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.
Papers
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Journal ArticleDOI
The SAMI galaxy survey: Kinematics of dusty early-type galaxies
R. Bassett,Kenji Bekki,Luca Cortese,Warrick J. Couch,Anne E. Sansom,J. van de Sande,Julia J. Bryant,Julia J. Bryant,Caroline Foster,Scott M. Croom,Sarah Brough,Sarah M. Sweet,Anne M. Medling,Anne M. Medling,Matt S. Owers,Matt S. Owers,Simon P. Driver,Luke J. M. Davies,O. I. Wong,Brent Groves,Joss Bland-Hawthorn,Samuel N. Richards,Samuel N. Richards,Michael Goodwin,Iraklis S. Konstantopoulos,Jon Lawrence +25 more
TL;DR: In this paper, the authors examined the 2D stellar and ionized gas kinematics of dusty early-type galaxies using integral field spectroscopy observations from the SAMI Galaxy Survey, and integrated star formation rates, stellar masses and dust masses from the GAMA survey.
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The buildup of the intracluster light of Abell 85 as seen by Subaru's Hyper Suprime-Cam
TL;DR: In this article, the authors measured the radial surface brightness profiles of the Abell 85 galaxy out to the intracluster light (radius $1.215$ kpc), for the g and i bands.
Journal ArticleDOI
Radio and Deep Chandra Observations of the Disturbed Cool Core Cluster Abell 133
Scott W. Randall,Tracy Clarke,Paul Nulsen,Matt S. Owers,Craig L. Sarazin,William R. Forman,S. S. Murray +6 more
TL;DR: In this paper, Chandra and multi-frequency radio observations of the disturbed cool core cluster Abell 133 were used to find evidence for a weak elliptical X-ray surface brightness edge surrounding the core.
Journal ArticleDOI
The SAMI Pilot Survey: the fundamental and mass planes in three low-redshift clusters
Nicholas Scott,Lisa Fogarty,Matt S. Owers,Matt S. Owers,Scott M. Croom,Matthew Colless,Roger L. Davies,Sarah Brough,Michael Pracy,Joss Bland-Hawthorn,D. Heath Jones,D. Heath Jones,J. T. Allen,Julia J. Bryant,Julia J. Bryant,Luca Cortese,Michael Goodwin,Andrew W. Green,I. S. Konstantopoulos,Jon Lawrence,Jon Lawrence,Samuel N. Richards,Samuel N. Richards,Rob Sharp +23 more
TL;DR: In this paper, the intrinsic scatter of the Fundamental Plane depends on the way in which the velocity dispersion and effective radius are measured, and it is shown that the resulting Mass Plane has further reduced scatter, consistent with zero intrinsic scatter.
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The SAMI Galaxy Survey: gravitational potential and surface density drive stellar populations -- I. early-type galaxies.
Tania M. Barone,Francesco D'Eugenio,Matthew Colless,Nicholas Scott,Jesse van de Sande,Joss Bland-Hawthorn,Sarah Brough,Julia J. Bryant,Julia J. Bryant,Luca Cortese,Scott M. Croom,Caroline Foster,Michael Goodwin,Iraklis S. Konstantopoulos,Jon Lawrence,Nuria P. F. Lorente,Anne M. Medling,Anne M. Medling,Matt S. Owers,Matt S. Owers,Samuel N. Richards +20 more
TL;DR: For early-type galaxies, the authors found that the color and stellar metallicity [Z/H] correlate more strongly with gravitational potential than with mass $M$, whereas stellar population age correlates best with surface density $Sigma.