The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters
Appel, John W. · Ali, Aamir · Amiri, Mandana · Araujo, Derek · Bennett, Charles L. · Boone, Fletcher · Chan, Manwei · Cho, Hsiao-Mei · Chuss, David T. · Colazo, Felipe · Crowe, Erik · Denis, Kevin · Dunner, Rolando · Eimer, Joseph · Essinger-Hileman, Thomas · Gothe, Dominik · Halpern, Mark · Harrington, Kathleen · Hilton, Gene · Hinshaw, Gary F. · Huang, Caroline · Irwin, Kent · Jones, Glenn · Karakla, John · Kogut, Alan J. · Larson, David · Limon, Michele · Lowry, Lindsay · Marriage, Tobias · Mehrle, Nicholas · Miller, Amber D. · Miller, Nathan · Moseleyb, Samuel H. · Novakh, Giles · Reintsemad, Carl · Rostemab, Karwan · Stevensonb, Thomas · Towner, Deborah · U-Yen, Kongpop · Wagner, Emily · Watts, Duncan · Wollack, Edward · Xu, Zhilei · Zeng, Lingzhen
Original · EN
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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