The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

C. Foster; J. T. Mendel; C. D. P. Lagos; E. Wisnioski; T. Yuan; F. D'Eugenio; T. M. Barone; K. E. Harborne; S. P. Vaughan; F. Schulze; R. -S. Remus; A. Gupta; F. Collacchioni; D. J. Khim; P. Taylor; R. Bassett; S. M. Croom; R. M. McDermid; A. Poci; A. J. Battisti; J. Bland-Hawthorn; S. Bellstedt; M. Colless; L. J. M. Davies; C. Derkenne; S. Driver; A. Ferré-Mateu; D. B. Fisher; E. Gjergo; E. J. Johnston; A. Khalid; C. Kobayashi; S. Oh; Y. Peng; A. S. G. Robotham; P. Sharda; S. M. Sweet; E. N. Taylor; K. -V. H. Tran; J. W. Trayford; J. van de Sande; S. K. Yi; L. Zanisi

doi:10.1017/pasa.2021.25

The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

C. Foster
, J. T. Mendel
, C. D. P. Lagos
, E. Wisnioski
, T. Yuan
, F. D'Eugenio
, T. M. Barone
, K. E. Harborne
, S. P. Vaughan
, F. Schulze
, R. -S. Remus
, A. Gupta
, F. Collacchioni
, D. J. Khim
, P. Taylor
, R. Bassett
, S. M. Croom
, R. M. McDermid
, A. Poci
, A. J. Battisti

J. Bland-Hawthorn, S. Bellstedt, M. Colless, L. J. M. Davies, C. Derkenne, S. Driver, A. Ferré-Mateu, D. B. Fisher, E. Gjergo, E. J. Johnston, A. Khalid, C. Kobayashi, S. Oh, Y. Peng, A. S. G. Robotham, P. Sharda, S. M. Sweet, E. N. Taylor, K. -V. H. Tran, J. W. Trayford, J. van de Sande, S. K. Yi, L. Zanisi

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Abstract

We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during which the dynamical, morphological, and chemical properties of galaxies are predicted to evolve significantly. The survey uses new medium-deep adaptive optics aided MUSE observations of fields selected from the GAMA survey, providing a wealth of publicly available ancillary multi-wavelength data. With these data, MAGPI will map the kinematic and chemical properties of stars and ionised gas for a sample of 60 massive (> 7 x 10^10 M_Sun) central galaxies at 0.25 < z

Original language	English
Article number	e031
Number of pages	31
Journal	Publications of the Astronomical Society of Australia
Volume	38
DOIs	https://doi.org/10.1017/pasa.2021.25
Publication status	Published - 26 Jul 2021

Keywords

astro-ph.GA

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© The Author(s), 2021. Published by Cambridge University Press on behalf of the Astronomical Society of Australia. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1017/pasa.2021.25
Accepted author manuscript, 10.7 MBLicence: CC BY-NC-ND

Cite this

Foster, C., Mendel, J. T., Lagos, C. D. P., Wisnioski, E., Yuan, T., D'Eugenio, F., Barone, T. M., Harborne, K. E., Vaughan, S. P., Schulze, F., Remus, R. .-S., Gupta, A., Collacchioni, F., Khim, D. J., Taylor, P., Bassett, R., Croom, S. M., McDermid, R. M., Poci, A., ... Zanisi, L. (2021). The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework. Publications of the Astronomical Society of Australia, 38, Article e031. https://doi.org/10.1017/pasa.2021.25

@article{5baadc234e48452a98beed1aaf46f2d1,

title = "The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework",

abstract = " We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during which the dynamical, morphological, and chemical properties of galaxies are predicted to evolve significantly. The survey uses new medium-deep adaptive optics aided MUSE observations of fields selected from the GAMA survey, providing a wealth of publicly available ancillary multi-wavelength data. With these data, MAGPI will map the kinematic and chemical properties of stars and ionised gas for a sample of 60 massive (> 7 x 10\textasciicircum{}10 M\_Sun) central galaxies at 0.25 < z ",

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author = "C. Foster and Mendel, \{J. T.\} and Lagos, \{C. D. P.\} and E. Wisnioski and T. Yuan and F. D'Eugenio and Barone, \{T. M.\} and Harborne, \{K. E.\} and Vaughan, \{S. P.\} and F. Schulze and Remus, \{R. -S.\} and A. Gupta and F. Collacchioni and Khim, \{D. J.\} and P. Taylor and R. Bassett and Croom, \{S. M.\} and McDermid, \{R. M.\} and A. Poci and Battisti, \{A. J.\} and J. Bland-Hawthorn and S. Bellstedt and M. Colless and Davies, \{L. J. M.\} and C. Derkenne and S. Driver and A. Ferr{\'e}-Mateu and Fisher, \{D. B.\} and E. Gjergo and Johnston, \{E. J.\} and A. Khalid and C. Kobayashi and S. Oh and Y. Peng and Robotham, \{A. S. G.\} and P. Sharda and Sweet, \{S. M.\} and Taylor, \{E. N.\} and Tran, \{K. -V. H.\} and Trayford, \{J. W.\} and Sande, \{J. van de\} and Yi, \{S. K.\} and L. Zanisi",

note = "{\textcopyright} The Author(s), 2021. Published by Cambridge University Press on behalf of the Astronomical Society of Australia. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1017/pasa.2021.25",

year = "2021",

month = jul,

day = "26",

doi = "10.1017/pasa.2021.25",

language = "English",

volume = "38",

journal = "Publications of the Astronomical Society of Australia",

issn = "1323-3580",

publisher = "Cambridge University Press",

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Foster, C, Mendel, JT, Lagos, CDP, Wisnioski, E, Yuan, T, D'Eugenio, F, Barone, TM, Harborne, KE, Vaughan, SP, Schulze, F, Remus, R-S, Gupta, A, Collacchioni, F, Khim, DJ, Taylor, P, Bassett, R, Croom, SM, McDermid, RM, Poci, A, Battisti, AJ, Bland-Hawthorn, J, Bellstedt, S, Colless, M, Davies, LJM, Derkenne, C, Driver, S, Ferré-Mateu, A, Fisher, DB, Gjergo, E, Johnston, EJ, Khalid, A, Kobayashi, C, Oh, S, Peng, Y, Robotham, ASG, Sharda, P, Sweet, SM, Taylor, EN, Tran, K-VH, Trayford, JW, Sande, JVD, Yi, SK & Zanisi, L 2021, 'The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework', Publications of the Astronomical Society of Australia, vol. 38, e031. https://doi.org/10.1017/pasa.2021.25

TY - JOUR

T1 - The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

AU - Foster, C.

AU - Mendel, J. T.

AU - Lagos, C. D. P.

AU - Wisnioski, E.

AU - Yuan, T.

AU - D'Eugenio, F.

AU - Barone, T. M.

AU - Harborne, K. E.

AU - Vaughan, S. P.

AU - Schulze, F.

AU - Remus, R. -S.

AU - Gupta, A.

AU - Collacchioni, F.

AU - Khim, D. J.

AU - Taylor, P.

AU - Bassett, R.

AU - Croom, S. M.

AU - McDermid, R. M.

AU - Poci, A.

AU - Battisti, A. J.

AU - Bland-Hawthorn, J.

AU - Bellstedt, S.

AU - Colless, M.

AU - Davies, L. J. M.

AU - Derkenne, C.

AU - Driver, S.

AU - Ferré-Mateu, A.

AU - Fisher, D. B.

AU - Gjergo, E.

AU - Johnston, E. J.

AU - Khalid, A.

AU - Kobayashi, C.

AU - Oh, S.

AU - Peng, Y.

AU - Robotham, A. S. G.

AU - Sharda, P.

AU - Sweet, S. M.

AU - Taylor, E. N.

AU - Tran, K. -V. H.

AU - Trayford, J. W.

AU - Sande, J. van de

AU - Yi, S. K.

AU - Zanisi, L.

N1 - © The Author(s), 2021. Published by Cambridge University Press on behalf of the Astronomical Society of Australia. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1017/pasa.2021.25

PY - 2021/7/26

Y1 - 2021/7/26

N2 - We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during which the dynamical, morphological, and chemical properties of galaxies are predicted to evolve significantly. The survey uses new medium-deep adaptive optics aided MUSE observations of fields selected from the GAMA survey, providing a wealth of publicly available ancillary multi-wavelength data. With these data, MAGPI will map the kinematic and chemical properties of stars and ionised gas for a sample of 60 massive (> 7 x 10^10 M_Sun) central galaxies at 0.25 < z

AB - We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during which the dynamical, morphological, and chemical properties of galaxies are predicted to evolve significantly. The survey uses new medium-deep adaptive optics aided MUSE observations of fields selected from the GAMA survey, providing a wealth of publicly available ancillary multi-wavelength data. With these data, MAGPI will map the kinematic and chemical properties of stars and ionised gas for a sample of 60 massive (> 7 x 10^10 M_Sun) central galaxies at 0.25 < z

KW - astro-ph.GA

U2 - 10.1017/pasa.2021.25

DO - 10.1017/pasa.2021.25

M3 - Article

SN - 1323-3580

VL - 38

JO - Publications of the Astronomical Society of Australia

JF - Publications of the Astronomical Society of Australia

M1 - e031

ER -

The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

Abstract

Keywords

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