| Autor: |
K. Y. Lo, Keiichi Umetsu, Jeremy Lim, Pablo Altimirano, Michael Kesteven, Huei Wang, Yen Shen Lin, Mark Birkinshaw, Yuh-Jing Hwang, Sandor M. Molnar, Hiroaki Nishioka, Jiun-Huei Proty Wu, Ferdinand Patt, Derek Kubo, W. Y. Pauchy Hwang, Tah-Hsiung Chu, Tzihong Chiueh, Jeffrey B. Peterson, Pierre Martin-Cocher, Homin Jiang, Chi Wei Huang, Patrick M. Koch, Kai-Yang Lin, Katy Lancaster, Fabi Romano, Guo-Chin Liu, Ming-Tang Chen, Robert N. Martin, Chan Gyung Park, Paul T. P. Ho, Chao-Te Li, Cheng Jiun Ma, Su-Wei Chang, Yao De Huang, Kin-Wang Ng, Tzi Dar Chiueh, Philippe Raffin, Ke Jun Chen, Haida Liang, Chih Chiang Han, Yao Wei Liao, Fu-Cheng Wang, Cha Hao Chang |
| Rok vydání: |
2008 |
| Předmět: |
|
| Zdroj: |
Modern Physics Letters A. 23:1243-1251 |
| ISSN: |
1793-6632
0217-7323 |
| DOI: |
10.1142/s021773230802762x |
| Popis: |
The Array for Microwave Background Anisotropy is a 7-element interferometer sited on Mauna Loa, Hawaii. The seven 60cm telescopes are mounted on a 6-meter platform, and operates at 3mm wavelength. In October 2006, the telescope was officially dedicated and renamed as the Y. T. Lee AMiBA. During 2007, scientific operations have begun, after a long process of calibration and testing. At the time of this meeting, six clusters of galaxies have been detected and mapped via the inverse Compton scattering of the Cosmic Microwave Background radiation, also known as the Sunyaev-Zel'dovich Effect. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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