The Cosmology Large Angular Scale Surveyor (CLASS) : 38 GHz Detector Array of Bolometric Polarimeters
- Wollack, Edward
- July 23, 2014.
- Physical Description:
- 1 electronic document
- Additional Creators:
- Ali, Aamir, Boone, Fletcher, Bennett, Charles L., Dunner, Rolando, Halpern, Mark, Stevenson, Thomas, Miller, Nathan, Eimer, Joseph, Colazo, Felipe, Amiri, Mandana, Chan, Manwei, Kogut, Alan J.., Harrington, Kathleen, Crowe, Erik, Cho, Hsiao-Mei, Towner, Deborah, U-Yen, Kongpop, Gothe, Dominik, Denis, Kevin, Moseley, Samuel H., Chuss, David T., Appel, John W., Essinger-Hileman, Thomas, and Araujo, Derek
- Restrictions on Access:
- Unclassified, Unlimited, Publicly available. and Free-to-read Unrestricted online access
- 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.
- NASA Technical Reports Server (NTRS) Collection.
- Document ID: 20140017649., GSFC-E-DAA-TN17264., and SPIE Proceedings: CMB Instruments: New Developments I; Volume 9153; 91531J.
- Copyright, Distribution as joint owner in the copyright.
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