The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters

John W. Appel,Aamir Ali,Mandana Amiri,Derek Araujo,Charles L. Bennett, Fletcher Boone,Manwei Chan,Hsiao-Mei Cho,David T. Chuss,Felipe Colazo,Erik Crowe,Kevin Denis,Rolando Dunner,Joseph Eimer,Thomas Essinger-Hileman, Dominik Gothe,Mark Halpern,Kathleen Harrington,Gene Hilton,Gary F. Hinshaw,Caroline Huang,Kent Irwin,Glenn Jones,John Karakla,Alan J. Kogut,David Larson,Michele Limon,Lindsay Lowry,Tobias Marriage, Nicholas Mehrle,Amber D. Miller,Nathan Miller, Samuel H. Moseleyb, Giles Novakh, Carl Reintsemad, Karwan Rostemab, Thomas Stevensonb,Deborah Towner,Kongpop U-Yen,Emily Wagner,Duncan Watts,Edward Wollack,Zhilei Xu,Lingzhen Zeng

MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VII（2014）

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摘要

The Cosmology Large Angular Scale Surveyor (CLASS) experiment aims to map the polarization of the Cosmic Microwave Background (CMB) at angular scales larger than a few degrees. Operating from Cerro Toco in the Atacama Desert of Chile, it will observe over 65% of the sky at 38, 93, 148, and 217 GHz. In this paper we discuss the design, construction, and characterization of the CLASS 38 GHz detector focal plane, the first ever Q-band bolometric polarimeter array.

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关键词

CMB, Polarimeter, Bolometer, TES

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