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MOONRISE : the main MOONS GTO Extragalactic Survey
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dc.contributor.author | Maiolino, R. | |
dc.contributor.author | Cirasuolo, M. | |
dc.contributor.author | Afonso, J. | |
dc.contributor.author | Bauer, F. E. | |
dc.contributor.author | Bowler, R. | |
dc.contributor.author | Cucciati, O. | |
dc.contributor.author | Daddi, E. | |
dc.contributor.author | De Lucia, G. | |
dc.contributor.author | Evans, C. | |
dc.contributor.author | Flores, H. | |
dc.contributor.author | Gargiulo, A. | |
dc.contributor.author | Garilli, B. | |
dc.contributor.author | Jablonka, P. | |
dc.contributor.author | Jarvis, M. | |
dc.contributor.author | Kneib, J.-P. | |
dc.contributor.author | Lilly, S. | |
dc.contributor.author | Looser, T. | |
dc.contributor.author | Magliocchetti, M. | |
dc.contributor.author | Man, Z. | |
dc.contributor.author | Mannucci, F. | |
dc.contributor.author | Maurogordato, S. | |
dc.contributor.author | McLure, R. J. | |
dc.contributor.author | Norberg, P. | |
dc.contributor.author | Oesch, P. | |
dc.contributor.author | Oliva, E. | |
dc.contributor.author | Paltani, S. | |
dc.contributor.author | Pappalardo, C. | |
dc.contributor.author | Peng, Y. | |
dc.contributor.author | Pentericci, L. | |
dc.contributor.author | Pozzetti, L. | |
dc.contributor.author | Renzini, A. | |
dc.contributor.author | Rodrigues, M. | |
dc.contributor.author | Royer, F. | |
dc.contributor.author | Serjeant, S. | |
dc.contributor.author | Vanzi, L. | |
dc.contributor.author | Wild, V. | |
dc.contributor.author | Zamorani, G. | |
dc.date.accessioned | 2020-10-28T17:30:04Z | |
dc.date.available | 2020-10-28T17:30:04Z | |
dc.date.issued | 2020-06-30 | |
dc.identifier.citation | Maiolino , R , Cirasuolo , M , Afonso , J , Bauer , F E , Bowler , R , Cucciati , O , Daddi , E , De Lucia , G , Evans , C , Flores , H , Gargiulo , A , Garilli , B , Jablonka , P , Jarvis , M , Kneib , J-P , Lilly , S , Looser , T , Magliocchetti , M , Man , Z , Mannucci , F , Maurogordato , S , McLure , R J , Norberg , P , Oesch , P , Oliva , E , Paltani , S , Pappalardo , C , Peng , Y , Pentericci , L , Pozzetti , L , Renzini , A , Rodrigues , M , Royer , F , Serjeant , S , Vanzi , L , Wild , V & Zamorani , G 2020 , ' MOONRISE : the main MOONS GTO Extragalactic Survey ' The Messenger , vol. 180 , pp. 24-29 . https://doi.org/10.18727/0722-6691/5197 | en |
dc.identifier.issn | 0722-6691 | |
dc.identifier.other | PURE: 270929292 | |
dc.identifier.other | PURE UUID: 25e69423-e92b-45bb-98d4-6555d921c668 | |
dc.identifier.other | BibCode: 2020Msngr.180...24M | |
dc.identifier.uri | https://hdl.handle.net/10023/20849 | |
dc.description.abstract | The MOONS instrument possesses an exceptional combination of large multiplexing, high sensitivity, broad simultaneous spectral coverage (from optical to near-infrared bands), large patrol area and high fibre density. These properties provide the unprecedented potential of enabling, for the very first time, SDSS-like surveys around Cosmic Noon(z ~ 1–2.5), when the star formation rate in the Universe peaked. The high-quality spectra delivered by MOONS will sample the same nebular and stellar diagnostics observed in extensive surveys of local galaxies, providing an accurate and consistent description of the evolution ofvarious physical properties of galaxies, and hence a solid test of different scenarios of galaxy formation and transformation. Most importantly, by spectroscopically identifying hundreds of thousands of galaxies at high redshift, the MOONS surveys will be capable of determining the environments in which primeval galaxies lived and will reveal how such environments affected galaxy evolution. In this article, we specifically focus on the main Guaranteed Time Observation (GTO) MOONS extragalactic survey, MOONRISE, by providing an overview of its scientific goals and observing strategy. | |
dc.format.extent | 6 | |
dc.language.iso | eng | |
dc.relation.ispartof | The Messenger | en |
dc.rights | Copyright © 2020 ESO. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.18727/0722-6691/5197. | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | T-NDAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | MOONRISE : the main MOONS GTO Extragalactic Survey | en |
dc.type | Journal article | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.18727/0722-6691/5197 | |
dc.identifier.url | http://adsabs.harvard.edu/abs/2020Msngr.180...24M | en |
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