E
Elaine M. Sadler
Researcher at University of Sydney
Publications - 379
Citations - 27208
Elaine M. Sadler is an academic researcher from University of Sydney. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 74, co-authored 368 publications receiving 24757 citations. Previous affiliations of Elaine M. Sadler include Spanish National Research Council & National Science Foundation.
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Journal ArticleDOI
The RASS–6dFGS catalogue: a sample of X-ray selected AGN from the 6dF Galaxy Survey
TL;DR: In this article, the authors presented a catalogue of 3405 X-ray sources from the ROSAT All Sky Survey (RASS) Bright Source Catalogue which fall within the area covered by the 6dF Galaxy Survey (6dFGS).
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The challenges of low-frequency radio polarimetry: lessons from the Murchison Widefield Array
Emil Lenc,C. S. Anderson,Nichole Barry,Judd D. Bowman,Iver H. Cairns,Jamie Farnes,Bryan Gaensler,George Heald,Melanie Johnston-Hollitt,David L. Kaplan,Christene Lynch,Patrick I. McCauley,Daniel A. Mitchell,John Morgan,Miguel F. Morales,Tara Murphy,A. R. Offringa,Stephen M. Ord,Bartosz Pindor,C. J. Riseley,Elaine M. Sadler,Charlotte Sobey,Marcin Sokolowski,Ian Sullivan,Shane O'Sullivan,Xiaohui Sun,S. E. Tremblay,Cathryn M. Trott,Randall B. Wayth +28 more
TL;DR: In this article, the Murchison Widefield Array (MWA) was used to calibrate and correct low frequency (72-300 MHz) radio observations for polarimetry.
Journal ArticleDOI
The fornax spectroscopic survey: the number of unresolved compact galaxies
Michael J. Drinkwater,Steven Phillipps,Michael D. Gregg,Quentin A. Parker,Rodney Smith,Jonathan Ivor Davies,J. Bryn Jones,Elaine M. Sadler +7 more
TL;DR: In this paper, the authors describe a sample of 13 bright (18.5 < BJ < 20.1), compact galaxies at low redshift (0.05 < z < 0.21) behind the Fornax Cluster.
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GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies
D. Wijesinghe,E. da Cunha,Andrew M. Hopkins,Loretta Dunne,Rob Sharp,Madusha Gunawardhana,Sarah Brough,Elaine M. Sadler,Simon P. Driver,Ivan K. Baldry,Steven P. Bamford,Jochen Liske,Jon Loveday,Peder Norberg,John A. Peacock,Cristina Popescu,Richard J. Tuffs,E. Andrae,Robbie Richard Auld,Maarten Baes,Joss Bland-Hawthorn,S. Buttiglione,Antonio Cava,Ewan Cameron,Christopher J. Conselice,Asantha Cooray,Scott M. Croom,Aliakbar Dariush,G. DeZotti,Simon Dye,Stephen Anthony Eales,Carlos S. Frenk,Jacopo Fritz,Denis Hill,R. Hopwood,Edo Ibar,Rob Ivison,Matt J. Jarvis,David Heath Jones,E. van Kampen,Lee S. Kelvin,Konrad Kuijken,Steve Maddox,Barry F. Madore,Michał J. Michałowski,B. Nichol,H Parkinson,Enzo Pascale,Kevin A. Pimbblet,Michael Pohlen,Matthew Prescott,G. Rhodighiero,Aaron S. G. Robotham,E. E. Rigby,Mark Seibert,S. Sergeant,Daniel J. Smith,Pasquale Temi,William J. Sutherland,Edward N. Taylor,Daniel Thomas,P. van der Werf +61 more
TL;DR: In this paper, the relationship between various dust obscuration measures in galaxies was explored using multi-wavelength data from the Galaxy And Mass Assembly (GAMA) and Herschel-ATLAS (H-ATlAS) surveys.
Journal ArticleDOI
Wide-field broad-band radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETA
Ian Heywood,Ian Heywood,Keith W. Bannister,J. Marvil,James R. Allison,L. Ball,Martin Bell,Douglas C.-J. Bock,John D. Bunton,Aaron Chippendale,F. Cooray,Tim J. Cornwell,D. de Boer,D. de Boer,Philip G. Edwards,R. G. Gough,N. Gupta,N. Gupta,Lisa Harvey-Smith,S. Hay,Aidan Hotan,Balthasar T. Indermuehle,C. Jacka,Chloe Jackson,Chloe Jackson,Simon Johnston,Amy Kimball,B. S. Koribalski,Emil Lenc,Emil Lenc,A. Macleod,Naomi McClure-Griffiths,Naomi McClure-Griffiths,David McConnell,P. Mirtschin,Tara Murphy,S. Neuhold,Ray P. Norris,Sarah Pearce,Attila Popping,Attila Popping,R. Y. Qiao,John Reynolds,Elaine M. Sadler,Robert J. Sault,Robert J. Sault,A. E. T. Schinckel,Paolo Serra,Timothy W. Shimwell,Timothy W. Shimwell,Jamie Stevens,J. Tuthill,Anastasios Tzioumis,Maxim Voronkov,Tobias Westmeier,Matthew Whiting +55 more
TL;DR: The first generation of ASKAP's phased array feed (PAF) receivers were used for wide-area imaging via the deployment of simultaneous multiple beams within a 30 square degree field of view.