Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence
External Organisations Sydney Institute for Astronomy; University of Sydney; ARC Centre of Excellence for All-sky Astrophysics; The University of Western Australia; ARC Centre of Excellence for Astrophysics in Three Dimensions (ASTRO3D); Curtin University; Sydney Inst Astron SIfA; Western Sydney Uni...
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ftands:oai:ands.org.au::1682070 2024-10-06T13:52:31+00:00 Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence Barbara Catinella (Creator) Brent Groves (Creator) Intl Centre for Radio Astronomy Research (ICRAR) (isManagedBy) Luca Cortese (Creator) https://researchdata.edu.au/data-from-the-drivers-turbulence/1682070 unknown The University of Western Australia University of Western Australia methods: data analysis methods: statistical techniques: imaging spectroscopy galaxies: disc Astrophysics - Astrophysics of Galaxies dataset ftands 2024-09-24T14:15:21Z External Organisations Sydney Institute for Astronomy; University of Sydney; ARC Centre of Excellence for All-sky Astrophysics; The University of Western Australia; ARC Centre of Excellence for Astrophysics in Three Dimensions (ASTRO3D); Curtin University; Sydney Inst Astron SIfA; Western Sydney University; University of New South Wales; ARC Australian Research Council; Swinburne University of Technology; Johns Hopkins University; Australian Astronomical Observatory; University of Cambridge; University of California Berkeley; Australian National University; Macquarie University; Australian Astronomical Optics; Christ University, Bangalore; NASA, National Aeronautics & Space Administration (NASA), Armstrong Flight Res Ctr, SOFIA Operat Ctr, USRA; NASA Armstrong Flight Research Center; NASA Ames Research Center; National Institute on Aging; SOFIA Science Center; University of Queensland; University of Oxford Associated Persons Mathew R Varidel (Creator); Scott M. Croom (Creator); Geraint F. Lewis (Creator); Deanne B. Fisher (Creator); Karl Glazebrook (Creator); Mark R Krumholz (Creator); Joss Bland-Hawthorn (Creator); Julia Bryant (Creator); Sarah Brough (Creator); Christoph Federrath (Creator); Jon S. Lawrence (Creator); Nuria P F Lorente (Creator); Matt S. Owers (Creator); Samuel N. Richards (Creator); Ángel R. López-Sánchez (Creator); Sarah M. Sweet (Creator); Jesse Van De Sande (Creator); Sam P. Vaughan (Creator) We infer the intrinsic ionized gas kinematics for 383 star-forming galaxies across a range of integrated star formation rates (SFR ∈ [10-3, 102] M☉ yr-1) at z ≲ 0.1 using a consistent 3D forward-modelling technique. The total sample is a combination of galaxies from the Sydney-AAO Multiobject Integral field Spectrograph (SAMI) Galaxy survey and DYnamics of Newly Assembled Massive Objects survey. For typical low-z galaxies taken from the SAMI Galaxy Survey, we find the vertical velocity dispersion (σV,z) to be positively correlated with measures of SFR, stellar mass, H I gas mass, and ... Dataset sami Research Data Australia (Australian National Data Service - ANDS) Queensland Bryant ENVELOPE(-60.942,-60.942,-71.236,-71.236) Mathew ENVELOPE(159.950,159.950,-81.683,-81.683) Sande ENVELOPE(7.527,7.527,62.631,62.631) |
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Open Polar |
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Research Data Australia (Australian National Data Service - ANDS) |
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unknown |
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methods: data analysis methods: statistical techniques: imaging spectroscopy galaxies: disc Astrophysics - Astrophysics of Galaxies |
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methods: data analysis methods: statistical techniques: imaging spectroscopy galaxies: disc Astrophysics - Astrophysics of Galaxies Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
topic_facet |
methods: data analysis methods: statistical techniques: imaging spectroscopy galaxies: disc Astrophysics - Astrophysics of Galaxies |
description |
External Organisations Sydney Institute for Astronomy; University of Sydney; ARC Centre of Excellence for All-sky Astrophysics; The University of Western Australia; ARC Centre of Excellence for Astrophysics in Three Dimensions (ASTRO3D); Curtin University; Sydney Inst Astron SIfA; Western Sydney University; University of New South Wales; ARC Australian Research Council; Swinburne University of Technology; Johns Hopkins University; Australian Astronomical Observatory; University of Cambridge; University of California Berkeley; Australian National University; Macquarie University; Australian Astronomical Optics; Christ University, Bangalore; NASA, National Aeronautics & Space Administration (NASA), Armstrong Flight Res Ctr, SOFIA Operat Ctr, USRA; NASA Armstrong Flight Research Center; NASA Ames Research Center; National Institute on Aging; SOFIA Science Center; University of Queensland; University of Oxford Associated Persons Mathew R Varidel (Creator); Scott M. Croom (Creator); Geraint F. Lewis (Creator); Deanne B. Fisher (Creator); Karl Glazebrook (Creator); Mark R Krumholz (Creator); Joss Bland-Hawthorn (Creator); Julia Bryant (Creator); Sarah Brough (Creator); Christoph Federrath (Creator); Jon S. Lawrence (Creator); Nuria P F Lorente (Creator); Matt S. Owers (Creator); Samuel N. Richards (Creator); Ángel R. López-Sánchez (Creator); Sarah M. Sweet (Creator); Jesse Van De Sande (Creator); Sam P. Vaughan (Creator) We infer the intrinsic ionized gas kinematics for 383 star-forming galaxies across a range of integrated star formation rates (SFR ∈ [10-3, 102] M☉ yr-1) at z ≲ 0.1 using a consistent 3D forward-modelling technique. The total sample is a combination of galaxies from the Sydney-AAO Multiobject Integral field Spectrograph (SAMI) Galaxy survey and DYnamics of Newly Assembled Massive Objects survey. For typical low-z galaxies taken from the SAMI Galaxy Survey, we find the vertical velocity dispersion (σV,z) to be positively correlated with measures of SFR, stellar mass, H I gas mass, and ... |
author2 |
Barbara Catinella (Creator) Brent Groves (Creator) Intl Centre for Radio Astronomy Research (ICRAR) (isManagedBy) Luca Cortese (Creator) |
format |
Dataset |
title |
Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
title_short |
Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
title_full |
Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
title_fullStr |
Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
title_full_unstemmed |
Data from: The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
title_sort |
data from: the sami galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence |
publisher |
The University of Western Australia |
url |
https://researchdata.edu.au/data-from-the-drivers-turbulence/1682070 |
long_lat |
ENVELOPE(-60.942,-60.942,-71.236,-71.236) ENVELOPE(159.950,159.950,-81.683,-81.683) ENVELOPE(7.527,7.527,62.631,62.631) |
geographic |
Queensland Bryant Mathew Sande |
geographic_facet |
Queensland Bryant Mathew Sande |
genre |
sami |
genre_facet |
sami |
op_source |
University of Western Australia |
_version_ |
1812180915839827968 |