Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Dan S Taranu"'
Autor:
Sarah Casura, Jochen Liske, Aaron S G Robotham, Sarah Brough, Simon P Driver, Alister W Graham, Boris Häußler, Benne W Holwerda, Andrew M Hopkins, Lee S Kelvin, Amanda J Moffett, Dan S Taranu, Edward N Taylor
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:942-974
We derive single S\'ersic fits and bulge-disk decompositions for 13096 galaxies at redshifts z < 0.08 in the GAMA II equatorial survey regions in the Kilo-Degree Survey (KiDS) g, r and i bands. The surface brightness fitting is performed using the Ba
Autor:
John D. Silverman, Ivana Damjanov, Song Huang, Naoki Yasuda, Marcin Sawicki, Masayuki Tanaka, Lalitwadee Kawinwanichakij, Masato Onodera, Angelo George, Takatoshi Shibuya, Xuheng Ding, Simon Birrer, Junyao Li, Dan S. Taranu
We present the galaxy size-mass ($R_{e}-M_{\ast}$) distributions using a stellar-mass complete sample of $\sim1.5$ million galaxies, covering $\sim100$ deg$^2$, with $\log(M_{\ast}/M_{\odot})>10.2~(9.2)$ over the redshift range $0.2
Comment: Acc
Comment: Acc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3e4e32275d8af7f8c20dd37be5d563b
http://arxiv.org/abs/2109.09766
http://arxiv.org/abs/2109.09766
Autor:
Sree Oh, Gerald Cecil, Scott M. Croom, Edoardo Tescari, Adam D. Thomas, Jesse van de Sande, Rebecca McElroy, Dan S. Taranu, Jochen Liske, Luca Cortese, Danail Obreschkow, Julia J. Bryant, Barbara Catinella, Michael J. Drinkwater, James Tocknell, Angel R. Lopez-Sanchez, Amelia Fraser-McKelvie, Ignacio Ferreras, Francesco D'Eugenio, Sarah Brough, Samuel N. Richards, Sarah Casura, Tania M. Barone, Anne M. Medling, Henry Poetrodjojo, Sarah K. Leslie, Sam P. Vaughan, Edward N. Taylor, Roger L. Davies, James Agostino, Matt S. Owers, Rob Sharp, Jon Lawrence, Nuria P. F. Lorente, Nicholas Scott, Caroline Foster, Simon P. Driver, Joss Bland-Hawthorn, Matthew Colless, Sarah M. Sweet, Brent Groves
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 505(1), 991-1016
We have entered a new era where integral-field spectroscopic surveys of galaxies are sufficiently large to adequately sample large-scale structure over a cosmologically significant volume. This was the primary design goal of the SAMI Galaxy Survey. H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bf4c6b19bf2ae222f351c29020b5407
http://arxiv.org/abs/2101.12224
http://arxiv.org/abs/2101.12224
Autor:
Anne M. Medling, Nicholas Scott, Dan S. Taranu, Brent Groves, K. E. Harborne, A. Khalid, Sam P. Vaughan, Scott M. Croom, Michael Goodwin, Joss Bland-Hawthorn, Matt S. Owers, Samuel N. Richards, Luca Cortese, Claudia del P. Lagos, Caroline Foster, Jon Lawrence, J. van de Sande, Julia J. Bryant, Sarah Brough
We use comparisons between the SAMI Galaxy Survey and equilibrium galaxy models to infer the importance of disc fading in the transition of spirals into lenticular (S0) galaxies. The local S0 population has both higher photometric concentration and l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cefe134670da423ea2979fcb57fa2b42
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 483:249-262
A primary goal of integral field spectroscopic (IFS) surveys is to provide a statistical census of galaxies classified by their internal kinematics. As a result, the observational spin parameter, $\lambda_R$, has become one of the most popular method
Autor:
Tayyaba Zafar, Joss Bland-Hawthorn, Jon Lawrence, Matt S. Owers, Francesco D'Eugenio, Michael Goodwin, Angel R. Lopez-Sanchez, Caroline Foster, Sarah Brough, Richard M. McDermid, Nicholas Scott, Anne M. Medling, C. Tonini, Iraklis S. Konstantopoulos, Samuel N. Richards, Scott M. Croom, Dan S. Taranu, Luca Cortese, J. van de Sande, Julia J. Bryant
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 472:966-978
Using the stellar kinematic maps and ancillary imaging data from the Sydney AAO Multi Integral field (SAMI) Galaxy Survey, the intrinsic shape of kinematically-selected samples of galaxies is inferred. We implement an efficient and optimised algorith
Autor:
Sarah M. Sweet, Angel R. Lopez-Sanchez, Dan S. Taranu, Andrew M. Hopkins, Geraint F. Lewis, Matt S. Owers, Mathew R. Varidel, Jon Lawrence, Anne M. Medling, Michael Goodwin, Christoph Federrath, Scott M. Croom, Karl Glazebrook, Samuel N. Richards, Julia J. Bryant, Joss Bland-Hawthorn, Caroline Foster, Nicholas Scott, Brendon J. Brewer, Brent Groves, Jesse van de Sande, Enrico M. Di Teodoro, Richard Scalzo
We present a novel Bayesian method, referred to as Blobby3D, to infer gas kinematics that mitigates the effects of beam smearing for observations using Integral Field Spectroscopy (IFS). The method is robust for regularly rotating galaxies despite su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e143aa1b934c29bfda153f3404a94072
http://arxiv.org/abs/1903.03121
http://arxiv.org/abs/1903.03121
Autor:
Scott M. Croom, Michael J. Hudson, Kyle A. Oman, Joss Bland-Hawthorn, Warrick J. Couch, Julia J. Bryant, Sarah Brough, Matt S. Owers, Richard M. McDermid, Nicholas Scott, Nuria P. F. Lorente, Anne M. Medling, Sukyoung K. Yi, Luca Cortese, Charlotte Welker, Christoph Federrath, Dan S. Taranu, Andrew M. Hopkins, Samuel N. Richards, Jesse van de Sande, Brent Groves, Jon Lawrence
Publikováno v:
The Astrophysical Journal, 873(1):873-52. IOP PUBLISHING LTD
We use integral field spectroscopy from the SAMI Galaxy Survey to identify galaxies that show evidence for recent quenching of star formation. The galaxies exhibit strong Balmer absorption in the absence of ongoing star formation in more than 10% of
Autor:
Sarah Brough, Nicholas Scott, Claudia del P. Lagos, Matt S. Owers, Sree Oh, Samuel N. Richards, Matthew Colless, Dan S. Taranu, Angel R. Lopez-Sanchez, Scott M. Croom, Anne M. Medling, Jon Lawrence, Jesse van de Sande, Sarah M. Sweet, Caroline Foster, Joss Bland-Hawthorn, Alexander Rawlings, Iraklis S. Konstantopoulos, Nuria P. F. Lorente, Sukyoung K. Yi, Julia J. Bryant
We study the behaviour of the spin-ellipticity radial tracks for 507 galaxies from the Sydney AAO Multi-object Integral Field (SAMI) Galaxy Survey with stellar kinematics out to $\geq1.5R_\text{e}$. We advocate for a morpho-dynamical classification o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::167a384d765dd303c1088bc4e8b3a667
Autor:
Sarah Brough, Christoph Federrath, Samuel N. Richards, M. L. P. Gunawardhana, Simon P. Driver, Jon Lawrence, Mathew R. Varidel, Scott M. Croom, Francesco D'Eugenio, Henry Poetrodjojo, Matt S. Owers, Sarah M. Sweet, Andrew W. Green, Jesse van de Sande, Dan S. Taranu, Luca Cortese, Joss Bland-Hawthorn, Michael J. Drinkwater, Anne M. Medling, Katrina Sealey, Brent Groves, Sebastián F. Sánchez, Elizabeth Mannering, Sree Oh, Yifei Jin, Caroline Foster, Lloyd Harischandra, Simon J. O'Toole, Nicholas Scott, Dilyar Barat, Michael Goodwin, Rob Sharp, A. L. Schaefer, Nuria P. F. Lorente, Tania M. Barone, Matthew Colless, Julia J. Bryant
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 481(2), 2299-2319
Monthly Notices of the Royal Astronomical Society, 481(2), 2299-2319
We present the second major release of data from the SAMI Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50% of the full survey. Galaxies included have a redshift range 0.004 < z < 0.113 and a large stellar mass range 7.5 < lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab7bf445d43eafc7db56235c7a4c55f5
https://hdl.handle.net/10023/18682
https://hdl.handle.net/10023/18682