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dc.contributor.authorWeinreb, S.
dc.contributor.authorMani, H.
dc.contributor.authorZhong, W.
dc.contributor.authorFlygare, J.
dc.contributor.authorBillade, B.
dc.contributor.authorAkgiray, Ahmed Halid
dc.contributor.authorDong, L.
dc.date.accessioned2020-05-27T13:21:18Z
dc.date.available2020-05-27T13:21:18Z
dc.date.issued2018
dc.identifier.isbn978-1-78561-815-4
dc.identifier.urihttp://hdl.handle.net/10679/6599
dc.identifier.urihttps://ieeexplore.ieee.org/document/8568499
dc.description.abstractCurrent and future large arrays for radio astronomy are compared and the Next Generation Very Large Array, ngVLA, is introduced. Receiver requirements are described and a 4-feed system covering 1.2 to 116 GHz, in a single vacuum cryogenic enclosure is presented followed by description of the reflector optics, the wide-band feeds, and the expected system performanceen_US
dc.description.sponsorshipSander Weinreb ; Hamdi Mani
dc.language.isoengen_US
dc.publisherIEEEen_US
dc.relation.ispartof12th European Conference on Antennas and Propagation (EuCAP 2018)
dc.rightsrestrictedAccess
dc.titleCryogenic 1.2 to 116 GHz receiver for large arraysen_US
dc.typeConference paperen_US
dc.publicationstatusPublisheden_US
dc.contributor.departmentÖzyeğin University
dc.contributor.authorID(ORCID 0000-0002-7373-4158 & YÖK ID 319662) Akgiray, Ahmed
dc.contributor.ozuauthorAkgiray, Ahmed Halid
dc.subject.keywordsRadio astronomyen_US
dc.subject.keywordsCryogenicen_US
dc.subject.keywordsQRFHen_US
dc.subject.keywordsLow noise amplifiersen_US
dc.identifier.scopusSCOPUS:2-s2.0-85057339113
dc.contributor.authorMale1
dc.relation.publicationcategoryConference Paper - International - Institutional Academic Staff


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