THE AMIBA PROJECT

The Array for Microwave Background Anisotropy is a 7-element interferometer to be sited on Mauna Loa, Hawaii. The seven 1.2m telescopes are mounted on a 6-meter platform, and operates at 3mm wavelength. At the time of this meeting, the telescope is under construction at the Vertex factory in Germany...

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Veröffentlicht in:	Modern physics letters A 2004-05, Vol.19 (13n16), p.993-1000
Hauptverfasser:	HO, PAUL T. P., CHEN, MINGTANG, CHIUEH, TZI-DAR, CHIUEH, TZIHONG, CHU, TAH-HSIUNG, JIANG, HOMIN, KOCH, PATRICK, KUBO, DEREK, LI, CHAO-TE, KESTEVEN, MICHAEL, LIN, KAI-YANG, LIU, GUO-CHIN, LO, KWOK-YUNG, MA, CHENG-JIUN, MARTIN, ROBERT N., NG, KIN-WANG, NISHIOKA, HIROAKI, PATT, FERDINAND, PETERSON, JEFFREY B., RAFFIN, PHILIPPE, WANG, HUEI, HWANG, YUH-JING, UMETSU, KEIICHI, WU, JIUN-HUEI PROTY
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic Microwave Background Cosmology
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	The Array for Microwave Background Anisotropy is a 7-element interferometer to be sited on Mauna Loa, Hawaii. The seven 1.2m telescopes are mounted on a 6-meter platform, and operates at 3mm wavelength. At the time of this meeting, the telescope is under construction at the Vertex factory in Germany. It is due to be delivered in the middle of 2004. A 2-element prototype instrument has already been deployed to Mauna Loa where initial tests are underway.
ISSN:	0217-7323 1793-6632
DOI:	10.1142/S0217732304014276