Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 505, Issue 1, Pages 991-1016Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab229
Keywords
surveys; galaxies: clusters: general; galaxies: general; galaxies: kinematics and dynamics; galaxies: star formation; galaxies: stellar content
Categories
Funding
- Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) [CE170100013]
- Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO) [CE110001020]
- STFC (UK)
- ARC (Australia)
- AAO
- Australian Research Council [FT140100255, FT180100231, FT140101166]
- ERC [683184]
- Australian Research Council Discovery Early Career Research Award - Australian Government [DE200100461, DE190100375]
- Australian Government Research Training Program Scholarship
- Australian Research Council Future Fellowship - Australian Government [FT190100083, FT180100066]
- UK Science and Technology Facilities Council through the 'Astrophysics at Oxford' [ST/K00106X/1]
- Christ Church, Oxford
- Oxford Hintze Centre for Astrophysical Surveys - Hintze Family Charitable Foundation
- National Science Foundation [2009416]
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [2009416] Funding Source: National Science Foundation
- Australian Research Council [FT180100231] Funding Source: Australian Research Council
- European Research Council (ERC) [683184] Funding Source: European Research Council (ERC)
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The SAMI Galaxy Survey has released data for a total of 3068 unique galaxies, including 888 unique galaxies for the first time. Each galaxy has two primary spectral cubes covering the blue and red optical wavelength ranges, additional spatially binned spectral cubes, and standardized aperture spectra. 2D maps derived from parametrized fitting to the emission-line and absorption-line spectral data are also provided for each galaxy, offering insights into various physical properties.
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. Here, in Data Release 3, we release data for the full sample of 3068 unique galaxies observed. This includes the SAMI cluster sample of 888 unique galaxies for the first time. For each galaxy, there are two primary spectral cubes covering the blue (370-570nm) and red (630-740nm) optical wavelength ranges at spectral resolving power of R = 1808 and 4304, respectively. For each primary cube, we also provide three spatially binned spectral cubes and a set of standardized aperture spectra. For each galaxy, we include complete 2D maps from parametrized fitting to the emission-line and absorption-line spectral data. These maps provide information on the gas ionization and kinematics, stellar kinematics and populations, and more. All data are available online through Australian Astronomical Optics Data Central.
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