Antenna-Coupled TES Bolometer Arrays for CMB Polarimetry

被引:22
|
作者
Kuo, C. L. [1 ,2 ,3 ]
Bock, J. J. [3 ,4 ]
Bonetti, J. A. [4 ]
Brevik, J. [3 ]
Chattopadthyay, G. [4 ]
Day, P. K. [4 ]
Golwala, S. [1 ,3 ]
Kenyon, M. [4 ]
Lange, A. E. [3 ,4 ]
LeDuc, H. G. [4 ]
Nguyen, H. [4 ]
Ogburn, R. W. [3 ]
Orlando, A. [3 ]
Transgrud, A. [3 ]
Turner, A. [4 ]
Wang, G. [3 ,5 ]
Zmuidzinas, J. [3 ,4 ]
机构
[1] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[2] Stanford Linear Accelerator Ctr, Menlo Pk, CA 94025 USA
[3] CALTECH, Pasadena, CA 91125 USA
[4] Jet Prop Lab, Pasadena, CA 91109 USA
[5] Argonne Natl Lab, Argonne, IL 60439 USA
关键词
cosmic microwave background; polarization; millimeter wave instrumentation;
D O I
10.1117/12.788588
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe the design and performance of polarization selective antenna-coupled TES arrays that will be used in several upcoming Cosmic Microwave Background (CMB) experiments: SPIDER, BICEP-2/SPUD. The fully lithographic polarimeter arrays utilize planar phased-antennas for collimation (F/4 beam) and microstrip filters for band definition (25% bandwidth). These devices demonstrate high optical efficiency, excellent beam shapes, and well-defined spectral bands. The dual-polarization antennas provide well-matched beams and low cross polarization response, both important for high-fidelity polarization measurements. These devices have so far been developed for the 100 GHz and 150 GHz bands, two premier millimeter-wave atmospheric windows for CMB observations. In the near future, the flexible microstrip-coupled architecture can provide photon noise-limited detection for the entire frequency range of the CMBPOL mission. This paper is a summary of the progress we have made since the 2006 SPIE meeting in Orlando, FL.
引用
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页数:14
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