The ALMA 64-antenna Correlator: Main Technical Features and Science Modes - Archive ouverte HAL
Communication Dans Un Congrès Année : 2011

The ALMA 64-antenna Correlator: Main Technical Features and Science Modes

Alain Baudry
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FORMATION STELLAIRE 2011
J. Webber
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Résumé

We present the main features of the Atacama Large Millimeter/submm Array (ALMA) 64-antenna correlator sub-system and describe some original parts of the design. All correlator parts have been constructed, 3 quadrants are delivered to the 5000-m high site and 2 have been commissioned for ALMA Early Science. The basic observing modes are described and the huge flexibility embedded in the design is underlined.

Domaines

Astrophysique stellaire et solaire [astro-ph.SR] Astrophysique stellaire et solaire [astro-ph.SR]

Marie-Paule Pomies  : Connectez-vous pour contacter le contributeur

https://hal.science/hal-00677337

Soumis le : jeudi 8 mars 2012-08:09:42

Dernière modification le : mardi 3 décembre 2024-14:32:04

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Dates et versions

hal-00677337 , version 1 (08-03-2012)

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Citer

Alain Baudry, J. Webber. The ALMA 64-antenna Correlator: Main Technical Features and Science Modes. General Assembly and Scientific Symposium, 2011 XXXth URSI, 2011, Istanbul, Turkey. pp.1-4, ⟨10.1109/URSIGASS.2011.6051253⟩. ⟨hal-00677337⟩

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