The South Pole Telescope SZ-Receiver Detectors

We will discuss the design, fabrication, and testing of a 960-element TES array installed on the new 10 meter South Pole Telescope (SPT). This array is designed to survey for galaxy clusters using the Sunyaev-Zel'dovich (SZ) effect, which is the inverse-Compton scattering of Cosmic Microwave Ba...

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Bibliographic Details
Published in:IEEE transactions on applied superconductivity Vol. 19; no. 3; pp. 517 - 519
Main Authors: Shirokoff, E., Benson, B.A., Bleem, L.E., Chang, C.L., Hsiao-Mei Cho, Crites, A.T., Dobbs, M.A., Holzapfel, W.L., Lanting, T., Lee, A.T., Lueker, M., Mehl, J., Plagge, T., Spieler, H.G., Vieira, J.D.
Format: Journal Article Conference Proceeding
Language:English
Published: New York, NY IEEE 01-06-2009
Institute of Electrical and Electronics Engineers
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
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Summary:We will discuss the design, fabrication, and testing of a 960-element TES array installed on the new 10 meter South Pole Telescope (SPT). This array is designed to survey for galaxy clusters using the Sunyaev-Zel'dovich (SZ) effect, which is the inverse-Compton scattering of Cosmic Microwave Background photons by plasma bound to clusters of galaxies. The SPT bolometer array consists of fully lithographed spider-web absorbers fabricated on adhesive-bonded silicon wafers with an embedded metal back plane. The absorbers are connected to aluminum-titanium bilayer TESs with a transition temperature of approximately 550 mK. Additional normal-metal features adjust the devices' thermal properties to suit our readout system and observational strategy. The focal plane is cooled using a commercial, closed cycle, pulse-tube refrigerator and a three-stage helium sorption refrigerator with a 250 mK base temperature.
Bibliography:ObjectType-Article-2
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ISSN:1051-8223
1558-2515
DOI:10.1109/TASC.2009.2018229