The SAMI Galaxy Survey: the third and final data release

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 (DR3), we release data for...

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Veröffentlicht in:arXiv.org 2021-01
Hauptverfasser: Croom, Scott M, Owers, Matt S, Scott, Nicholas, Poetrodjojo, Henry, Groves, Brent, van de Sande, Jesse, Barone, Tania M, Cortese, Luca, D'Eugenio, Francesco, Bland-Hawthorn, Joss, Bryant, Julia, Oh, Sree, Brough, Sarah, Agostino, James, Casura, Sarah, Catinella, Barbara, Colless, Matthew, Cecil, Gerald, Davies, Roger L, Drinkwater, Michael J, Driver, Simon P, Ferreras, Ignacio, Foster, Caroline, Fraser-McKelvie, Amelia, Lawrence, Jon, Leslie, Sarah K, Liske, Jochen, López-Sánchez, Ángel R, Lorente, Nuria P F, McElroy, Rebecca, Medling, Anne M, Obreschkow, Danail, Richards, Samuel N, Sharp, Rob, Sweet, Sarah M, Taranu, Dan S, Taylor, Edward N, Tescari, Edoardo, Thomas, Adam D, Tocknell, James, Vaughan, Sam P
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container_title arXiv.org
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creator Croom, Scott M
Owers, Matt S
Scott, Nicholas
Poetrodjojo, Henry
Groves, Brent
van de Sande, Jesse
Barone, Tania M
Cortese, Luca
D'Eugenio, Francesco
Bland-Hawthorn, Joss
Bryant, Julia
Oh, Sree
Brough, Sarah
Agostino, James
Casura, Sarah
Catinella, Barbara
Colless, Matthew
Cecil, Gerald
Davies, Roger L
Drinkwater, Michael J
Driver, Simon P
Ferreras, Ignacio
Foster, Caroline
Fraser-McKelvie, Amelia
Lawrence, Jon
Leslie, Sarah K
Liske, Jochen
López-Sánchez, Ángel R
Lorente, Nuria P F
McElroy, Rebecca
Medling, Anne M
Obreschkow, Danail
Richards, Samuel N
Sharp, Rob
Sweet, Sarah M
Taranu, Dan S
Taylor, Edward N
Tescari, Edoardo
Thomas, Adam D
Tocknell, James
Vaughan, Sam P
description 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 (DR3), 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 parameterized 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 (AAO) Data Central.
doi_str_mv 10.48550/arxiv.2101.12224
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subjects Celestial bodies
Cubes
Galactic clusters
Galaxies
Gas ionization
Kinematics
Large scale structure of the universe
Line spectra
Physics - Astrophysics of Galaxies
Resolution
Stars & galaxies
Stellar kinematics
title The SAMI Galaxy Survey: the third and final data release
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