Cryogenic 1.2 to 116 GHz receiver for large arrays
dc.contributor.author | Weinreb, S. | |
dc.contributor.author | Mani, H. | |
dc.contributor.author | Zhong, W. | |
dc.contributor.author | Flygare, J. | |
dc.contributor.author | Billade, B. | |
dc.contributor.author | Akgiray, Ahmed Halid | |
dc.contributor.author | Dong, L. | |
dc.date.accessioned | 2020-05-27T13:21:18Z | |
dc.date.available | 2020-05-27T13:21:18Z | |
dc.date.issued | 2018 | |
dc.identifier.isbn | 978-1-78561-815-4 | |
dc.identifier.uri | http://hdl.handle.net/10679/6599 | |
dc.identifier.uri | https://ieeexplore.ieee.org/document/8568499 | |
dc.description.abstract | Current 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 performance | en_US |
dc.description.sponsorship | Sander Weinreb ; Hamdi Mani | |
dc.language.iso | eng | en_US |
dc.publisher | IEEE | en_US |
dc.relation.ispartof | 12th European Conference on Antennas and Propagation (EuCAP 2018) | |
dc.rights | restrictedAccess | |
dc.title | Cryogenic 1.2 to 116 GHz receiver for large arrays | en_US |
dc.type | Conference paper | en_US |
dc.publicationstatus | Published | en_US |
dc.contributor.department | Özyeğin University | |
dc.contributor.authorID | (ORCID 0000-0002-7373-4158 & YÖK ID 319662) Akgiray, Ahmed | |
dc.contributor.ozuauthor | Akgiray, Ahmed Halid | |
dc.subject.keywords | Radio astronomy | en_US |
dc.subject.keywords | Cryogenic | en_US |
dc.subject.keywords | QRFH | en_US |
dc.subject.keywords | Low noise amplifiers | en_US |
dc.identifier.scopus | SCOPUS:2-s2.0-85057339113 | |
dc.contributor.authorMale | 1 | |
dc.relation.publicationcategory | Conference Paper - International - Institutional Academic Staff |
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