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2014-08-20
The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters
John W. AppelAamir AliMandana AmiriDerek AraujoCharles L. BennettFletcher BooneManwei ChanHsiao-Mei ChoDavid T. ChussFelipe ColazoErik CroweKevin DenisRolando DunnerJoseph EimerThomas Essinger-HilemanDominik GotheMark HalpernKathleen HarringtonGene HiltonGary F. HinshawCaroline HuangKent IrwinGlenn JonesJohn KaraklaAlan J. KogutDavid LarsonMichele LimonLindsay LowryTobias MarriageNicholas MehrleAmber D. MillerNathan MillerSamuel H. MoseleybGiles NovakhCarl ReintsemadKarwan RostemabThomas StevensonbDeborah TownerKongpop U-YenEmily WagnerDuncan WattsEdward WollackZhilei XuLingzhen Zeng
文献摘要
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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