Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24160
DC Field | Value | Language |
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dc.contributor.author | Conrad, A. | en_US |
dc.contributor.author | de Kleer, K. | en_US |
dc.contributor.author | Leisenring, J. | en_US |
dc.contributor.author | La Camera, A. | en_US |
dc.contributor.author | ARCIDIACONO, CARMELO | en_US |
dc.contributor.author | Bertero, M. | en_US |
dc.contributor.author | Boccacci, P. | en_US |
dc.contributor.author | Defrère, D. | en_US |
dc.contributor.author | de Pater, I. | en_US |
dc.contributor.author | Hinz, P. | en_US |
dc.contributor.author | Hoffman, K. -H. | en_US |
dc.contributor.author | Kürster, M. | en_US |
dc.contributor.author | Rathbun, J. | en_US |
dc.contributor.author | Schertl, D. | en_US |
dc.contributor.author | Skemer, A. | en_US |
dc.contributor.author | Skrutskie, M. | en_US |
dc.contributor.author | Spencer, J. | en_US |
dc.contributor.author | Veillet, C. | en_US |
dc.contributor.author | Weigelt, G. | en_US |
dc.contributor.author | Woodward, C. | en_US |
dc.date.accessioned | 2020-04-21T11:14:14Z | - |
dc.date.available | 2020-04-21T11:14:14Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24160 | - |
dc.description.abstract | We report here results from observing Io at high angular resolution, ̃32 mas at 4.8 μm, with LBT at two favorable oppositions as described in our report given at the 2011 EPSC [1]. Analysis of datasets acquired during the last two oppositions has yielded spatially resolved M-band emission at Loki Patera [2], L-band fringes at an eruption site, an occultation of Loki and Pele by Europa, and sufficient sub-earth longitude (SEL) and parallactic angle coverage to produce a full disk map.We summarize completed results for the first of these, and give brief progress reports for the latter three. Finally, we provide plans for imaging the full disk of Jupiter using the MCAO system which is in its commissioning phase at LBT. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | High resolution LBT imaging of Io and Jupiter | en_US |
dc.type | Conference abstract | - |
dc.identifier.url | https://www.epsc2015.eu/ | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | EPSC2015-351 | en_US |
dc.relation.numberofpages | 2 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 20 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.ispartofbook | European Planetary Science Congress 2015 (EPCS) | en_US |
dc.relation.conferencename | European Planetary Science Congress 2015 (EPCS) | en_US |
dc.relation.conferenceplace | Nantes, France | en_US |
dc.relation.conferencedate | 27 September-2 October, 2015 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 274 Abstract in Atti di convegno | - |
dc.identifier.adsbibcode | 2015EPSC...10..351C | 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 abstract | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0003-0142-8108 | - |
Appears in Collections: | 3.02 Abstract in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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EPSC2015-351.pdf | 700.84 kB | Adobe PDF | View/Open |
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