TY - JOUR
T1 - The SAMI Galaxy Survey
T2 - the third and final data release
AU - Croom, Scott M.
AU - Owers, Matt S.
AU - Scott, Nicholas
AU - Poetrodjojo, Henry
AU - Groves, Brent
AU - van de Sande, Jesse
AU - Barone, Tania M.
AU - Cortese, Luca
AU - D'Eugenio, Francesco
AU - Bland-Hawthorn, Joss
AU - Bryant, Julia
AU - Oh, Sree
AU - Brough, Sarah
AU - Agostino, James
AU - Casura, Sarah
AU - Catinella, Barbara
AU - Colless, Matthew
AU - Cecil, Gerald
AU - Davies, Roger L.
AU - Drinkwater, Michael J.
AU - Driver, Simon P.
AU - Ferreras, Ignacio
AU - Foster, Caroline
AU - Fraser-Mckelvie, Amelia
AU - Lawrence, Jon
AU - Leslie, Sarah K.
AU - Liske, Jochen
AU - López-Sánchez, Ángel R.
AU - Lorente, Nuria P.F.
AU - McElroy, Rebecca
AU - Medling, Anne M.
AU - Obreschkow, Danail
AU - Richards, Samuel N.
AU - Sharp, Rob
AU - Sweet, Sarah M.
AU - Taranu, Dan S.
AU - Taylor, Edward N.
AU - Tescari, Edoardo
AU - Thomas, Adam D.
AU - Tocknell, James
AU - Vaughan, Sam P.
PY - 2021/7/1
Y1 - 2021/7/1
N2 - 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 (370-570 nm) and red (630-740 nm) 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.
AB - 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 (370-570 nm) and red (630-740 nm) 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.
KW - Galaxies: clusters: general
KW - Galaxies: general
KW - Galaxies: kinematics and dynamics
KW - Galaxies: star formation
KW - Galaxies: stellar content
KW - Surveys
UR - http://www.scopus.com/inward/record.url?scp=85108177292&partnerID=8YFLogxK
UR - http://purl.org/au-research/grants/arc/FT140100255
U2 - 10.1093/mnras/stab229
DO - 10.1093/mnras/stab229
M3 - Article
AN - SCOPUS:85108177292
SN - 0035-8711
VL - 505
SP - 991
EP - 1016
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 1
ER -