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
GAMA/H-ATLAS: a meta-analysis of SFR indicators – comprehensive measures of the SFR–M* relation and cosmic star formation history at z < 0.4
Luke J. M. Davies,Simon P. Driver,Simon P. Driver,Aaron S. G. Robotham,Meiert W. Grootes,Cristina Carmen Popescu,Richard J. Tuffs,Andrew M. Hopkins,Mehmet Alpaslan,Stephen K. Andrews,Jonathan Bland-Hawthorn,Malcolm N. Bremer,Sarah Brough,Michael J. I. Brown,Michelle E. Cluver,Scott M. Croom,E. da Cunha,Loretta Dunne,Maritza A. Lara-López,Jochen Liske,Jonathan Loveday,Amanda J. Moffett,Matt S. Owers,S. Phillipps,Anne E. Sansom,Edward N. Taylor,Michał J. Michałowski,Edo Ibar,Matthew Smith,Nathan Bourne +29 more
TL;DR: In this paper, a meta-analysis of star-formation rate (SFR) indicators in the GAMA survey, producing 12 different SFR metrics and determining the SFR-M* relation for each.
Journal ArticleDOI
An example of 3D conductivity mapping using the TEMPEST airborne electromagnetic system
Richard Lane,Andy Green,Chris Golding,Matt S. Owers,Phil Pik,Caleb Plunkett,Daniel Sattel,Bob Thorn +7 more
TL;DR: The TEMPEST airborne electromagnetic system is designed to measure the information that is required to derive accurate, high-resolution three-dimensional conductivity estimates of the subsurface.
Journal ArticleDOI
GASP I: Gas stripping phenomena in galaxies with MUSE
Bianca M. Poggianti,Alessia Moretti,Marco Gullieuszik,Jacopo Fritz,Yara L. Jaffé,Daniela Bettoni,Giovanni Fasano,Callum Bellhouse,Callum Bellhouse,George K. T. Hau,Benedetta Vulcani,Benedetta Vulcani,Andrea Biviano,Alessandro Omizzolo,Angela Paccagnella,Angela Paccagnella,Mauro D'Onofrio,Antonio Cava,Yun-Kyeong Sheen,Warrick J. Couch,Matt S. Owers,Matt S. Owers +21 more
TL;DR: GASP (GAs Stripping Phenomena in galaxies with MUSE) as mentioned in this paper is a new integral field spectroscopic survey at the VLT aiming at studying gas removal processes in galaxies.
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The SAMI Galaxy Survey: Revisiting Galaxy Classification Through High-Order Stellar Kinematics
Jesse van de Sande,Joss Bland-Hawthorn,Lisa Fogarty,Luca Cortese,Francesco D'Eugenio,Scott M. Croom,Nicholas Scott,James T. Allen,Sarah Brough,Julia J. Bryant,Gerald Cecil,Matthew Colless,Warrick J. Couch,Roger L. Davies,Pascal J. Elahi,Caroline Foster,Greg Goldstein,Michael Goodwin,Brent Groves,I-Ting Ho,Hyunjin Jeong,D. Heath Jones,I. S. Konstantopoulos,Jon Lawrence,Sarah K. Leslie,Angel R. Lopez-Sanchez,Richard M. McDermid,Rebecca McElroy,Anne M. Medling,Sree Oh,Matt S. Owers,Samuel N. Richards,Adam L. Schaefer,Rob Sharp,Sarah M. Sweet,Dan S. Taranu,Chiara Tonini,C. Jakob Walcher,Sukyoung K. Yi +38 more
TL;DR: In this article, the authors measured the stellar kinematics on a sample of 315 galaxies, without a morphological selection, using 2D integral field data from the SAMI Galaxy Survey.
Journal ArticleDOI
Galaxy And Mass Assembly: evolution of the Hα luminosity function and star formation rate density up to z < 0.35
Madusha Gunawardhana,Madusha Gunawardhana,Andrew M. Hopkins,Jonathan Bland-Hawthorn,Sarah Brough,Rob Sharp,Jonathan Loveday,Edward N. Taylor,Edward N. Taylor,David Heath Jones,Maritza A. Lara-López,Amanda E. Bauer,Matthew Colless,Matthew Colless,Matt S. Owers,Ivan K. Baldry,Angel R. Lopez-Sanchez,Caroline Foster,Steven P. Bamford,Michael J. I. Brown,Simon P. Driver,Michael J. Drinkwater,Jochen Liske,Martin Meyer,Peder Norberg,Aaron S. G. Robotham,J. H. Y. Ching,Michelle E. Cluver,Scott M. Croom,Lee S. Kelvin,Lee S. Kelvin,Matthew Prescott,Oliver Steele,Daniel Thomas,Lingyu Wang +34 more
TL;DR: In this paper, it was shown that the decrease in Phi at bright luminosities is best described by a Saunders functional form rather than the traditional Schechter function, which is consistent with other published luminosity functions in the far-infrared and radio.