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    National Tsing Hua University Institutional Repository > 理學院 > 天文研究所 > 會議論文  >  Initial operation of the array for microwave background anisotropy (AMiBA)

    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/53746

    Title: Initial operation of the array for microwave background anisotropy (AMiBA)
    Authors: Li, Chao-Te;Han, Chih-Chiang;Chen, Ming-Tang;Huang, Yau-De;Jiang, Homin;Hwang, Yuh-Jing;Chang, Su-Wei;Chang, Shu-Hao;Martin-Cocher, Pierre;Chang, Chia-Hao;Chen, Chung-Cheng;Wilson, Warwick;Umetsu, Keiichi;Lin, Kai-Yang;Koch, Patrick;Liu, Guo-Chin;Nishioka, Hiroaki;Ho, Paul T. P.
    教師: 賀曾樸
    Date: 2006
    Relation: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III.,Proceedings of the SPIE, Volume 6275, pp. 62751I (2006)
    Keywords: Initial operation
    microwave background anisotropy
    Abstract: AMiBA, as a dual-polarization 86-102 GHz interferometer array, is designed to measure the power spectrum of fluctuations in the cosmic microwave background (CMB) radiation, and to detect the high-redshift clusters of galaxies via the Sunyaev-Zel'dovich Effect (SZE). The operation of AMiBA is about to begin after installation of the first two receivers and correlators onto the 6-meter diameter platform by the end of 2005. The initial setup of the array will consist of 7 antennas with 60 cm diameter reflectors in a hexagonal configuration, aiming at multipoles l ~ 3000. Signals from receivers are cross-correlated in analog lag correlators. The initial operation will focus on characterizing the systematics by observing various known objects on the sky. The expansion to 13 elements with larger dishes will commence once the 7-element array testing is completed.
    URI: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/53746
    Appears in Collections:[天文研究所] 會議論文

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