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Progress in the Design of the Atacama Large Aperture Submillimeter Telescope

dc.date.accessioned2024-01-29T18:20:53Z
dc.date.available2024-01-29T18:20:53Z
dc.date.created2024-01-15T12:30:23Z
dc.date.issued2023
dc.identifier.citationMroczkowski, Tony Cicone, Claudia Reichert, Matthias Gallardo, Patricio A. Kaercher, Hans Hills, Richard Bok, Daniel Dahl, Erik Dubois-Dit-Bonclaude, Pierre Kiselev, Aleksej Timpe, Martin Zimmerer, Thomas Dicker, Simon R. Macintosh, Mike Klaassen, Pamela D. Niemack, Michael D. . Progress in the Design of the Atacama Large Aperture Submillimeter Telescope. 2023 XXXVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS). 2023 Institute of Electrical and Electronics Engineers (IEEE)
dc.identifier.urihttp://hdl.handle.net/10852/107239
dc.description.abstractThe Atacama Large Aperture Submillimeter Telescope (At- LAST) aims to be the premier next generation large diameter (50 meter) single dish observatory capable of observations across the millimeter/submillimeter spectrum, from 30 GHz to 1 THz. AtLAST will be sited in Chile at approximately 5100 meters above sea level, high in the Atacama Desert near Llano de Chajnantor. The novel rockingchair telescope design allows for a unprecedentedly wide field of view (FoV) of 1-2◦ diameter, a large receiver cabin housing six major instruments, and high structural stability during fast scanning operations (up to ~ 3◦ per second in azimuth). Here we describe the current status of, and expected outcomes for, the antenna design study, which will be completed in 2024.
dc.languageEN
dc.publisherInstitute of Electrical and Electronics Engineers (IEEE)
dc.titleProgress in the Design of the Atacama Large Aperture Submillimeter Telescope
dc.title.alternativeENEngelskEnglishProgress in the Design of the Atacama Large Aperture Submillimeter Telescope
dc.typeChapter
dc.creator.authorMroczkowski, Tony
dc.creator.authorCicone, Claudia
dc.creator.authorReichert, Matthias
dc.creator.authorGallardo, Patricio A.
dc.creator.authorKaercher, Hans
dc.creator.authorHills, Richard
dc.creator.authorBok, Daniel
dc.creator.authorDahl, Erik
dc.creator.authorDubois-Dit-Bonclaude, Pierre
dc.creator.authorKiselev, Aleksej
dc.creator.authorTimpe, Martin
dc.creator.authorZimmerer, Thomas
dc.creator.authorDicker, Simon R.
dc.creator.authorMacintosh, Mike
dc.creator.authorKlaassen, Pamela D.
dc.creator.authorNiemack, Michael D.
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
dc.identifier.cristin2226571
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.btitle=2023 XXXVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)&rft.spage=&rft.date=2023
dc.identifier.doihttps://doi.org/10.23919/URSIGASS57860.2023.10265372
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentBokkapittel
dc.type.peerreviewedPeer reviewed
dc.source.isbn979-83-503-0997-3
dc.type.versionPublishedVersion
cristin.btitle2023 XXXVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS)


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