Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28338
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SCHREIBER, LAURA | en_US |
dc.contributor.author | Feautrier, Philippe | en_US |
dc.contributor.author | Stadler, Eric | en_US |
dc.contributor.author | Rabou, Patrick | en_US |
dc.contributor.author | Correia, Jean-Jacques | en_US |
dc.contributor.author | Glück, Laurence | en_US |
dc.contributor.author | Rochat, Sylvain | en_US |
dc.contributor.author | Jocou, Laurent | en_US |
dc.contributor.author | Magnard, Yves | en_US |
dc.contributor.author | Moulin, Thibaut | en_US |
dc.contributor.author | Delboulbé, Alain | en_US |
dc.contributor.author | Douté, Sylvain | en_US |
dc.contributor.author | Chauvin, Gaël. | en_US |
dc.contributor.author | Moraux, Estelle | en_US |
dc.contributor.author | Oberti, Sylvain | en_US |
dc.contributor.author | Verinaud, Christophe | en_US |
dc.contributor.author | CORTECCHIA, Fausto | en_US |
dc.contributor.author | ARCIDIACONO, CARMELO | en_US |
dc.contributor.author | DIOLAITI, EMILIANO | en_US |
dc.contributor.author | CILIEGI, Paolo | en_US |
dc.contributor.author | BELLAZZINI, Michele | en_US |
dc.contributor.author | ESPOSITO, Simone | en_US |
dc.contributor.author | BUSONI, LORENZO | en_US |
dc.contributor.author | RAGAZZONI, Roberto | en_US |
dc.date.accessioned | 2020-11-13T15:38:11Z | - |
dc.date.available | 2020-11-13T15:38:11Z | - |
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/20.500.12386/28338 | - |
dc.description | The author thanks the Institut de Planetologie et d'Astrophysique de Grenoble (IPAG) for hospitality. | en_US |
dc.description.abstract | MAORY will be the multi-adaptive optics module feeding the high resolution camera and spectrograph MICADO at the Extremely Large Telescope (ELT) first light. In order to ensure high and homogeneous image quality over the MICADO field of view and high sky coverage, the baseline is to operate wavefront sensing using six Sodium Laser Guide Stars. The Laser Guide Star Wavefront Sensor (LGS WFS) is the MAORY sub-system devoted to real-time measurement of the high order wavefront distortions. In this paper we describe the MAORY LGS WFS current design, including opto-mechanics, trade-offs and possible future improvements. | en_US |
dc.language.iso | eng | en_US |
dc.title | The MAORY laser guide star wavefront sensor: design status | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.2314467 | en_US |
dc.identifier.scopus | 2-s2.0-85053553813 | en_US |
dc.identifier.isi | 000452819300062 | en_US |
dc.identifier.url | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10703/2314467/The-MAORY-laser-guide-star-wavefront-sensor-design-status/10.1117/12.2314467.short | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 10703 | en_US |
dc.relation.firstpage | 107031Y-1 | en_US |
dc.relation.lastpage | 107031Y-9 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 24 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.relation.alleditors | Close, Laird; 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..1YS | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0277-786X | - |
crisitem.journal.ance | E136238 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-6657-8054 | - |
crisitem.author.orcid | 0000-0001-5072-7791 | - |
crisitem.author.orcid | 0000-0003-0142-8108 | - |
crisitem.author.orcid | 0000-0002-3978-0695 | - |
crisitem.author.orcid | 0000-0002-0447-4620 | - |
crisitem.author.orcid | 0000-0001-8200-810X | - |
crisitem.author.orcid | 0000-0002-3114-677X | - |
crisitem.author.orcid | 0000-0002-2074-0458 | - |
crisitem.author.orcid | 0000-0002-7697-5555 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2018_Schreiber_SPIE.pdf | Pdf editoriale | 1.02 MB | Adobe PDF | View/Open |
Schreiber.pdf | postprint | 1.17 MB | Adobe PDF | View/Open |
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