M
Matt S. Owers
Researcher at Macquarie University
Publications - 227
Citations - 10584
Matt S. Owers is an academic researcher from Macquarie University. The author has contributed to research in topics: Galaxy & Stellar mass. The author has an hindex of 56, co-authored 217 publications receiving 8765 citations. Previous affiliations of Matt S. Owers include University of Hull & Australian Research Council.
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Journal ArticleDOI
A High Fidelity Sample of Cold Front Clusters from the Chandra Archive
TL;DR: In this article, the authors presented a sample of cold front clusters from the Chandra archive, which were selected based purely on the existence of surface brightness edges in their Chandra images which are modeled as density jumps.
Journal ArticleDOI
The Sami Galaxy Survey: revisiting galaxy classification through high-order stellar kinematics
Jesse van de Sande,Joss Bland-Hawthorn,L. M. R. Fogarty,Luca Cortese,Francesco D'Eugenio,Scott M. Croom,Nicholas Scott,James T. Allen,Sarah Brough,Julia J. Bryant,Julia J. Bryant,Gerald Cecil,Matthew Colless,Warrick J. Couch,Roger L. Davies,Pascal J. Elahi,Caroline Foster,Gregory Goldstein,Michael Goodwin,Brent Groves,I. Ting Ho,Hyunjin Jeong,D. Heath Jones,Iraklis S. Konstantopoulos,Jon Lawrence,Sarah K. Leslie,Sarah K. Leslie,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Richard M. McDermid,Richard M. McDermid,Rebecca McElroy,Anne M. Medling,Anne M. Medling,Sree Oh,Matt S. Owers,Matt S. Owers,Samuel N. Richards,Samuel N. Richards,Adam L. Schaefer,Adam L. Schaefer,Rob Sharp,Sarah M. Sweet,Dan S. Taranu,C. Tonini,C. Jakob Walcher,Sukyoung K. Yi +46 more
TL;DR: In this paper, the authors measured the stellar kinematics on a sample of 315 galaxies, without a morphological selection, using two-dimensional integral field data from the SAMI Galaxy Survey and developed an alternative approach to kinematically classify galaxies from their individual h_3 versus V/σ signatures.
Journal ArticleDOI
Galaxy And Mass Assembly (GAMA): a deeper view of the mass, metallicity and SFR relationships
Maritza A. Lara-López,Andrew M. Hopkins,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Sarah Brough,Madusha Gunawardhana,Madusha Gunawardhana,Matthew Colless,Aaron S. G. Robotham,Aaron S. G. Robotham,Amanda E. Bauer,Joss Bland-Hawthorn,Michelle E. Cluver,Simon P. Driver,Simon P. Driver,Caroline Foster,Lee S. Kelvin,Lee S. Kelvin,Jochen Liske,Jon Loveday,Matt S. Owers,Trevor J. Ponman,Rob Sharp,O. Steele,Edward N. Taylor,Edward N. Taylor,Daniel Thomas +26 more
TL;DR: In this paper, the relationship between SFR, M*, Z and specific SFR (SSFR) on the Fundamental Plane for star-forming galaxies is investigated. But the dependence of SFR and metallicity evolution to z ∼ 0.2 is not investigated.
Journal ArticleDOI
Galaxy And Mass Assembly (GAMA) : trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments
Mehmet Alpaslan,Mehmet Alpaslan,Simon P. Driver,Simon P. Driver,Aaron S. G. Robotham,Danail Obreschkow,E. Andrae,Michelle E. Cluver,Lee S. Kelvin,Rebecca A. Lange,Matt S. Owers,Matt S. Owers,Edward N. Taylor,Stephen K. Andrews,Steven P. Bamford,Joss Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Matthew Colless,Luke J. M. Davies,Elizabeth Eardley,Meiert W. Grootes,Andrew M. Hopkins,Rebecca Kennedy,Jochen Liske,Maritza A. Lara-López,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Jon Loveday,Barry F. Madore,Smriti Mahajan,Martin Meyer,Amanda J. Moffett,Peder Norberg,Samantha J. Penny,Kevin A. Pimbblet,Kevin A. Pimbblet,Cristina C. Popescu,Cristina C. Popescu,Mark Seibert,Richard J. Tuffs +40 more
TL;DR: In this paper, the authors explore trends in galaxy properties with Mpc-scale structures using catalogues of environment and large-scale structure from the Galaxy And Mass Assembly (GAMA) survey.
Journal ArticleDOI
The XXL Survey. II. The bright cluster sample: catalogue and luminosity function
Florian Pacaud,N. Clerc,Paul Giles,C. Adami,T. Sadibekova,Marguerite Pierre,Ben J Maughan,M. Lieu,J. P. Le Fevre,Sinan Aliş,Sinan Aliş,Bruno Altieri,F. Ardila,Ivan K. Baldry,C. Benoist,Mark Birkinshaw,L. Chiappetti,J. Démoclès,Dominique Eckert,August E. Evrard,L. Faccioli,Fabio Gastaldello,L. Guennou,Cathy Horellou,A. Iovino,Elias Koulouridis,V. Le Brun,Christopher Lidman,Jochen Liske,Sophie Maurogordato,Felipe Menanteau,Matt S. Owers,Matt S. Owers,Bianca M. Poggianti,Daniel Pomarède,E. Pompei,Trevor J. Ponman,David Rapetti,David Rapetti,Thomas H. Reiprich,Graham P. Smith,Richard J. Tuffs,Patrick Valageas,Ivan Valtchanov,Jon Willis,F. Ziparo +45 more
TL;DR: The XXL bright cluster sample as discussed by the authors is a subsample of 100 galaxy clusters selected from the full XXL catalogue by setting a lower limit of $3\times 10^{-14}\,\mathrm{erg \,s^{-1}cm^{-2}) on the source flux within a 1$^{\prime}$ aperture.