ConferencePaper ISI SCOPUS
29TH INTERNATIONAL CONFERENCE ON OPTICAL FIBER SENSORS  (2014)

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

Appel J.W.; Ali A.; Amiri M.; Araujo D.; Bennett C.L.; Boone F.; Chan, MW; Cho H.M.; Chuss D.T.; Colazo F.; Crowe E.; Denis K.; Eimer J.; Essinger-Hileman T.; Gothe D.; et. al.

Keywords: cmb, tes, bolometer, polarimeter

Abstract

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.

Más información

Título según WOS: The Cosmology Large Angular Scale Surveyor (CLASS): 38-GHz detector array of bolometric polarimeters
Título según SCOPUS: The cosmology large angular scale surveyor (CLASS): 38-GHz detector array of bolometric polarimeters
Título de la Revista: 29TH INTERNATIONAL CONFERENCE ON OPTICAL FIBER SENSORS
Volumen: 9153
Editorial: SPIE-INT SOC OPTICAL ENGINEERING
Fecha de publicación: 2014
Idioma: English
DOI:

10.1117/12.2056530
Notas: ISI, SCOPUS