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Paper detail

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

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.

preprint2014arXivOpen access
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
astro-ph.IM
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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

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