Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31086
DC Field | Value | Language |
---|---|---|
dc.contributor.author | AGAPITO, GUIDO | en_US |
dc.contributor.author | Vassallo, Daniele | en_US |
dc.contributor.author | PLANTET, CEDRIC ANTOINE ADRIEN GABRIEL | en_US |
dc.contributor.author | VIOTTO, VALENTINA | en_US |
dc.contributor.author | PINNA, Enrico | en_US |
dc.contributor.author | Benoit Neichel | en_US |
dc.contributor.author | Thierry Fusco | en_US |
dc.contributor.author | Francois Rigaut | en_US |
dc.date.accessioned | 2021-11-16T10:09:36Z | - |
dc.date.available | 2021-11-16T10:09:36Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.isbn | 9781510636835 | en_US |
dc.identifier.isbn | 9781510636842 | en_US |
dc.identifier.issn | 0277-786X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31086 | - |
dc.description.abstract | The MCAO Assisted Visible Imager and Spectrograph (MAVIS) Adaptive Optics Module has very demanding goals to support science in the optical: providing 15% SR in V band on a large FoV of 30arcsec diameter in standard atmospheric conditions at Paranal. It will be able to work in closed loop on up to three natural guide stars down to H=19, providing a sky coverage larger than 50% in the south galactic pole. Such goals and the exploration of a large MCAO system parameters space have required a combination of analytical and end- to-end simulations to assess performance, sky coverage and drive the design. In this work we report baseline performance, statistical sky coverage and parameters sensitivity analysis done in the phase-A instrument study. | en_US |
dc.language.iso | eng | en_US |
dc.title | MAVIS: system modelling and performance prediction | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.2561252 | en_US |
dc.identifier.scopus | 2-s2.0-85100004433 | en_US |
dc.identifier.url | http://arxiv.org/abs/2012.14487v1 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 11448 | en_US |
dc.relation.firstpage | 103 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.alleditors | Schreiber, Laura; Schmidt, Dirk; Vernet, Elise | en_US |
dc.relation.ispartofbook | Adaptive Optics Systems VII | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Adaptive Optics Systems VII | en_US |
dc.relation.conferenceplace | California, United States | en_US |
dc.relation.conferencedate | 14-18 December, 2020 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | PROCEEDINGS OF SPIE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2020SPIE11448E..3RA | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-6382-2613 | - |
crisitem.author.orcid | 0000-0002-3286-6349 | - |
crisitem.author.orcid | 0000-0002-3898-4004 | - |
crisitem.author.orcid | 0000-0001-5700-9565 | - |
crisitem.author.orcid | 0000-0002-6243-5697 | - |
crisitem.journal.journalissn | 0277-786X | - |
crisitem.journal.ance | E136238 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
MAVIS__System_modelling_and_performance_prediction.pdf | preprint | 1.6 MB | Adobe PDF | View/Open |
SPIE114483R.pdf | Pdf editoriale | 1.68 MB | Adobe PDF | View/Open |
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