The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework

Autores
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, Florencia; Khim, D. J.; Taylor, P.; Bassett, R.; Croom, S. M.; McDermid, R. M.; Poci, A.; Battisti, A. J.; Bland-Hawthorn, J.; Bellstedt, S.; Colless, M.; Davies, L. J. M.; Derkenne, C.; Driver, S.; Ferré-Mateu, A.; Fisher, D. B.; Gjergo, E.; Johnston, E. J.; Khalid, A.; Kobayashi, C.; Oh, S.; Peng, Y.; Robotham, A. S. G.; Sharda, P.; Sweet, S. M.; Taylor, E. N.; Tran, K. V. H.; Trayford, J. W.; van de Sande, J.; Yi, S. K.; Zanisi, L.
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on the European Southern Observatory Very Large Telescope. MAGPI is designed to study the physical drivers of galaxy transformation at a look-back 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 Multi-Unit Spectroscopic Explorer (MUSE) observations of fields selected from the Galaxy and Mass Assembly (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 1010 M⊙) central galaxies at 0.25 < z < 0.35 in a representative range of environments (isolated, groups and clusters). The spatial resolution delivered by MUSE with Ground Layer Adaptive Optics (0.6 − 0.8 arcsec FWHM) will facilitate a direct comparison with Integral Field Spectroscopy surveys of the nearby Universe, such as SAMI and MaNGA, and at higher redshifts using adaptive optics, for example, SINS. In addition to the primary (central) galaxy sample, MAGPI will deliver resolved and unresolved spectra for as many as 150 satellite galaxies at 0.25 < z < 0.35, as well as hundreds of emission-line sources at z < 6. This paper outlines the science goals, survey design, and observing strategy of MAGPI. We also present a first look at the MAGPI data, and the theoretical framework to which MAGPI data will be compared using the current generation of cosmological hydrodynamical simulations including EAGLE, MAGNETICUM, HORIZON-AGN, and ILLUSTRIS-TNG. Our results show that cosmological hydrodynamical simulations make discrepant predictions in the spatially resolved properties of galaxies at z ≈ 0.3. MAGPI observations will place new constraints and allow for tangible improvements in galaxy formation theory.
Fil: Foster, C.. The University Of Sydney; Australia
Fil: Mendel, J. T.. International Centre For Radio Astronomy Research; Australia
Fil: Lagos, C. D. P.. International Centre For Radio Astronomy Research; Australia
Fil: Wisnioski, E.. Australian National University; Australia
Fil: Yuan, T.. Swinburne University Of Technology; Australia
Fil: D'Eugenio, F.. International Centre For Radio Astronomy Research; Australia
Fil: Barone, T. M.. International Centre For Radio Astronomy Research; Australia
Fil: Harborne, K. E.. International Centre For Radio Astronomy Research; Australia
Fil: Vaughan, S. P.. International Centre For Radio Astronomy Research; Australia
Fil: Schulze, F.. International Centre For Radio Astronomy Research; Australia
Fil: Remus, R.-S.. International Centre For Radio Astronomy Research; Australia
Fil: Gupta, A.. International Centre For Radio Astronomy Research; Australia
Fil: Collacchioni, Florencia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Khim, D. J.. International Centre For Radio Astronomy Research; Australia
Fil: Taylor, P.. International Centre For Radio Astronomy Research; Australia
Fil: Bassett, R.. International Centre For Radio Astronomy Research; Australia
Fil: Croom, S. M.. International Centre For Radio Astronomy Research; Australia
Fil: McDermid, R. M.. International Centre For Radio Astronomy Research; Australia
Fil: Poci, A.. International Centre For Radio Astronomy Research; Australia
Fil: Battisti, A. J.. International Centre For Radio Astronomy Research; Australia
Fil: Bland-Hawthorn, J.. International Centre For Radio Astronomy Research; Australia
Fil: Bellstedt, S.. International Centre For Radio Astronomy Research; Australia
Fil: Colless, M.. International Centre For Radio Astronomy Research; Australia
Fil: Davies, L. J. M.. International Centre For Radio Astronomy Research; Australia
Fil: Derkenne, C.. International Centre For Radio Astronomy Research; Australia
Fil: Driver, S.. International Centre For Radio Astronomy Research; Australia
Fil: Ferré-Mateu, A.. International Centre For Radio Astronomy Research; Australia
Fil: Fisher, D. B.. International Centre For Radio Astronomy Research; Australia
Fil: Gjergo, E.. International Centre For Radio Astronomy Research; Australia
Fil: Johnston, E. J.. International Centre For Radio Astronomy Research; Australia
Fil: Khalid, A.. International Centre For Radio Astronomy Research; Australia
Fil: Kobayashi, C.. International Centre For Radio Astronomy Research; Australia
Fil: Oh, S.. International Centre For Radio Astronomy Research; Australia
Fil: Peng, Y.. International Centre For Radio Astronomy Research; Australia
Fil: Robotham, A. S. G.. International Centre For Radio Astronomy Research; Australia
Fil: Sharda, P.. International Centre For Radio Astronomy Research; Australia
Fil: Sweet, S. M.. International Centre For Radio Astronomy Research; Australia
Fil: Taylor, E. N.. International Centre For Radio Astronomy Research; Australia
Fil: Tran, K. V. H.. International Centre For Radio Astronomy Research; Australia
Fil: Trayford, J. W.. Leiden Observatory, Leiden University; Países Bajos
Fil: van de Sande, J.. International Centre For Radio Astronomy Research; Australia
Fil: Yi, S. K.. International Centre For Radio Astronomy Research; Australia
Fil: Zanisi, L.. International Centre For Radio Astronomy Research; Australia
Materia
SURVEYS
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STELLAR CONTENT
GALAXIES: STRUCTURE
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/169536
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/169536
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The MAGPI survey: science goals, design, observing strategy, early results and theoretical frameworkFoster, 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, FlorenciaKhim, D. J.Taylor, P.Bassett, R.Croom, S. M.McDermid, R. M.Poci, A.Battisti, A. J.Bland-Hawthorn, J.Bellstedt, S.Colless, M.Davies, L. J. M.Derkenne, C.Driver, S.Ferré-Mateu, A.Fisher, D. B.Gjergo, E.Johnston, E. J.Khalid, A.Kobayashi, C.Oh, S.Peng, Y.Robotham, A. S. G.Sharda, P.Sweet, S. M.Taylor, E. N.Tran, K. V. H.Trayford, J. W.van de Sande, J.Yi, S. K.Zanisi, L.SURVEYSGALAXIES: EVOLUTIONGALAXIES: KINEMATICS AND DYNAMICSGALAXIES: STAR FORMATIONGALAXIES: STELLAR CONTENTGALAXIES: STRUCTUREhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on the European Southern Observatory Very Large Telescope. MAGPI is designed to study the physical drivers of galaxy transformation at a look-back 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 Multi-Unit Spectroscopic Explorer (MUSE) observations of fields selected from the Galaxy and Mass Assembly (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 1010 M⊙) central galaxies at 0.25 < z < 0.35 in a representative range of environments (isolated, groups and clusters). The spatial resolution delivered by MUSE with Ground Layer Adaptive Optics (0.6 − 0.8 arcsec FWHM) will facilitate a direct comparison with Integral Field Spectroscopy surveys of the nearby Universe, such as SAMI and MaNGA, and at higher redshifts using adaptive optics, for example, SINS. In addition to the primary (central) galaxy sample, MAGPI will deliver resolved and unresolved spectra for as many as 150 satellite galaxies at 0.25 < z < 0.35, as well as hundreds of emission-line sources at z < 6. This paper outlines the science goals, survey design, and observing strategy of MAGPI. We also present a first look at the MAGPI data, and the theoretical framework to which MAGPI data will be compared using the current generation of cosmological hydrodynamical simulations including EAGLE, MAGNETICUM, HORIZON-AGN, and ILLUSTRIS-TNG. Our results show that cosmological hydrodynamical simulations make discrepant predictions in the spatially resolved properties of galaxies at z ≈ 0.3. MAGPI observations will place new constraints and allow for tangible improvements in galaxy formation theory.Fil: Foster, C.. The University Of Sydney; AustraliaFil: Mendel, J. T.. International Centre For Radio Astronomy Research; AustraliaFil: Lagos, C. D. P.. International Centre For Radio Astronomy Research; AustraliaFil: Wisnioski, E.. Australian National University; AustraliaFil: Yuan, T.. Swinburne University Of Technology; AustraliaFil: D'Eugenio, F.. International Centre For Radio Astronomy Research; AustraliaFil: Barone, T. M.. International Centre For Radio Astronomy Research; AustraliaFil: Harborne, K. E.. International Centre For Radio Astronomy Research; AustraliaFil: Vaughan, S. P.. International Centre For Radio Astronomy Research; AustraliaFil: Schulze, F.. International Centre For Radio Astronomy Research; AustraliaFil: Remus, R.-S.. International Centre For Radio Astronomy Research; AustraliaFil: Gupta, A.. International Centre For Radio Astronomy Research; AustraliaFil: Collacchioni, Florencia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Khim, D. J.. International Centre For Radio Astronomy Research; AustraliaFil: Taylor, P.. International Centre For Radio Astronomy Research; AustraliaFil: Bassett, R.. International Centre For Radio Astronomy Research; AustraliaFil: Croom, S. M.. International Centre For Radio Astronomy Research; AustraliaFil: McDermid, R. M.. International Centre For Radio Astronomy Research; AustraliaFil: Poci, A.. International Centre For Radio Astronomy Research; AustraliaFil: Battisti, A. J.. International Centre For Radio Astronomy Research; AustraliaFil: Bland-Hawthorn, J.. International Centre For Radio Astronomy Research; AustraliaFil: Bellstedt, S.. International Centre For Radio Astronomy Research; AustraliaFil: Colless, M.. International Centre For Radio Astronomy Research; AustraliaFil: Davies, L. J. M.. International Centre For Radio Astronomy Research; AustraliaFil: Derkenne, C.. International Centre For Radio Astronomy Research; AustraliaFil: Driver, S.. International Centre For Radio Astronomy Research; AustraliaFil: Ferré-Mateu, A.. International Centre For Radio Astronomy Research; AustraliaFil: Fisher, D. B.. International Centre For Radio Astronomy Research; AustraliaFil: Gjergo, E.. International Centre For Radio Astronomy Research; AustraliaFil: Johnston, E. J.. International Centre For Radio Astronomy Research; AustraliaFil: Khalid, A.. International Centre For Radio Astronomy Research; AustraliaFil: Kobayashi, C.. International Centre For Radio Astronomy Research; AustraliaFil: Oh, S.. International Centre For Radio Astronomy Research; AustraliaFil: Peng, Y.. International Centre For Radio Astronomy Research; AustraliaFil: Robotham, A. S. G.. International Centre For Radio Astronomy Research; AustraliaFil: Sharda, P.. International Centre For Radio Astronomy Research; AustraliaFil: Sweet, S. M.. International Centre For Radio Astronomy Research; AustraliaFil: Taylor, E. N.. International Centre For Radio Astronomy Research; AustraliaFil: Tran, K. V. H.. International Centre For Radio Astronomy Research; AustraliaFil: Trayford, J. W.. Leiden Observatory, Leiden University; Países BajosFil: van de Sande, J.. International Centre For Radio Astronomy Research; AustraliaFil: Yi, S. K.. International Centre For Radio Astronomy Research; AustraliaFil: Zanisi, L.. International Centre For Radio Astronomy Research; AustraliaCsiro Publishing2021-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/169536Foster, C.; Mendel, J. T.; Lagos, C. D. P.; Wisnioski, E.; Yuan, T.; et al.; The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework; Csiro Publishing; Publications Of The Astronomical Society Of Australia; 38; 7-2021; 1-241323-3580CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/product/identifier/S1323358021000254/type/journal_articleinfo:eu-repo/semantics/altIdentifier/doi/10.1017/pasa.2021.25info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-04-15T10:04:05Zoai:ri.conicet.gov.ar:11336/169536instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-04-15 10:04:05.701CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
title The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
spellingShingle The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
Foster, C.
SURVEYS
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STELLAR CONTENT
GALAXIES: STRUCTURE
title_short The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
title_full The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
title_fullStr The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
title_full_unstemmed The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
title_sort The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework
dc.creator.none.fl_str_mv 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, Florencia
Khim, D. J.
Taylor, P.
Bassett, R.
Croom, S. M.
McDermid, R. M.
Poci, A.
Battisti, A. J.
Bland-Hawthorn, J.
Bellstedt, S.
Colless, M.
Davies, L. J. M.
Derkenne, C.
Driver, S.
Ferré-Mateu, A.
Fisher, D. B.
Gjergo, E.
Johnston, E. J.
Khalid, A.
Kobayashi, C.
Oh, S.
Peng, Y.
Robotham, A. S. G.
Sharda, P.
Sweet, S. M.
Taylor, E. N.
Tran, K. V. H.
Trayford, J. W.
van de Sande, J.
Yi, S. K.
Zanisi, L.
author Foster, C.
author_facet 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, Florencia
Khim, D. J.
Taylor, P.
Bassett, R.
Croom, S. M.
McDermid, R. M.
Poci, A.
Battisti, A. J.
Bland-Hawthorn, J.
Bellstedt, S.
Colless, M.
Davies, L. J. M.
Derkenne, C.
Driver, S.
Ferré-Mateu, A.
Fisher, D. B.
Gjergo, E.
Johnston, E. J.
Khalid, A.
Kobayashi, C.
Oh, S.
Peng, Y.
Robotham, A. S. G.
Sharda, P.
Sweet, S. M.
Taylor, E. N.
Tran, K. V. H.
Trayford, J. W.
van de Sande, J.
Yi, S. K.
Zanisi, L.
author_role author
author2 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, Florencia
Khim, D. J.
Taylor, P.
Bassett, R.
Croom, S. M.
McDermid, R. M.
Poci, A.
Battisti, A. J.
Bland-Hawthorn, J.
Bellstedt, S.
Colless, M.
Davies, L. J. M.
Derkenne, C.
Driver, S.
Ferré-Mateu, A.
Fisher, D. B.
Gjergo, E.
Johnston, E. J.
Khalid, A.
Kobayashi, C.
Oh, S.
Peng, Y.
Robotham, A. S. G.
Sharda, P.
Sweet, S. M.
Taylor, E. N.
Tran, K. V. H.
Trayford, J. W.
van de Sande, J.
Yi, S. K.
Zanisi, L.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv SURVEYS
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STELLAR CONTENT
GALAXIES: STRUCTURE
topic SURVEYS
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STELLAR CONTENT
GALAXIES: STRUCTURE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on the European Southern Observatory Very Large Telescope. MAGPI is designed to study the physical drivers of galaxy transformation at a look-back 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 Multi-Unit Spectroscopic Explorer (MUSE) observations of fields selected from the Galaxy and Mass Assembly (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 1010 M⊙) central galaxies at 0.25 < z < 0.35 in a representative range of environments (isolated, groups and clusters). The spatial resolution delivered by MUSE with Ground Layer Adaptive Optics (0.6 − 0.8 arcsec FWHM) will facilitate a direct comparison with Integral Field Spectroscopy surveys of the nearby Universe, such as SAMI and MaNGA, and at higher redshifts using adaptive optics, for example, SINS. In addition to the primary (central) galaxy sample, MAGPI will deliver resolved and unresolved spectra for as many as 150 satellite galaxies at 0.25 < z < 0.35, as well as hundreds of emission-line sources at z < 6. This paper outlines the science goals, survey design, and observing strategy of MAGPI. We also present a first look at the MAGPI data, and the theoretical framework to which MAGPI data will be compared using the current generation of cosmological hydrodynamical simulations including EAGLE, MAGNETICUM, HORIZON-AGN, and ILLUSTRIS-TNG. Our results show that cosmological hydrodynamical simulations make discrepant predictions in the spatially resolved properties of galaxies at z ≈ 0.3. MAGPI observations will place new constraints and allow for tangible improvements in galaxy formation theory.
Fil: Foster, C.. The University Of Sydney; Australia
Fil: Mendel, J. T.. International Centre For Radio Astronomy Research; Australia
Fil: Lagos, C. D. P.. International Centre For Radio Astronomy Research; Australia
Fil: Wisnioski, E.. Australian National University; Australia
Fil: Yuan, T.. Swinburne University Of Technology; Australia
Fil: D'Eugenio, F.. International Centre For Radio Astronomy Research; Australia
Fil: Barone, T. M.. International Centre For Radio Astronomy Research; Australia
Fil: Harborne, K. E.. International Centre For Radio Astronomy Research; Australia
Fil: Vaughan, S. P.. International Centre For Radio Astronomy Research; Australia
Fil: Schulze, F.. International Centre For Radio Astronomy Research; Australia
Fil: Remus, R.-S.. International Centre For Radio Astronomy Research; Australia
Fil: Gupta, A.. International Centre For Radio Astronomy Research; Australia
Fil: Collacchioni, Florencia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Khim, D. J.. International Centre For Radio Astronomy Research; Australia
Fil: Taylor, P.. International Centre For Radio Astronomy Research; Australia
Fil: Bassett, R.. International Centre For Radio Astronomy Research; Australia
Fil: Croom, S. M.. International Centre For Radio Astronomy Research; Australia
Fil: McDermid, R. M.. International Centre For Radio Astronomy Research; Australia
Fil: Poci, A.. International Centre For Radio Astronomy Research; Australia
Fil: Battisti, A. J.. International Centre For Radio Astronomy Research; Australia
Fil: Bland-Hawthorn, J.. International Centre For Radio Astronomy Research; Australia
Fil: Bellstedt, S.. International Centre For Radio Astronomy Research; Australia
Fil: Colless, M.. International Centre For Radio Astronomy Research; Australia
Fil: Davies, L. J. M.. International Centre For Radio Astronomy Research; Australia
Fil: Derkenne, C.. International Centre For Radio Astronomy Research; Australia
Fil: Driver, S.. International Centre For Radio Astronomy Research; Australia
Fil: Ferré-Mateu, A.. International Centre For Radio Astronomy Research; Australia
Fil: Fisher, D. B.. International Centre For Radio Astronomy Research; Australia
Fil: Gjergo, E.. International Centre For Radio Astronomy Research; Australia
Fil: Johnston, E. J.. International Centre For Radio Astronomy Research; Australia
Fil: Khalid, A.. International Centre For Radio Astronomy Research; Australia
Fil: Kobayashi, C.. International Centre For Radio Astronomy Research; Australia
Fil: Oh, S.. International Centre For Radio Astronomy Research; Australia
Fil: Peng, Y.. International Centre For Radio Astronomy Research; Australia
Fil: Robotham, A. S. G.. International Centre For Radio Astronomy Research; Australia
Fil: Sharda, P.. International Centre For Radio Astronomy Research; Australia
Fil: Sweet, S. M.. International Centre For Radio Astronomy Research; Australia
Fil: Taylor, E. N.. International Centre For Radio Astronomy Research; Australia
Fil: Tran, K. V. H.. International Centre For Radio Astronomy Research; Australia
Fil: Trayford, J. W.. Leiden Observatory, Leiden University; Países Bajos
Fil: van de Sande, J.. International Centre For Radio Astronomy Research; Australia
Fil: Yi, S. K.. International Centre For Radio Astronomy Research; Australia
Fil: Zanisi, L.. International Centre For Radio Astronomy Research; Australia
description We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on the European Southern Observatory Very Large Telescope. MAGPI is designed to study the physical drivers of galaxy transformation at a look-back 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 Multi-Unit Spectroscopic Explorer (MUSE) observations of fields selected from the Galaxy and Mass Assembly (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 1010 M⊙) central galaxies at 0.25 < z < 0.35 in a representative range of environments (isolated, groups and clusters). The spatial resolution delivered by MUSE with Ground Layer Adaptive Optics (0.6 − 0.8 arcsec FWHM) will facilitate a direct comparison with Integral Field Spectroscopy surveys of the nearby Universe, such as SAMI and MaNGA, and at higher redshifts using adaptive optics, for example, SINS. In addition to the primary (central) galaxy sample, MAGPI will deliver resolved and unresolved spectra for as many as 150 satellite galaxies at 0.25 < z < 0.35, as well as hundreds of emission-line sources at z < 6. This paper outlines the science goals, survey design, and observing strategy of MAGPI. We also present a first look at the MAGPI data, and the theoretical framework to which MAGPI data will be compared using the current generation of cosmological hydrodynamical simulations including EAGLE, MAGNETICUM, HORIZON-AGN, and ILLUSTRIS-TNG. Our results show that cosmological hydrodynamical simulations make discrepant predictions in the spatially resolved properties of galaxies at z ≈ 0.3. MAGPI observations will place new constraints and allow for tangible improvements in galaxy formation theory.
publishDate 2021
dc.date.none.fl_str_mv 2021-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/169536
Foster, C.; Mendel, J. T.; Lagos, C. D. P.; Wisnioski, E.; Yuan, T.; et al.; The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework; Csiro Publishing; Publications Of The Astronomical Society Of Australia; 38; 7-2021; 1-24
1323-3580
CONICET Digital
CONICET
url http://hdl.handle.net/11336/169536
identifier_str_mv Foster, C.; Mendel, J. T.; Lagos, C. D. P.; Wisnioski, E.; Yuan, T.; et al.; The MAGPI survey: science goals, design, observing strategy, early results and theoretical framework; Csiro Publishing; Publications Of The Astronomical Society Of Australia; 38; 7-2021; 1-24
1323-3580
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/product/identifier/S1323358021000254/type/journal_article
info:eu-repo/semantics/altIdentifier/doi/10.1017/pasa.2021.25
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Csiro Publishing
publisher.none.fl_str_mv Csiro Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1862631182661844992
score 13.203462

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