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; J. 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:10.48550/arxiv.2101.12224

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, J. 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

Australian Astronomical Optics

Research output: Working paper › Preprint

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 (370-570nm) 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.

Original language	English
Number of pages	27
DOIs	https://doi.org/10.48550/arxiv.2101.12224
Publication status	Published - 2021

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Name	arXiv

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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. (arXiv). https://doi.org/10.48550/arxiv.2101.12224

@techreport{b48fc63a8dad4b1a9762658bfa2b43e6,

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 (370-570nm) 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. ",

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{\textquoteright}Eugenio and Joss Bland-Hawthorn and J. 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",

doi = "10.48550/arxiv.2101.12224",

language = "English",

series = "arXiv",

type = "WorkingPaper",

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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' arXiv. https://doi.org/10.48550/arxiv.2101.12224

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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, J.

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

Y1 - 2021

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 (370-570nm) 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.

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 (370-570nm) 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.

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DO - 10.48550/arxiv.2101.12224

M3 - Preprint

T3 - arXiv

BT - The SAMI Galaxy Survey

ER -

The SAMI Galaxy Survey: the third and final data release

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