The SAMI Galaxy Survey: the third and final data release

Scott M. Croom; Matt S. Owers; Nicholas Scott; Henry Poetrodjojo; Brent Groves; Jesse van de Sande; Tania M. Barone; Luca Cortese; Francesco D'Eugenio; Joss Bland-Hawthorn; Julia Bryant; Sree Oh; Sarah Brough; James Agostino; Sarah Casura; Barbara Catinella; Matthew Colless; Gerald Cecil; Roger L. Davies; Michael J. Drinkwater; Simon P. Driver; Ignacio Ferreras; Caroline Foster; Amelia Fraser-McKelvie; Jon Lawrence; Sarah K. Leslie; Jochen Liske; Ángel R. López-Sánchez; Nuria P. F. Lorente; Rebecca McElroy; Anne M. Medling; Danail Obreschkow; Samuel N. Richards; Rob Sharp; Sarah M. Sweet; Dan S. Taranu; Edward N. Taylor; Edoardo Tescari; Adam D. Thomas; James Tocknell; Sam P. Vaughan

doi:10.1093/mnras/stab229

The SAMI Galaxy Survey: the third and final data release

Scott M. Croom, Matt S. Owers, Nicholas Scott, Henry Poetrodjojo, Brent Groves, Jesse van de Sande, Tania M. Barone, Luca Cortese, Francesco D'Eugenio, Joss Bland-Hawthorn, Julia Bryant, Sree Oh, Sarah Brough, James Agostino, Sarah Casura, Barbara Catinella, Matthew Colless, Gerald Cecil, Roger L. Davies, Michael J. DrinkwaterSimon P. Driver, Ignacio Ferreras, Caroline Foster, Amelia Fraser-McKelvie, Jon Lawrence, Sarah K. Leslie, Jochen Liske, Ángel R. López-Sánchez, Nuria P. F. Lorente, Rebecca McElroy, Anne M. Medling, Danail Obreschkow, Samuel N. Richards, Rob Sharp, Sarah M. Sweet, Dan S. Taranu, Edward N. Taylor, Edoardo Tescari, Adam D. Thomas, James Tocknell, Sam P. Vaughan

International Centre for Radio Astronomy Research (ICRAR)

Research output: Contribution to journal › Article › peer-review

90 Citations (Scopus)

Abstract

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 (370-570 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 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.

Original language	English
Pages (from-to)	991–1016
Number of pages	26
Journal	Monthly Notices of the Royal Astronomical Society
Volume	505
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stab229
Publication status	Published - 1 Jul 2021

Access to Document

10.1093/mnras/stab229

http://adsabs.harvard.edu/abs/2021MNRAS.tmp..291C

1 Finished
1 Active

The Enigma of Galactic Rotation
Obreschkow, D. (Investigator 01)
ARC Australian Research Council
2/12/19 → 1/12/26
Project: Research
Beyond Appearance: revealing the physics of galaxy transformation
Cortese, L. (Investigator 01)
ARC Australian Research Council
1/10/18 → 30/09/23
Project: Research

Cite this

Croom, S. M., Owers, M. S., Scott, N., Poetrodjojo, H., Groves, B., van de Sande, J., Barone, T. M., Cortese, L., D'Eugenio, F., Bland-Hawthorn, J., Bryant, J., Oh, S., Brough, S., Agostino, J., Casura, S., Catinella, B., Colless, M., Cecil, G., Davies, R. L., ... Vaughan, S. P. (2021). The SAMI Galaxy Survey: the third and final data release. Monthly Notices of the Royal Astronomical Society, 505(1), 991–1016. https://doi.org/10.1093/mnras/stab229

@article{48a4345fd1124b91828e5c4628b97847,

title = "The SAMI Galaxy Survey: the third and final data release",

abstract = "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 (370-570 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 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.",

keywords = "galaxies: general, galaxies: kinematics and dynamics, galaxies: star formation, galaxies: stellar content, galaxies: clusters: general, astronomical data bases: surveys",

author = "Croom, {Scott M.} and Owers, {Matt S.} and Nicholas Scott and Henry Poetrodjojo and Brent Groves and {van de Sande}, Jesse and Barone, {Tania M.} and Luca Cortese and Francesco D'Eugenio and Joss Bland-Hawthorn and Julia Bryant and Sree Oh and Sarah Brough and James Agostino and Sarah Casura and Barbara Catinella and Matthew Colless and Gerald Cecil and Davies, {Roger L.} and Drinkwater, {Michael J.} and Driver, {Simon P.} and Ignacio Ferreras and Caroline Foster and Amelia Fraser-McKelvie and Jon Lawrence and Leslie, {Sarah K.} and Jochen Liske and L{\'o}pez-S{\'a}nchez, {{\'A}ngel R.} and Lorente, {Nuria P. F.} and Rebecca McElroy and Medling, {Anne M.} and Danail Obreschkow and Richards, {Samuel N.} and Rob Sharp and Sweet, {Sarah M.} and Taranu, {Dan S.} and Taylor, {Edward N.} and Edoardo Tescari and Thomas, {Adam D.} and James Tocknell and Vaughan, {Sam P.}",

year = "2021",

month = jul,

day = "1",

doi = "10.1093/mnras/stab229",

language = "English",

volume = "505",

pages = "991–1016",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Croom, SM, Owers, MS, Scott, N, Poetrodjojo, H, Groves, B, van de Sande, J, Barone, TM, Cortese, L, D'Eugenio, F, Bland-Hawthorn, J, Bryant, J, Oh, S, Brough, S, Agostino, J, Casura, S, Catinella, B, Colless, M, Cecil, G, Davies, RL, Drinkwater, MJ, Driver, SP, Ferreras, I, Foster, C, Fraser-McKelvie, A, Lawrence, J, Leslie, SK, Liske, J, López-Sánchez, ÁR, Lorente, NPF, McElroy, R, Medling, AM, Obreschkow, D, Richards, SN, Sharp, R, Sweet, SM, Taranu, DS, Taylor, EN, Tescari, E, Thomas, AD, Tocknell, J & Vaughan, SP 2021, 'The SAMI Galaxy Survey: the third and final data release', Monthly Notices of the Royal Astronomical Society, vol. 505, no. 1, pp. 991–1016. https://doi.org/10.1093/mnras/stab229

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 (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 (370-570 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 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.

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 (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 (370-570 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 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.

KW - galaxies: general

KW - galaxies: kinematics and dynamics

KW - galaxies: star formation

KW - galaxies: stellar content

KW - galaxies: clusters: general

KW - astronomical data bases: surveys

U2 - 10.1093/mnras/stab229

DO - 10.1093/mnras/stab229

M3 - Article

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 -

The SAMI Galaxy Survey: the third and final data release

Abstract

Access to Document

Fingerprint

Projects

The Enigma of Galactic Rotation

Beyond Appearance: revealing the physics of galaxy transformation

Cite this