The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
dc.contributor.author | Foster, C. | |
dc.contributor.author | Mendel, J. T. | |
dc.contributor.author | Lagos, C. D. P. | |
dc.contributor.author | Wisnioski, E. | |
dc.contributor.author | Yuan, T. | |
dc.contributor.author | D'Eugenio, F. | |
dc.contributor.author | Barone, T. M. | |
dc.contributor.author | Harborne, K. E. | |
dc.contributor.author | Vaughan, S. P. | |
dc.contributor.author | Schulze, F. | |
dc.contributor.author | Remus, R. -S. | |
dc.contributor.author | Gupta, A. | |
dc.contributor.author | Collacchioni, F. | |
dc.contributor.author | Khim, D. J. | |
dc.contributor.author | Taylor, P. | |
dc.contributor.author | Bassett, R. | |
dc.contributor.author | Croom, S. M. | |
dc.contributor.author | McDermid, R. M. | |
dc.contributor.author | Poci, A. | |
dc.contributor.author | Battisti, A. J. | |
dc.contributor.author | Bland-Hawthorn, J. | |
dc.contributor.author | Bellstedt, S. | |
dc.contributor.author | Colless, M. | |
dc.contributor.author | Davies, L. J. M. | |
dc.contributor.author | Derkenne, C. | |
dc.contributor.author | Driver, S. | |
dc.contributor.author | Ferré-Mateu, A. | |
dc.contributor.author | Fisher, D. B. | |
dc.contributor.author | Gjergo, E. | |
dc.contributor.author | Johnston, E. J. | |
dc.contributor.author | Khalid, A. | |
dc.contributor.author | Kobayashi, C. | |
dc.contributor.author | Oh, S. | |
dc.contributor.author | Peng, Y. | |
dc.contributor.author | Robotham, A. S. G. | |
dc.contributor.author | Sharda, P. | |
dc.contributor.author | Sweet, S. M. | |
dc.contributor.author | Taylor, E. N. | |
dc.contributor.author | Tran, K. -V. H. | |
dc.contributor.author | Trayford, J. W. | |
dc.contributor.author | Sande, J. van de | |
dc.contributor.author | Yi, S. K. | |
dc.contributor.author | Zanisi, L. | |
dc.date.accessioned | 2021-08-06T11:00:01Z | |
dc.date.available | 2021-08-06T11:00:01Z | |
dc.date.issued | 2021-07-26 | |
dc.identifier.citation | 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 , 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 , Sande , J V D , Yi , S K & 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 | |
dc.identifier.issn | 1323-3580 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/2011.13567v3 | |
dc.identifier.other | ORCID: /0000-0002-4343-0487/work/98164021 | |
dc.identifier.uri | http://hdl.handle.net/2299/24963 | |
dc.description | © 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 | |
dc.description.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 | en |
dc.format.extent | 31 | |
dc.format.extent | 11208839 | |
dc.language.iso | eng | |
dc.relation.ispartof | Publications of the Astronomical Society of Australia | |
dc.subject | astro-ph.GA | |
dc.title | The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework | en |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.date.embargoedUntil | 2021-07-26 | |
rioxxterms.versionofrecord | 10.1017/pasa.2021.25 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |