Scheduled Maintenance Notice
Please note that Researcher Profiles will be undergoing scheduled maintenance on Wednesday 7th Oct, from 8:00am to 9:00am. During this time, the Researcher Profiles system will be unavailable. We apologise for any inconvenience and appreciate your understanding.
Select Publications
Preprints
, 2026, The SAMI Galaxy Survey: Linking Tidal Features and Orbit Populations Using Schwarzschild Modelling, http://dx.doi.org/10.48550/arxiv.2608.14012
, 2026, Comparison and verification methods to trace interaction-driven disturbances in galaxies, http://dx.doi.org/10.48550/arxiv.2606.11313
, 2026, Tidal features as tracers of galaxy merger histories: the colours of tidal features in HSC-SSP, http://dx.doi.org/10.48550/arxiv.2601.20974
, 2025, The dependence of the intracluster light fraction on galaxy cluster properties, http://dx.doi.org/10.48550/arxiv.2512.05187
, 2025, Investigating the imprints of tidal features on simulated galaxy outskirts in LSST-like mock observations, http://dx.doi.org/10.48550/arxiv.2511.05424
, 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 kinematic morphology-density relation (or lack thereof) and the Hubble sequence at $z\sim0.3$, https://arxiv.org/abs/2502.16751v1
, 2025, Measuring the intracluster light fraction with machine learning, http://dx.doi.org/10.48550/arxiv.2501.08378
, 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/10.48550/arxiv.2501.08461
, 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://dx.doi.org/10.48550/arxiv.2411.17882
, 2024, RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution, http://dx.doi.org/10.48550/arxiv.2404.05792
, 2024, The SAMI Galaxy Survey: On the importance of applying multiple selection criteria for finding Milky Way Analogues, http://dx.doi.org/10.48550/arxiv.2408.12223
, 2024, Bright Star Subtraction Pipeline for LSST: Phase one report, http://dx.doi.org/10.48550/arxiv.2408.04387
, 2024, Detecting Galaxy Tidal Features Using Self-Supervised Representation Learning, http://dx.doi.org/10.48550/arxiv.2308.07962
, 2024, Characterising Tidal Features Around Galaxies in Cosmological Simulations, http://dx.doi.org/10.48550/arxiv.2404.12436
, 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://dx.doi.org/10.48550/arxiv.2402.11817
, 2024, The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment, http://dx.doi.org/10.48550/arxiv.2402.06877
, 2024, The SAMI galaxy survey: predicting kinematic morphology with logistic regression, http://dx.doi.org/10.48550/arxiv.2402.03676
, 2024, The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies, http://dx.doi.org/10.48550/arxiv.2402.02728
, 2024, Attenuation proxy hidden in surface brightness-colour diagrams. A new strategy for the LSST era, http://dx.doi.org/10.48550/arxiv.2401.12831
, 2023, The SAMI Galaxy Survey: $Σ_{\rm SFR}$ drives the presence of complex emission line profiles in star-forming galaxies, http://dx.doi.org/10.48550/arxiv.2312.03659
, 2023, Preparing for low surface brightness science with the Vera C. Rubin Observatory: A Comparison of Observable and Simulated Intracluster Light Fractions, http://dx.doi.org/10.48550/arxiv.2311.18016
, 2023, The MAGPI Survey: Drivers of kinematic asymmetries in the ionised gas of $z\sim0.3$ star-forming galaxies, http://dx.doi.org/10.48550/arxiv.2311.10268
, 2023, Galaxy And Mass Assembly: The xSAGA Galaxy Complement in Nearby Galaxy Groups, http://dx.doi.org/10.48550/arxiv.2309.16875
, 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/10.48550/arxiv.2305.17894
, 2023, Red riding on hood: Exploring how galaxy colour depends on environment, http://dx.doi.org/10.48550/arxiv.2210.16112
, 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://dx.doi.org/10.48550/arxiv.2303.05520
, 2023, Different higher-order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI and LEGA-C surveys, http://dx.doi.org/10.48550/arxiv.2303.04157
, 2023, The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies, http://dx.doi.org/10.48550/arxiv.2303.04161
, 2023, The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations, http://dx.doi.org/10.48550/arxiv.2302.06712
, 2023, Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA, http://dx.doi.org/10.48550/arxiv.2301.05320
, 2022, Does the virial mass drive the intra-cluster light? The relationship between the ICL and M$_{vir}$ from VEGAS, http://dx.doi.org/10.48550/arxiv.2212.06164
, 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/10.48550/arxiv.2211.12749
, 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, Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data, http://dx.doi.org/10.48550/arxiv.2210.09697
, 2022, The SAMI Galaxy Survey: Physical drivers of stellar-gas kinematic misalignments in the nearby Universe, http://dx.doi.org/10.48550/arxiv.2210.01147
, 2022, The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching, http://dx.doi.org/10.48550/arxiv.2209.00290
, 2022, Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe, http://dx.doi.org/10.48550/arxiv.2208.07608
, 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/10.48550/arxiv.2208.06939
, 2022, Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity, http://dx.doi.org/10.48550/arxiv.2208.01679