Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28314
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | PLANTET, CEDRIC ANTOINE ADRIEN GABRIEL | en_US |
dc.contributor.author | Bond, Charlotte Z. | en_US |
dc.contributor.author | Giordano, Christophe | en_US |
dc.contributor.author | AGAPITO, GUIDO | en_US |
dc.contributor.author | Taheri, Mojtaba | en_US |
dc.contributor.author | ESPOSITO, Simone | en_US |
dc.contributor.author | Wizinowich, Peter | en_US |
dc.date.accessioned | 2020-11-13T12:04:46Z | - |
dc.date.available | 2020-11-13T12:04:46Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 9781510619593 | en_US |
dc.identifier.isbn | 9781510619609 | en_US |
dc.identifier.issn | 0277-786X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28314 | - |
dc.description.abstract | A future upgrade of the Keck II telescope's adaptive optics system will include a near-infrared pyramid wavefront sensor. It will benefit from low-noise infrared detector technology, specifically the avalanche photodiode array SAPHIRA (Leonardo). The system will either operate with a natural guide star in a single conjugated adaptive optics system, or using a laser guide star (LGS), with the pyramid working as a low-order sensor. We present a study of the pyramid sensor's performance via end-to-end simulations, including an analysis of calibration strategies. For LGS operation, we compare the pyramid to LIFT, a focal-plane sensor dedicated to low-order sensing. | en_US |
dc.language.iso | eng | en_US |
dc.title | Keck II adaptive optics upgrade: simulations of the near-infrared pyramid sensor | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.2313190 | en_US |
dc.identifier.scopus | 2-s2.0-85053550097 | en_US |
dc.identifier.isi | 000452819300096 | en_US |
dc.identifier.url | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10703/2313190/Keck-II-adaptive-optics-upgrade--simulations-of-the-near/10.1117/12.2313190.short | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 10703 | en_US |
dc.relation.firstpage | 1070335 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 7 | en_US |
dc.description.international | sì | en_US |
dc.relation.alleditors | Close, Laird M.; Schreiber, Laura; Schmidt, Dirk | en_US |
dc.relation.ispartofbook | Adaptive Optics Systems VI | en_US |
dc.relation.conferencename | Adaptive Optics Systems VI | en_US |
dc.relation.conferenceplace | Austin, Texas, United States | en_US |
dc.relation.conferencedate | 10-15 June, 2018 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF SPIE | en_US |
dc.identifier.adsbibcode | 2018SPIE10703E..35P | 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. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-3898-4004 | - |
crisitem.author.orcid | 0000-0002-6382-2613 | - |
crisitem.author.orcid | 0000-0002-3114-677X | - |
crisitem.journal.journalissn | 0277-786X | - |
crisitem.journal.ance | E136238 | - |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
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[C56] Plantet (2018).pdf | Pdf editoriale | 517.72 kB | Adobe PDF | Visualizza/apri |
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