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    題名: The Yuan-Tseh Lee Array for Microwave Background Anisotropy
    作者: Ho, Paul T. P.;Altamirano, Pablo;Chang, Chia-hao;Chang, Shu-hao;Chang, Su-wei;Chen, Chung-cheng;Chen, Ke-jung;Chen, Ming-tang;Han, Chih-chiang;Ho, West M.;Huang, Yau-de;Hwang, Yuh-jing;Ibañez-Romano, Fabiola;Jiang, Homin;Koch, Patrick M.;Kubo, Derek Y.;Li, Chao-te;Lim, Jeremy;Lin, Kai-yang;Liu, Guo-chin;Lo, Kwok-Yung;Ma, Cheng-Jiun;Martin, Robert N.;Martin-Cocher, Pierre;Molnar, Sandor M.;Ng, Kin-Wang;Nishioka, Hiroaki;O'Connell, Kevin E.;Oshiro, Peter;Patt, Ferdinand;Raffin, Philippe;Umetsu, Keiichi;Wei, Tashun;Wu, Jiun-huei Proty;Chiueh, Tzi-dar;Chiueh, Tzihong;Chu, Tah-hsiung;Huang, Chih-wei Locutus;Hwang, W. Y. Pauchy;Liao, Yu-wei;Lien, Chun-hsien;Wang, Fu-cheng;Wang, Huei;Wei, Ray-ming;Yang, Chia-hsiang;Kesteven, Michael;Kingsley, Jeff;Sinclair, Malcolm M.;Wilson, Warwick;Birkinshaw, Mark;Liang, Haida;Lancaster, Katy;Park, Chan-gyung;Pen, Ue-li;Peterson, Jeffrey B.
    貢獻者: 淡江大學物理學系
    關鍵詞: cosmic microwave background;instrumentation: interferometers;telescopes
    日期: 2009-04
    上傳時間: 2010-08-10 15:15:34 (UTC+8)
    出版者: Philadelphia: Institute of Physics Publishing, Inc.
    摘要: The Yuan-Tseh Lee Array for microwave background anisotropy is the first interferometer dedicated to study the cosmic microwave background radiation at 3 mm wavelength. The choice of 3 mm is to minimize the contributions from foreground synchrotron radiation and Galactic dust emission. The initial configuration of seven 0.6 m telescopes mounted on a 6 m hexapod platform was dedicated in 2006 October on Mauna Loa, Hawaii. Scientific operations began with the detection of a number of clusters of galaxies via the thermal Sunyaev-Zel'dovich effect. We compare our data with Subaru weak-lensing data to study the structure of dark matter. We also compare our data with X-ray data to derive the Hubble constant.
    關聯: The Astrophysical Journal 694(2), pp.1610-1618
    DOI: 10.1088/0004-637X/694/2/1610
    顯示於類別:[物理學系暨研究所] 期刊論文

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