Probing the Epoch of Reionization with 21CMA: Status and Prospects

Details Probing the Epoch of Reionization with 21CMA: Status and Prospects Probing the Epoch of Reionization with 21CMA: Status and Prospects

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21322605w&link_type=abstract

American Astronomical Society, AAS Meeting #213, #226.05; Bulletin of the American Astronomical Society, Vol. 41, p.474

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21CMA is an interferometric radio array dedicated to measurement of the redshifted 21 cm emission signatures of neutral hygrogen against CMB in the epoch of reionization. The array, located in Xinjiang, west China, consists of 81 pods with a total of 10287 log periodic antennas. It operates at frequencies from 50 to 200 MHz, covering a reshishift range of 6-27. In this talk, I will present the motivation, construction and performance of 21CMA and its impact on our undestanding of cosmic evolution of reionization.

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