The SAMI galaxy survey: instrument specification and target selection

J. J. Bryant, M. S. Owers, A. S. G. Robotham, S. M. Croom, S. P. Driver, M. J. Drinkwater, N. P F Lorente, L. Cortese, N. Scott, M. Colless, A. Schaefer, E. N. Taylor, I. S. Konstantopoulos, J. T. Allen, I. Baldry, L. Barnes, A. E. Bauer, J. Bland-Hawthorn, J. V. Bloom, A. M. Brooks & 38 others S. Brough, G. Cecil, W. Couch, D. Croton, R. Davies, S. Ellis, L. M R Fogarty, C. Foster, K. Glazebrook, M. Goodwin, A. Green, M. L. Gunawardhana, E. Hampton, I. T. Ho, A. M. Hopkins, L. Kewley, J. S. Lawrence, S. G. Leon-Saval, S. Leslie, R. McElroy, G. Lewis, J. Liske, R. López-Sánchez, S. Mahajan, A. M. Medling, N. Metcalfe, M. Meyer, J. Mould, D. Obreschkow, S. O'Toole, M. Pracy, S. N. Richards, T. Shanks, R. Sharp, S. M. Sweet, A. D. Thomas, C. Tonini, C. J. Walcher

Research output: Contribution to journalArticleResearchpeer-review

Abstract

The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey which began in 2013. We present the throughput of the SAMI system, the science basis and specifications for the target selection, the survey observation plan and the combined properties of the selected galaxies. The survey includes four volume-limited galaxy samples based on cuts in a proxy for stellar mass, along with low-stellar-mass dwarf galaxies all selected from the Galaxy And Mass Assembly (GAMA) survey. The GAMA regions were selected because of the vast array of ancillary data available, including ultraviolet through to radio bands. These fields are on the celestial equator at 9, 12 and 14.5 h, and cover a total of 144 deg2 (in GAMA-I). Higher density environments are also included with the addition of eight clusters. The clusters have spectroscopy from 2-degree Field Galaxy Redshift Survey (2dFGRS) and Sloan Digital Sky Survey (SDSS) and photometry in regions covered by the SDSS and/or VLT Survey Telescope/ATLAS. The aim is to cover a broad range in stellar mass and environment, and therefore the primary survey targets cover redshifts 0.004<z<0.095, magnitudes rpet <19.4, stellar masses 107-1012 M⊙, and environments from isolated field galaxies through groups to clusters of ~1015 M⊙.

LanguageEnglish
Pages2857-2879
Number of pages23
JournalMonthly Notices of the Royal Astronomical Society
Volume447
Issue number3
DOIs
Publication statusPublished - 2015

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spectrographs
specifications
galaxies
stellar mass
assembly
telescopes
galactic clusters
dwarf galaxies
equators
photometry
spectroscopy
radio

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Bryant, J. J., Owers, M. S., Robotham, A. S. G., Croom, S. M., Driver, S. P., Drinkwater, M. J., ... Walcher, C. J. (2015). The SAMI galaxy survey: instrument specification and target selection. Monthly Notices of the Royal Astronomical Society, 447(3), 2857-2879. https://doi.org/10.1093/mnras/stu2635
Bryant, J. J. ; Owers, M. S. ; Robotham, A. S. G. ; Croom, S. M. ; Driver, S. P. ; Drinkwater, M. J. ; Lorente, N. P F ; Cortese, L. ; Scott, N. ; Colless, M. ; Schaefer, A. ; Taylor, E. N. ; Konstantopoulos, I. S. ; Allen, J. T. ; Baldry, I. ; Barnes, L. ; Bauer, A. E. ; Bland-Hawthorn, J. ; Bloom, J. V. ; Brooks, A. M. ; Brough, S. ; Cecil, G. ; Couch, W. ; Croton, D. ; Davies, R. ; Ellis, S. ; Fogarty, L. M R ; Foster, C. ; Glazebrook, K. ; Goodwin, M. ; Green, A. ; Gunawardhana, M. L. ; Hampton, E. ; Ho, I. T. ; Hopkins, A. M. ; Kewley, L. ; Lawrence, J. S. ; Leon-Saval, S. G. ; Leslie, S. ; McElroy, R. ; Lewis, G. ; Liske, J. ; López-Sánchez, R. ; Mahajan, S. ; Medling, A. M. ; Metcalfe, N. ; Meyer, M. ; Mould, J. ; Obreschkow, D. ; O'Toole, S. ; Pracy, M. ; Richards, S. N. ; Shanks, T. ; Sharp, R. ; Sweet, S. M. ; Thomas, A. D. ; Tonini, C. ; Walcher, C. J. / The SAMI galaxy survey : instrument specification and target selection. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 447, No. 3. pp. 2857-2879.
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Bryant, JJ, Owers, MS, Robotham, ASG, Croom, SM, Driver, SP, Drinkwater, MJ, Lorente, NPF, Cortese, L, Scott, N, Colless, M, Schaefer, A, Taylor, EN, Konstantopoulos, IS, Allen, JT, Baldry, I, Barnes, L, Bauer, AE, Bland-Hawthorn, J, Bloom, JV, Brooks, AM, Brough, S, Cecil, G, Couch, W, Croton, D, Davies, R, Ellis, S, Fogarty, LMR, Foster, C, Glazebrook, K, Goodwin, M, Green, A, Gunawardhana, ML, Hampton, E, Ho, IT, Hopkins, AM, Kewley, L, Lawrence, JS, Leon-Saval, SG, Leslie, S, McElroy, R, Lewis, G, Liske, J, López-Sánchez, R, Mahajan, S, Medling, AM, Metcalfe, N, Meyer, M, Mould, J, Obreschkow, D, O'Toole, S, Pracy, M, Richards, SN, Shanks, T, Sharp, R, Sweet, SM, Thomas, AD, Tonini, C & Walcher, CJ 2015, 'The SAMI galaxy survey: instrument specification and target selection' Monthly Notices of the Royal Astronomical Society, vol. 447, no. 3, pp. 2857-2879. https://doi.org/10.1093/mnras/stu2635

The SAMI galaxy survey : instrument specification and target selection. / Bryant, J. J.; Owers, M. S.; Robotham, A. S. G.; Croom, S. M.; Driver, S. P.; Drinkwater, M. J.; Lorente, N. P F; Cortese, L.; Scott, N.; Colless, M.; Schaefer, A.; Taylor, E. N.; Konstantopoulos, I. S.; Allen, J. T.; Baldry, I.; Barnes, L.; Bauer, A. E.; Bland-Hawthorn, J.; Bloom, J. V.; Brooks, A. M.; Brough, S.; Cecil, G.; Couch, W.; Croton, D.; Davies, R.; Ellis, S.; Fogarty, L. M R; Foster, C.; Glazebrook, K.; Goodwin, M.; Green, A.; Gunawardhana, M. L.; Hampton, E.; Ho, I. T.; Hopkins, A. M.; Kewley, L.; Lawrence, J. S.; Leon-Saval, S. G.; Leslie, S.; McElroy, R.; Lewis, G.; Liske, J.; López-Sánchez, R.; Mahajan, S.; Medling, A. M.; Metcalfe, N.; Meyer, M.; Mould, J.; Obreschkow, D.; O'Toole, S.; Pracy, M.; Richards, S. N.; Shanks, T.; Sharp, R.; Sweet, S. M.; Thomas, A. D.; Tonini, C.; Walcher, C. J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 447, No. 3, 2015, p. 2857-2879.

Research output: Contribution to journalArticleResearchpeer-review

TY - JOUR

T1 - The SAMI galaxy survey

T2 - Monthly Notices of the Royal Astronomical Society

AU - Bryant,J. J.

AU - Owers,M. S.

AU - Robotham,A. S. G.

AU - Croom,S. M.

AU - Driver,S. P.

AU - Drinkwater,M. J.

AU - Lorente,N. P F

AU - Cortese,L.

AU - Scott,N.

AU - Colless,M.

AU - Schaefer,A.

AU - Taylor,E. N.

AU - Konstantopoulos,I. S.

AU - Allen,J. T.

AU - Baldry,I.

AU - Barnes,L.

AU - Bauer,A. E.

AU - Bland-Hawthorn,J.

AU - Bloom,J. V.

AU - Brooks,A. M.

AU - Brough,S.

AU - Cecil,G.

AU - Couch,W.

AU - Croton,D.

AU - Davies,R.

AU - Ellis,S.

AU - Fogarty,L. M R

AU - Foster,C.

AU - Glazebrook,K.

AU - Goodwin,M.

AU - Green,A.

AU - Gunawardhana,M. L.

AU - Hampton,E.

AU - Ho,I. T.

AU - Hopkins,A. M.

AU - Kewley,L.

AU - Lawrence,J. S.

AU - Leon-Saval,S. G.

AU - Leslie,S.

AU - McElroy,R.

AU - Lewis,G.

AU - Liske,J.

AU - López-Sánchez,R.

AU - Mahajan,S.

AU - Medling,A. M.

AU - Metcalfe,N.

AU - Meyer,M.

AU - Mould,J.

AU - Obreschkow,D.

AU - O'Toole,S.

AU - Pracy,M.

AU - Richards,S. N.

AU - Shanks,T.

AU - Sharp,R.

AU - Sweet,S. M.

AU - Thomas,A. D.

AU - Tonini,C.

AU - Walcher,C. J.

PY - 2015

Y1 - 2015

N2 - The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey which began in 2013. We present the throughput of the SAMI system, the science basis and specifications for the target selection, the survey observation plan and the combined properties of the selected galaxies. The survey includes four volume-limited galaxy samples based on cuts in a proxy for stellar mass, along with low-stellar-mass dwarf galaxies all selected from the Galaxy And Mass Assembly (GAMA) survey. The GAMA regions were selected because of the vast array of ancillary data available, including ultraviolet through to radio bands. These fields are on the celestial equator at 9, 12 and 14.5 h, and cover a total of 144 deg2 (in GAMA-I). Higher density environments are also included with the addition of eight clusters. The clusters have spectroscopy from 2-degree Field Galaxy Redshift Survey (2dFGRS) and Sloan Digital Sky Survey (SDSS) and photometry in regions covered by the SDSS and/or VLT Survey Telescope/ATLAS. The aim is to cover a broad range in stellar mass and environment, and therefore the primary survey targets cover redshifts 0.004pet <19.4, stellar masses 107-1012 M⊙, and environments from isolated field galaxies through groups to clusters of ~1015 M⊙.

AB - The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey which began in 2013. We present the throughput of the SAMI system, the science basis and specifications for the target selection, the survey observation plan and the combined properties of the selected galaxies. The survey includes four volume-limited galaxy samples based on cuts in a proxy for stellar mass, along with low-stellar-mass dwarf galaxies all selected from the Galaxy And Mass Assembly (GAMA) survey. The GAMA regions were selected because of the vast array of ancillary data available, including ultraviolet through to radio bands. These fields are on the celestial equator at 9, 12 and 14.5 h, and cover a total of 144 deg2 (in GAMA-I). Higher density environments are also included with the addition of eight clusters. The clusters have spectroscopy from 2-degree Field Galaxy Redshift Survey (2dFGRS) and Sloan Digital Sky Survey (SDSS) and photometry in regions covered by the SDSS and/or VLT Survey Telescope/ATLAS. The aim is to cover a broad range in stellar mass and environment, and therefore the primary survey targets cover redshifts 0.004pet <19.4, stellar masses 107-1012 M⊙, and environments from isolated field galaxies through groups to clusters of ~1015 M⊙.

UR - http://www.scopus.com/inward/record.url?scp=84928550134&partnerID=8YFLogxK

U2 - 10.1093/mnras/stu2635

DO - 10.1093/mnras/stu2635

M3 - Article

VL - 447

SP - 2857

EP - 2879

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -