Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24522
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Yagoubov, Pavel | en_US |
dc.contributor.author | Gonzalez, A. | en_US |
dc.contributor.author | Tapia, V. | en_US |
dc.contributor.author | Reyes, N. | en_US |
dc.contributor.author | Mena, F. P. | en_US |
dc.contributor.author | NESTI, Renzo | en_US |
dc.contributor.author | CUTTAIA, FRANCESCO | en_US |
dc.contributor.author | RICCIARDI, SARA | en_US |
dc.contributor.author | VILLA, FABRIZIO | en_US |
dc.date.accessioned | 2020-05-05T15:23:09Z | - |
dc.date.available | 2020-05-05T15:23:09Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 978-1-4673-8485-8 | en_US |
dc.identifier.isbn | 978-1-4673-8486-5 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24522 | - |
dc.description.abstract | In this paper we report the first results of the optical components development and the overall optical design for a wideband receiver to simultaneously cover ALMA bands 2 and 3. Two types of feed horns and OMTs have been designed to couple to the ALMA telescope beam using a modified Fresnel lens. Both types of hardware have been manufactured and tested in a near field beam scanner. The measured beam patterns and optical efficiencies are in good agreement with simulations. | en_US |
dc.language.iso | eng | en_US |
dc.title | 67-116 GHz optics development for ALMA band 2-3 receivers | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1109/IRMMW-THz.2016.7758971 | en_US |
dc.identifier.scopus | 2-s2.0-85006173274 | en_US |
dc.identifier.url | https://ieeexplore.ieee.org/document/7758971 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 1 | en_US |
dc.relation.lastpage | 2 | en_US |
dc.relation.numberofpages | 2 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | CHL | en_US |
dc.contributor.country | JPN | en_US |
dc.relation.ispartofbook | 2016 41st International Conference on Infrared, Millimeter, and Terahertz waves (IRMMW-THz) | en_US |
dc.publisher.name | IEEE | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | 2016 41st International Conference on Infrared, Millimeter, and Terahertz waves (IRMMW-THz) | en_US |
dc.relation.conferenceplace | Copenhagen, Denmark | en_US |
dc.relation.conferencedate | 25-30 Sept. 2016 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2016imtw.confE...2Y | 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::PE9_17 Instrumentation – telescopes, detectors and techniques | 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 | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-0303-839X | - |
crisitem.author.orcid | 0000-0001-6608-5017 | - |
crisitem.author.orcid | 0000-0002-3807-4043 | - |
crisitem.author.orcid | 0000-0003-1798-861X | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
PID4362061.pdf | postprint | 467.47 kB | Adobe PDF | View/Open |
07758971.pdf | [Administrators only] | 346.57 kB | Adobe PDF |
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