for Clinical Kinematics (SILCK)', in 2013 IEEE 13TH INTERNATIONAL CONFERENCE ON REHABILITATION ROBOTICS (ICORR), IEEE, WA, Univ Washington Campus, Seattle, presented at
, 2012, 'SAMI - A new multi-object IFS for the Anglo-Australian telescope', in Proceedings of SPIE the International Society for Optical Engineering, http://dx.doi.org/10.1117/12.925115
, 2009, 'Developing the rock physics model - Improved carbon dioxide mixing rules for Carbon Capture and Storage', in 71st European Association of Geoscientists and Engineers Conference and Exhibition 2009 Balancing Global Resources Incorporating SPE Europec 2009, pp. 1899 - 1903, http://dx.doi.org/10.3997/2214-4609.201400270
, 2007, 'The eridanus supergroup', in Eso Astrophysics Symposia, pp. 261 - 266, http://dx.doi.org/10.1007/978-3-540-71173-5_43
, 2003, 'The evolution of Brightest Cluster Galaxies', in Astrophysics and Space Science, pp. 51 - 60, http://dx.doi.org/10.1023/A:1024613910300
Preprints
, 2025, Tidal features around simulated groups and cluster galaxies: Enhancement and suppression of merger events through environment in LSST-like mock observations, http://dx.doi.org/10.48550/arxiv.2509.20723
, 2025, Analysing the prevalence of tidal features in HSC-SSP using self-supervised representation learning, http://dx.doi.org/10.48550/arxiv.2509.18274
, 2025, The intragroup light in KiDS+GAMA groups: A stacking analysis, http://dx.doi.org/10.48550/arxiv.2509.00233
, 2025, Cluster passage driving galaxy kinematic and structural evolution in the SAMI Galaxy Survey, http://dx.doi.org/10.48550/arxiv.2508.07589
, 2025, Intracluster light is a biased tracer of the dark matter distribution in clusters, http://dx.doi.org/10.48550/arxiv.2504.03518
, 2025, Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations, http://dx.doi.org/10.48550/arxiv.2503.20857
, 2025, The SAMI Galaxy Survey: large-scale environment affects galaxy spin amplitudes and the formation of slow rotators, http://dx.doi.org/10.48550/arxiv.2503.09052
, 2025, The MAGPI Survey: the subtle role of environment and not-so-subtle impact of generations of stars on galaxy dynamics, http://dx.doi.org/10.1017/pasa.2025.11
, 2025, Measuring the intracluster light fraction with machine learning, http://dx.doi.org/10.48550/arxiv.2501.08378
, 2025, Morphological Classification of Galaxies Through Structural and Star Formation Parameters Using Machine Learning, http://dx.doi.org/10.48550/arxiv.2501.06340
, 2024, The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at $z \sim$ 0.3, http://arxiv.org/abs/2411.17882v1
, 2024, The SAMI Galaxy Survey: On the importance of applying multiple selection criteria for finding Milky Way Analogues, http://arxiv.org/abs/2408.12223v1
, 2024, Bright Star Subtraction Pipeline for LSST: Phase one report, http://dx.doi.org/10.48550/arxiv.2408.04387
, 2024, Characterising Tidal Features Around Galaxies in Cosmological Simulations, http://arxiv.org/abs/2404.12436v1
, 2024, RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution, http://dx.doi.org/10.33232/001c.123524
, 2024, Bright Star Subtraction Pipeline for LSST: Progress Review, http://dx.doi.org/10.48550/arxiv.2404.04802
, 2024, EMU/GAMA: A Technique for Detecting Active Galactic Nuclei in Low Mass Systems, http://arxiv.org/abs/2402.11817v1
, 2024, The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment, http://dx.doi.org/10.1093/mnras/stae458
, 2024, The SAMI galaxy survey: predicting kinematic morphology with logistic regression, http://arxiv.org/abs/2402.03676v1
, 2024, The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies, http://dx.doi.org/10.1093/mnras/stae398
, 2024, Attenuation proxy hidden in surface brightness-colour diagrams. A new strategy for the LSST era, http://arxiv.org/abs/2401.12831v2
, 2023, The SAMI Galaxy Survey: $Σ_{\rm SFR}$ drives the presence of complex emission line profiles in star-forming galaxies, http://arxiv.org/abs/2312.03659v1
, 2023, Preparing for low surface brightness science with the Vera C. Rubin Observatory: A Comparison of Observable and Simulated Intracluster Light Fractions, http://arxiv.org/abs/2311.18016v1
, 2023, The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of $z\sim0.3$ star-forming galaxies, http://arxiv.org/abs/2311.10268v2
, 2023, Galaxy And Mass Assembly: The xSAGA Galaxy Complement in Nearby Galaxy Groups, http://arxiv.org/abs/2309.16875v2
, 2023, Detecting Tidal Features using Self-Supervised Representation Learning, http://arxiv.org/abs/2307.04967v1
, 2023, Detecting Tidal Features using Self-Supervised Representation Learning, http://dx.doi.org/10.48550/arxiv.2307.04967
, 2023, Optimizing Roman's High Latitude Wide Area Survey for Low Surface Brightness Astronomy, http://dx.doi.org/10.48550/arxiv.2306.09414
, 2023, Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples, http://dx.doi.org/10.1093/mnras/stad1639
, 2023, 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, http://arxiv.org/abs/2303.05520v1
, 2023, Different higher-order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI and LEGA-C surveys, http://arxiv.org/abs/2303.04157v1
, 2023, The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies, http://dx.doi.org/10.1093/mnras/stad713
, 2023, The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations, http://dx.doi.org/10.1093/mnras/stad487
, 2023, Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA, http://dx.doi.org/10.1093/mnras/stad133
, 2022, Does the virial mass drive the intra-cluster light? The relationship between the ICL and M$_{vir}$ from VEGAS, http://dx.doi.org/10.1051/0004-6361/202245530
, 2022, Galaxy and Mass Assembly (GAMA): Extended Intra-Group Light in a group at $z=0.2$ from deep Hyper-Suprime Cam images, http://dx.doi.org/10.1093/mnras/stac3119
, 2022, Galaxy And Mass Assembly: Galaxy Morphology in the Green Valley, Prominent rings and looser Spiral Arms, http://dx.doi.org/10.48550/arxiv.2211.08355
, 2022, Red riding on hood: Exploring how galaxy colour depends on environment, http://dx.doi.org/10.1093/mnras/stad1218
, 2022, Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data, http://dx.doi.org/10.1093/mnras/stac3065
, 2022, The SAMI Galaxy Survey: Physical drivers of stellar-gas kinematic misalignments in the nearby Universe, http://dx.doi.org/10.1093/mnras/stac2839
, 2022, The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching, http://dx.doi.org/10.1093/mnras/stac2428
, 2022, Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe, http://dx.doi.org/10.1093/mnras/stac2267
, 2022, The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationship, http://dx.doi.org/10.1093/mnras/stac2304
https://orcid.org/0000-0002-9796-1363