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

hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorBAUDRY, Alain
dc.contributor.authorWEBBER, J.
dc.date.issued2011
dc.date.conference2011
dc.description.abstractEnWe 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.
dc.language.isoen
dc.source.titleGeneral Assembly and Scientific Symposium, 2011 XXXth URSI
dc.title.enThe ALMA 64-antenna Correlator: Main Technical Features and Science Modes
dc.typeCommunication dans un congrès
dc.identifier.doi10.1109/URSIGASS.2011.6051253
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page1-4
bordeaux.countryTR
bordeaux.title.proceedingGeneral Assembly and Scientific Symposium, 2011 XXXth URSI
bordeaux.conference.cityIstanbul
bordeaux.peerReviewedoui
hal.identifierhal-00677337
hal.version1
hal.invitedoui
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00677337v1
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