By Professor Sarah Brough

Conference Papers

Roberts J; Brough S, 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

Brough S, 2007, 'The eridanus supergroup', in Eso Astrophysics Symposia, pp. 261 - 266, http://dx.doi.org/10.1007/978-3-540-71173-5_43

Collins C; Brough S; Burke D; Mann R; Lynam P, 2003, 'The evolution of Brightest Cluster Galaxies', in Astrophysics and Space Science, pp. 51 - 60, http://dx.doi.org/10.1023/A:1024613910300

Preprints

Butler J; Martin G; Hatch NA; Pearce F; Brough S; Dubois Y, 2025, Intracluster light is a biased tracer of the dark matter distribution in clusters, http://dx.doi.org/10.48550/arxiv.2504.03518

Kimmig LC; Brough S; Dolag K; Remus R-S; Bahé YM; Martin G; Pillepich A; Hatch N; Montes M; Ahad SL; Bellhouse C; Brown HJ; Ellien A; Golden-Marx JB; Gonzalez AH; Iodice E; Jiménez-Teja Y; Kluge M; Knapen JH; Mihos JC; Ragusa R; Spavone M, 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

Barsanti S; Croom SM; Colless M; Bland-Hawthorn J; Brough S; Bryant JJ; Lorente N; Oh S; Santucci G; Sweet S; van de Sande J; Welker C, 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

Foster C; Bellstedt S; DEugenio F; Poci A; Bagge R; Harborne K; Venville T; Mendel JT; Lagos CDP; Wisnioski E; Barone TM; Battisti AJ; Barsanti S; Brough S; Croom SM; Derkenne C; Kimmig LC; Mailvaganam A; Remus R-S; Sharma G; Sweet SM; Thater S; Valenzuela LM; Sande JVD; Vaughan SP; Ziegler B, 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

Canepa L; Brough S; Lanusse F; Montes M; Hatch N, 2025, Measuring the intracluster light fraction with machine learning, http://dx.doi.org/10.48550/arxiv.2501.08378

Aguilar-Argüello G; Fuentes-Pineda G; Hernández-Toledo HM; Martínez-Vázquez LA; Vázquez-Mata JA; Brough S; Demarco R; Ghosh A; Jiménez-Teja Y; Martin G; Pearson WJ; Sifón C, 2025, Morphological Classification of Galaxies Through Structural and Star Formation Parameters Using Machine Learning, http://dx.doi.org/10.48550/arxiv.2501.06340

Mun M; Wisnioski E; Harborne KE; Lagos CDP; Valenzuela LM; Remus R-S; Mendel JT; Battisti AJ; Ellison SL; Foster C; Bravo M; Brough S; Croom SM; Gao T; Grasha K; Gupta A; Mai Y; Mailvaganam A; Muller EGM; Sharma G; Sweet SM; Taylor EN; Zafar T, 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

Tuntipong S; Sande JVD; Croom SM; Barsanti S; Bland-Hawthorn J; Brough S; Bryant JJ; Casura S; Fraser-McKelvie A; Lawrence JS; Ristea A; Sweet SM; Zafar T, 2024, The SAMI Galaxy Survey: On the importance of applying multiple selection criteria for finding Milky Way Analogues, http://arxiv.org/abs/2408.12223v1

Bazkiaei AE; Kelvin LS; Brough S; O'Toole SJ; Watkins A; Schmitz MA, 2024, Bright Star Subtraction Pipeline for LSST: Phase one report, http://dx.doi.org/10.48550/arxiv.2408.04387

Khalid A; Brough S; Martin G; Kimmig LC; Lagos CDP; Remus R-S; Martinez-Lombilla C, 2024, Characterising Tidal Features Around Galaxies in Cosmological Simulations, http://arxiv.org/abs/2404.12436v1

Sazonova E; Morgan CR; Balogh M; Alatalo K; Benavides JA; Bluck A; Brough S; Busa I; Demarco R; Donevski D; Figueira M; Martin G; Mullaney JR; Rodriguez-Gomez V; Román J; Rowlands K, 2024, RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution, http://dx.doi.org/10.33232/001c.123524

Bazkiaei AE; Kelvin LS; Brough S; O'Toole SJ; Watkins A; Schmitz MA, 2024, Bright Star Subtraction Pipeline for LSST: Progress Review, http://dx.doi.org/10.48550/arxiv.2404.04802

Prathap J; Hopkins AM; Robotham ASG; Bellstedt S; Afonso J; Ahmed UT; Bilicki M; Bremer MN; Brough S; Brown MJI; Gordon Y; Holwerda BW; Leahy D; López-Sánchez ÁR; Marvil JR; Mukherjee T; Prandoni I; Shabala SS; Vernstrom T; Zafar T, 2024, EMU/GAMA: A Technique for Detecting Active Galactic Nuclei in Low Mass Systems, http://arxiv.org/abs/2402.11817v1

Croom SM; Sande JVD; Vaughan SP; Rutherford TH; Lagos CP; Barsanti S; Bland-Hawthorn J; Brough S; Bryant JJ; Colless M; Cortese L; D'Eugenio F; Fraser-McKelvie A; Goodwin M; Lorente NPF; Richards SN; Ristea A; Sweet SM; Yi SK; Zafar T, 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

Vaughan SP; Sande JVD; Fraser-McKelvie A; Croom S; McDermid R; Liquet-Weiland B; Barsanti S; Cortese L; Brough S; Sweet S; Bryant JJ; Goodwin M; Lawrence J, 2024, The SAMI galaxy survey: predicting kinematic morphology with logistic regression, http://arxiv.org/abs/2402.03676v1

Rutherford TH; Sande JVD; Croom SM; Valenzuela LM; Remus R-S; D'Eugenio F; Vaughan SP; Zovaro HRM; Casura S; Barsanti S; Bland-Hawthorn J; Brough S; Bryant JJ; Goodwin M; Lorente N; Oh S; Ristea A, 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

Małek K; Junais ; Pollo A; Boquien M; Buat V; Salim S; Brough S; Demarco R; Graham AW; Hamed M; Mullaney JR; Romano M; Sifón C; Aravena M; Benavides JA; Busà I; Donevski D; Dorey O; Hernandez-Toledo HM; Nanni A; Pearson WJ; Pistis F; Ragusa R; Riccio G; Román J, 2024, Attenuation proxy hidden in surface brightness-colour diagrams. A new strategy for the LSST era, http://arxiv.org/abs/2401.12831v2

Zovaro HRM; Mendel JT; Groves B; Kewley LJ; Colless M; Ristea A; Cortese L; Oh S; D'Eugenio F; Croom SM; López-Sánchez ÁR; Sande JVD; Brough S; Medling AM; Bland-Hawthorn J; Bryant JJ, 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

Brough S; Ahad SL; Bahe YM; Ellien A; Gonzalez AH; Jiménez-Teja Y; Kimmig LC; Martin G; Martínez-Lombilla C; Montes M; Pillepich A; Ragusa R; Remus R-S; Collins CA; Knapen JH; Mihos JC, 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

Bagge RS; Foster C; Battisti A; Bellstedt S; Mun M; Harborne K; Barsanti S; Mendel T; Brough S; Croom SM; Lagos CDP; Mukherjee T; Peng Y; Remus R-S; Santucci G; Sharda P; Thater S; Sande JVD; Zafar LMVEWT; Ziegler B, 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

Holwerda BW; Phillipps S; Weerasooriya S; Bovill MS; Brough S; Brown MJI; Robertson C; Cook K, 2023, Galaxy And Mass Assembly: The xSAGA Galaxy Complement in Nearby Galaxy Groups, http://arxiv.org/abs/2309.16875v2

Desmons A; Brough S; Lanusse F, 2023, Detecting Tidal Features using Self-Supervised Representation Learning, http://arxiv.org/abs/2307.04967v1

Desmons A; Brough S; Lanusse F, 2023, Detecting Tidal Features using Self-Supervised Representation Learning, http://dx.doi.org/10.48550/arxiv.2307.04967

Montes M; Annibali F; Bellazzini M; Borlaff AS; Brough S; Buitrago F; Chamba N; Collins C; Dell'Antonio I; Escala I; Gonzalez AH; Holwerda B; Kaviraj S; Knapen J; Koekemoer A; Laine S; Marcum P; Martin G; Martinez-Delgado D; Mihos C; Ricotti M; Trujillo I; Watkins AE, 2023, Optimizing Roman's High Latitude Wide Area Survey for Low Surface Brightness Astronomy, http://dx.doi.org/10.48550/arxiv.2306.09414

Desmons A; Brough S; Martínez-Lombilla C; Propris RD; Holwerda B; Sánchez ÁRL, 2023, Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples, http://dx.doi.org/10.1093/mnras/stad1639

D'Eugenio F; Wel AVD; Piotrowska JM; Bezanson R; Taylor EN; Sande JVD; Baker WM; Bell EF; Bellstedt S; Bland-Hawthorn J; Bluck AFL; Brough S; Bryant JJ; Colless M; Cortese L; Croom SM; Derkenne C; Dokkum PV; Fisher D; Foster C; Gallazzi A; Graaff AD; Groves B; Houdt JV; Lagos CDP; Looser TJ; Maiolino R; Maseda M; Mendel JT; Nersesian A; Pacifici C; Poci A; Remus R-S; Sweet SM; Thater S; Tran K-V; Übler H; Valenzuela LM; Wisnioski E; Zibetti S, 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

D'Eugenio F; Wel AVD; Derkenne C; Houdt JV; Bezanson R; Taylor EN; Sande JVD; Baker WM; Bell EF; Bland-Hawthorn J; Bluck AFL; Brough S; Bryant JJ; Colless M; Cortese L; Croom SM; Dokkum PV; Fisher D; Foster C; Fraser-McKelvie A; Gallazzi A; Graaff AD; Groves B; Lagos CDP; Looser TJ; Maiolino R; Maseda M; Mendel JT; Nersesian A; Pacifici C; Piotrowska JM; Poci A; Remus R-S; Sharma G; Sweet SM; Thater S; Tran KV; Übler H; Valenzuela LM; Wisnioski E; Zibetti S, 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

Santucci G; Brough S; Sande JVD; McDermid R; Barsanti S; Bland-Hawthorn J; Bryant JJ; Croom SM; Lagos C; Lawrence JS; Owers MS; Ven GVD; Vaughan SP; Yi SK, 2023, The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies, http://dx.doi.org/10.1093/mnras/stad713

Foster C; Vaughan S; Fraser-McKelvie A; Brough S; Bryant JJ; Croom SM; D'Eugenio F; Groves B; Konstantopoulos IS; López-Sánchez ÁR; Oh S; Owers MS; Sweet SM; Sande JVD; Wisnioski E; Yi SK; Zovaro HRM, 2023, The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations, http://dx.doi.org/10.1093/mnras/stad487

Knabel S; Holwerda BW; Nightingale J; Treu T; Bilicki M; Brough S; Driver S; Finnerty L; Haberzettl L; Hegde S; Hopkins AM; Kuijken K; Liske J; Pimbblet KA; Steele RC; Wright AH, 2023, Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA, http://dx.doi.org/10.1093/mnras/stad133

Ragusa R; Iodice E; Spavone M; Montes M; Forbes DA; Brough S; Mirabile M; Cantiello M; Paolillo M; Schipani P, 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

Martinez-Lombilla C; Brough S; Montes M; Baena-Galle R; Akhlaghi M; Infante-Sainz R; Driver SP; Holwerda BW; Pimbblet KA; Robotham ASG, 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

Smith D; Haberzettl L; Porter LE; Porter-Temple R; Henry CPA; Holwerda B; Lopez-Sanchez AR; Phillipps S; Graham AW; Brough S; Pimbblet KA; Liske J; Kelvin LS; Robertson CD; Roemer W; Walmsley M; O'Ryan D; Geron T, 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

Bhambhani PC; Baldry IK; Brough S; Hill AD; Lara-Lopez MA; Loveday J; Holwerda BW, 2022, Red riding on hood: Exploring how galaxy colour depends on environment, http://dx.doi.org/10.1093/mnras/stad1218

Rhee J; Meyer M; Popping A; Bellstedt S; Driver SP; Robotham ASG; Whiting M; Baldry IK; Brough S; Brown MJI; Bunton JD; Dodson R; Holwerda BW; Hopkins AM; Koribalski BS; Lee-Waddell K; López-Sánchez ÁR; Loveday J; Mahony E; Roychowdhury S; Rozgonyi K; Staveley-Smith L, 2022, Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data, http://dx.doi.org/10.1093/mnras/stac3065

Ristea A; Cortese L; Fraser-McKelvie A; Brough S; Bryant JJ; Catinella B; Croom SM; Groves B; Richards SN; Sande JVD; Bland-Hawthorn J; Owers MS; Lawrence JS, 2022, The SAMI Galaxy Survey: Physical drivers of stellar-gas kinematic misalignments in the nearby Universe, http://dx.doi.org/10.1093/mnras/stac2839

Wang D; Croom SM; Bryant JJ; Vaughan SP; Schaefer AL; D'Eugenio F; Barsanti S; Brough S; Lagos CDP; Medling AM; Oh S; Sande JVD; Santucci G; Bland-Hawthorn J; Goodwin M; Groves B; Lawrence J; Owers MS; Richards S, 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

Casura S; Liske J; Robotham ASG; Brough S; Driver SP; Graham AW; Häußler B; Holwerda BW; Hopkins AM; Kelvin LS; Moffett AJ; Taranu DS; Taylor EN, 2022, Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe, http://dx.doi.org/10.1093/mnras/stac2267

Vaughan SP; Barone TM; Croom SM; Cortese L; D'Eugenio F; Brough S; Colless M; McDermid RM; Sande JVD; Scott N; Bland-Hawthorn J; Bryant JJ; Lawrence JS; López-Sánchez ÁR; Lorente NPF; Owers MS; Richards SN, 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

Yao HFM; Cluver ME; Jarrett TH; Jozsa GIG; Santos MG; Marchetti L; Brown MJI; Gordon YA; Brough S; Hopkins AM; Holwerda BW; Driver SP; Sadler EM, 2022, Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity, http://dx.doi.org/10.3847/1538-4357/ac8790

Cooke J; Angus C; Auchettl K; Bally J; Bolin B; Brough S; Burchett JN; Foley R; Foran G; Forbes D; Gannon J; Hirai R; Kacprzak GG; Margutti R; Martinez-Lombilla C; Mestric U; Moller A; Rest A; Rhodes J; Rich RM; Schussler F; Wainscoat R; Walawender J; Wold I; Zhang J, 2022, Science Cases for the Keck Wide-Field Imager, http://dx.doi.org/10.48550/arxiv.2207.11698

Mai Y; Vaughan SP; Croom SM; Sande JVD; Barsanti S; Bland-Hawthorn J; Brough S; Bryant JJ; Colless M; Goodwin M; Groves B; Konstantopoulos IS; Lawrence JS; Lorente NPF; Richards SN, 2022, The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours, http://dx.doi.org/10.1093/mnras/stac1841

Watson PJ; Davies RL; Sande JVD; Brough S; Croom SM; D'Eugenio F; Glazebrook K; Groves B; López-Sánchez ÁR; Scott N; Vaughan SP; Walcher CJ; Bland-Hawthorn J; Bryant JJ; Goodwin M; Lawrence JS; Lorente NPF; Owers MS; Richards S, 2022, The SAMI Galaxy Survey: The Link Between [$α$/Fe] and Kinematic Morphology, http://dx.doi.org/10.1093/mnras/stac1221

Häußler B; Vika M; Bamford SP; Johnston EJ; Brough S; Casura S; Holwerda BW; Kelvin LS; Popescu C, 2022, Galapagos-2/Galfitm/GAMA -- multi-wavelength measurement of galaxy structure: separating the properties of spheroid and disk components in modern surveys, http://dx.doi.org/10.1051/0004-6361/202142935

Cortese L; Fraser-McKelvie A; Woo J; Catinella B; Harborne K; Sande JVD; Bland-Hawthorn J; Brough S; Bryant JJ; Croom S; Sweet S, 2022, The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies, http://dx.doi.org/10.1093/mnras/stac1023

Crossett JP; McGee SL; Ponman TJ; Ramos-Ceja ME; Brown MJI; Maughan BJ; Robotham ASG; Willis JP; Wood C; Bland-Hawthorn J; Brough S; Driver SP; Holwerda BW; Hopkins AM; Loveday J; Owers MS; Phillipps S; Pierre M; Pimbblet KA, 2022, The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission, http://dx.doi.org/10.1051/0004-6361/202142057

Driver SP; Robotham ASG; Obreschkow D; Peacock JA; Baldry IK; Bellstedt S; Bland-Hawthorn J; Brough S; Cluver M; Holwerda BW; Hopkins A; Lagos C; Liske J; Loveday J; Phillipps S; Taylor EN, 2022, An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data, http://dx.doi.org/10.1093/mnras/stac581

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