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Search: WFRF:(Connors R. M. T.) > (2020-2024) > The Simons Observat...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005106naa a2201069 4500
001oai:DiVA.org:su-199549
003SwePub
008211214s2021 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1995492 URI
024a https://doi.org/10.3847/1538-4357/ac22322 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a McCarrick, Heather4 aut
2451 0a The Simons Observatory Microwave SQUID Multiplexing Detector Module Design
264 c 2021-11-18
264 1b American Astronomical Society,c 2021
338 a print2 rdacarrier
520 a Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever larger focal planes. High multiplexing factors reduce the thermal loading on the cryogenic receivers and simplify their design. We present the design of focal-plane modules with an order of magnitude higher multiplexing factor than has previously been achieved with TES bolometers. We focus on the novel cold readout component, which employs microwave SQUID multiplexing (μmux). Simons Observatory will use 49 modules containing 70,000 bolometers to make exquisitely sensitive measurements of the CMB. We validate the focal-plane module design, presenting measurements of the readout component with and without a prototype detector array of 1728 polarization-sensitive bolometers coupled to feedhorns. The readout component achieves a 95% yield and a 910 multiplexing factor. The median white noise of each readout channel is 65 pA √Hz . This impacts the projected SO mapping speed by <8%, which is less than is assumed in the sensitivity projections. The results validate the full functionality of the module. We discuss the measured performance in the context of SO science requirements, which are exceeded.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a Cosmic microwave background radiation
653 a CMBR detectors
653 a Astronomical instrumentation
653 a Cosmology
700a Healy, Erin4 aut
700a Ahmed, Zeeshan4 aut
700a Arnold, Kam4 aut
700a Atkins, Zachary4 aut
700a Austermann, Jason E.4 aut
700a Bhandarkar, Tanay4 aut
700a Beall, James A.4 aut
700a Bruno, Sarah Marie4 aut
700a Choi, Steve K.4 aut
700a Connors, Jake4 aut
700a Cothard, Nicholas F.4 aut
700a Crowley, Kevin D.4 aut
700a Dicker, Simon4 aut
700a Dober, Bradley4 aut
700a Duell, Cody J.4 aut
700a Duff, Shannon M.4 aut
700a Dutcher, Daniel4 aut
700a Frisch, Josef C.4 aut
700a Galitzki, Nicholas4 aut
700a Gralla, Megan B.4 aut
700a Gudmundsson, Jon E.u Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Fysikum4 aut0 (Swepub:su)jgudm
700a Henderson, Shawn W.4 aut
700a Hilton, Gene C.4 aut
700a Ho, Shuay-Pwu Patty4 aut
700a Huber, Zachary B.4 aut
700a Hubmayr, Johannes4 aut
700a Iuliano, Jeffrey4 aut
700a Johnson, Bradley R.4 aut
700a Kofman, Anna M.4 aut
700a Kusaka, Akito4 aut
700a Lashner, Jack4 aut
700a Lee, Adrian T.4 aut
700a Li, Yaqiong4 aut
700a Link, Michael J.4 aut
700a Lucas, Tammy J.4 aut
700a Lungu, Marius4 aut
700a Mates, J. A. B.4 aut
700a McMahon, Jeffrey J.4 aut
700a Niemack, Michael D.4 aut
700a Orlowski-Scherer, John4 aut
700a Seibert, Joseph4 aut
700a Silva-Feaver, Maximiliano4 aut
700a Simon, Sara M.4 aut
700a Staggs, Suzanne4 aut
700a Suzuki, Aritoki4 aut
700a Terasaki, Tomoki4 aut
700a Ullom, Joel N.4 aut
700a Vavagiakis, Eve M.4 aut
700a Vale, Leila R.4 aut
700a Van Lanen, Jeff4 aut
700a Vissers, Michael R.4 aut
700a Wang, Yuhan4 aut
700a Wollack, Edward J.4 aut
700a Xu, Zhilei4 aut
700a Young, Edward4 aut
700a Yu, Cyndia4 aut
700a Zheng, Kaiwen4 aut
700a Zhu, Ningfeng4 aut
700a Thornton, Robert4 aut
710a Stockholms universitetb Oskar Klein-centrum för kosmopartikelfysik (OKC)4 org
773t Astrophysical Journald : American Astronomical Societyg 922:1q 922:1x 0004-637Xx 1538-4357
856u https://arxiv.org/abs/2106.14797y arXiv:2106.14797
856u http://arxiv.org/pdf/2106.14797
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-199549
8564 8u https://doi.org/10.3847/1538-4357/ac2232

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