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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8346
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dc.contributor.authorGalitzki, Nicholas-
dc.contributor.authorTsan, Tran-
dc.contributor.authorSpisak, Jake-
dc.contributor.authorRandall, Michael-
dc.contributor.authorSilva-Feaver, Max-
dc.contributor.authorSeibert, Joseph-
dc.contributor.authorLashner, Jacob-
dc.contributor.authorAdachi, Shunsuke-
dc.contributor.authorAdkins, Sean M.-
dc.contributor.authorAlford, Thomas-
dc.contributor.authorArnold, Kam-
dc.contributor.authorAshton, Peter C.-
dc.contributor.authorAustermann, Jason E.-
dc.contributor.authorBaccigalupi, Carlo-
dc.contributor.authorBazarko, Andrew-
dc.contributor.authorBeall, James A.-
dc.contributor.authorBhimani, Sanah-
dc.contributor.authorBixler, Bryce-
dc.contributor.authorCoppi, Gabriele-
dc.contributor.authorCorbett, Lance-
dc.contributor.authorCrowley, Kevin D.-
dc.contributor.authorCrowley, Kevin T.-
dc.contributor.authorDay-Weiss, Samuel-
dc.contributor.authorDevlin, Mark J.-
dc.contributor.authorDicker, Simon-
dc.contributor.authorDiGia, Brooke-
dc.contributor.authorDow, Peter N.-
dc.contributor.authorDuell, Cody J.-
dc.contributor.authorDuff, Shannon M.-
dc.contributor.authorGerras, Remington G.-
dc.contributor.authorGroh, John C.-
dc.contributor.authorGudmundsson, Jon E.-
dc.contributor.authorHarrington, Kathleen-
dc.contributor.authorHasegawa, Masaya-
dc.contributor.authorHealy, Erin-
dc.contributor.authorHenderson, Shawn W.-
dc.contributor.authorHubmayr, Johannes-
dc.contributor.authorIuliano, Jeffrey-
dc.contributor.authorJohnson, Bradley R.-
dc.contributor.authorKeating, Brian-
dc.contributor.authorKeller, Ben-
dc.contributor.authorKiuchi, Kenji-
dc.contributor.authorKofman, Anna M.-
dc.contributor.authorKoopman, Brian J.-
dc.contributor.authorKusaka, Akito-
dc.contributor.authorLee, Adrian T.-
dc.contributor.authorLew, Richard A.-
dc.contributor.authorLin, Lawrence T.-
dc.contributor.authorLink, Michael J.-
dc.contributor.authorLucas, Tammy J.-
dc.contributor.authorLungu, Marius-
dc.contributor.authorMangu, Aashrita-
dc.contributor.authorMcMahon, Jeffrey J.-
dc.contributor.authorMiller, Amber D.-
dc.contributor.authorMoore, Jenna E.-
dc.contributor.authorMorshed, Magdy-
dc.contributor.authorNakata, Hironobu-
dc.contributor.authorNati, Federico-
dc.contributor.authorNewburgh, Laura B.-
dc.contributor.authorNguyen, David V.-
dc.contributor.authorNiemack, Michael D.-
dc.contributor.authorPage, Lyman A.-
dc.contributor.authorSakaguri, Kana-
dc.contributor.authorSakurai, Yuki-
dc.contributor.authorRao, Mayuri Sathyanarayana-
dc.contributor.authorSaunders, Lauren J.-
dc.contributor.authorShroyer, Jordan E.-
dc.contributor.authorSugiyama, Junna-
dc.contributor.authorTajima, Osamu-
dc.contributor.authorTakeuchi, Atsuto-
dc.contributor.authorBua, Refilwe Tanah-
dc.contributor.authorTeply, Grant-
dc.contributor.authorTerasaki, Tomoki-
dc.contributor.authorUllom, Joel N.-
dc.contributor.authorVan Lanen, Jeffrey L.-
dc.contributor.authorVavagiakis, Eve M.-
dc.contributor.authorVissers, Michael R.-
dc.contributor.authorWalters, Liam-
dc.contributor.authorWang, Yuhan-
dc.contributor.authorXu, Zhilei-
dc.contributor.authorYamada, Kyohei-
dc.contributor.authorZheng, Kaiwen-
dc.date.accessioned2024-10-23T05:54:28Z-
dc.date.available2024-10-23T05:54:28Z-
dc.date.issued2024-10-01-
dc.identifier.citationThe Astrophysical Journal Supplement Series, 2024, Vol. 274, p33en_US
dc.identifier.urihttp://hdl.handle.net/2289/8346-
dc.descriptionOpen Accessen_US
dc.description.abstractThe Simons Observatory (SO) is a cosmic microwave background survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands between 27 and 280 GHz to search for primordial B-modes to a sensitivity of σ(r) = 0.002, with quantified systematic errors well below this value. Each SAT is a self-contained cryogenic telescope with a 35° field of view, 42 cm diameter optical aperture, 40 K half-wave plate, 1 K refractive optics, and <0.1 K focal plane that holds >12,000 transition edge sensor detectors. We describe the nominal design of the SATs and present details about the integration and testing for one operating at 93 and 145 GHz.en_US
dc.language.isoenen_US
dc.publisherIOP Publishing Ltd.en_US
dc.relation.urihttp://arxiv.org/abs/2405.05550en_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2024ApJS..274...33G/abstracten_US
dc.relation.urihttps://doi.org/10.3847/1538-4365/ad64c9en_US
dc.relation.urihttps://inspirehep.net/literature/2784799en_US
dc.rights2024 The Author(s)en_US
dc.titleThe Simons Observatory: Design, Integration, and Testing of the Small Aperture Telescopesen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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