Sam P. Vaughan - Sch Math & Phys Sci, Macquarie Univ

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论文共 49 篇作者统计合作学者相似作者

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The MAGPI Survey: the Kinematic Morphology-Density Relation (or Lack Thereof) and the Hubble Sequence at Z∼0.3

Caroline Foster, Mark W. Donoghoe,Andrew Battisti,Francesco D'Eugenio, Katherine Harborne, Thomas Venville,Claudia Del P. Lagos,J. Trevor Mendel, Ryan Bagge,Stefania Barsanti,Sabine Bellstedt, Alina Boecker, Qianhui Chen,Caro Derkenne, Anna Ferre-Matteu, Eda Gjergo,Anshu Gupta, Eric G. M. Muller,Giulia Santucci, Hye-Jin Park,Rhea-Silvia Remus,Sabine Thater,Jesse van de Sande,Sam Vaughan,Sarah Brough, Scott M. Croom,Lucas M. Valenzuela,Emily Wisnioski, the MAGPI Team

arxiv（2025）

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The MAGPI Survey: the Subtle Role of Environment and Not-So-subtle Impact of Generations of Stars on Galaxy Dynamics

Caroline Foster,Sabine Bellstedt, Francesco DEugenio,Adriano Poci, Ryan Bagge, Katherine Harborne, Thomas Venville,J. Trevor Mendel,Claudia Del P. Lagos,Emily Wisnioski,Tania M. Barone,Andrew J. Battisti,Stefania Barsanti,Sarah Brough, Scott M. Croom,Caro Derkenne,Lucas C. Kimmig, Anilkumar Mailvaganam,Rhea-Silvia Remus,Gauri Sharma,Sarah M. Sweet,Sabine Thater,Lucas M. Valenzuela,Jesse van de Sande,Sam P. Vaughan,Bodo Ziegler

arxiv（2025）

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The SAMI Galaxy Survey: Fossil Group Centrals Are No More Likely to Be Slow Rotators

Frank Scuccimarra, Scott M. Croom,Jesse van de Sande,Stefania Barsanti,Sarah Brough,Julia J. Bryant,Lucas C. Kimmig,Claudia Lagos,Rhea-Silvia Remus,Andrei Ristea,Sarah M. Sweet,Sam Vaughan

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA (2024)

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The SAMI Galaxy Survey: Predicting Kinematic Morphology with Logistic Regression

Sam P. Vaughan,Jesse van de Sande,A. Fraser-McKelvie,Scott Croom,Richard Mcdermid,Benoit Liquet-Weiland,Stefania Barsanti,Luca Cortese,Sarah Brough,Sarah Sweet,Julia J. Bryant,Michael Goodwin,Jon Lawrence

Monthly Notices of the Royal Astronomical Societyno. 4 (2024): 5852-5863

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The MAGPI Survey: Using Kinematic Asymmetries in Stars and Gas to Dissect Drivers of Galaxy Dynamical Evolution

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 3 (2024): 3011-3022

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The MAGPI Survey: the Evolution and Drivers of Gas Turbulence in Intermediate-Redshift Galaxies

Monthly Notices of the Royal Astronomical Society (2024)

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The Hyperplane of Early-Type Galaxies: Using Stellar Population Properties to Increase the Precision and Accuracy of the Fundamental Plane As a Distance Indicator

Francesco D'Eugenio,Matthew Colless,Arjen van der Wel,Sam P. Vaughan,Khaled Said,Jesse van de Sande,Joss Bland-Hawthorn,Julia J. Bryant,Scott M. Croom,angel R. Lopez-Sanchez,Nuria P. F. Lorente,Roberto Maiolino,Edward N. Taylor

Monthly Notices of the Royal Astronomical Societyno. 2 (2024): 1775-1795

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Hector - Performance of the New Integral Field Spectrograph Instrument for the Anglo-Australian Telescope

Julia J. Bryant,Sree Oh,Madusha Gunawardhana, Gabriella Quattropani, Gurashish Singh Bhatia,Joss Bland-Hawthorn, David Broderick,Rebecca Brown,Robert Content,Scott Croom,Fred Crous,Tony Farrell,Peter Gillingham,Ellen Houston,Jon Lawrence,Helen McGregor, Seong-Sik Minh,Mahesh Mohanan,Barnaby Norris,Matthew Owers,Naveen Pai,David Robertson,Will Saunders,Sam Vaughan,Sudharshan Venkatesan,Adeline Wang,Ross Zhelem,Jessica Zheng

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY X (2024)

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Validating Full-Spectrum Fitting with a Synthetic Integral-Field Spectroscopic Observation of the Milky Way

Zixian Wang,Sanjib Sharma,Michael R. Hayden,Jesse van de Sande,Joss Bland-Hawthorn,Sam Vaughan,Marie Martig,Francesca Pinna

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 2 (2024): 1175-1204

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The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies

Tomas H. Rutherford,Jesse van de Sande,Scott M. Croom,Lucas M. Valenzuela,Rhea-Silvia Remus,Francesco D'Eugenio,Sam P. Vaughan,Henry R. M. Zovaro,Sarah Casura,Stefania Barsanti,Joss Bland-Hawthorn,Sarah Brough,Julia J. Bryant,Michael Goodwin,Nuria Lorente,Sree Oh,Andrei Ristea

Monthly Notices of the Royal Astronomical Society (2024)

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