Disambiguation evidence for ATA via surface form

"Allen Telescope Array"


As subject (43)

Triples where this entity appears as subject under the label "Allen Telescope Array".

Predicate Object
acronym ATA self-linksurface differs
affiliation SETI Institute research programs
affiliation Radio Astronomy Laboratory at UC Berkeley
surface form: UC Berkeley SETI Research Center
collaborator Radio Astronomy Laboratory at UC Berkeley
constructionStartDate 2004
correlatorType wide-field imaging correlator
country United States of America
surface form: United States
dataProcessing real-time digital signal processing
designFeature large field of view
designFeature modular, expandable array
designFeature simultaneous imaging and SETI observations
designFeature wideband receivers
designedFor radio astronomy
designedFor search for extraterrestrial intelligence
dishDiameter 6.1 meters
firstLightDate 2007
frequencyCoverage approximately 0.5–11.2 GHz
fundedBy Paul Allen
surface form: Paul G. Allen
fundedBy Paul G. Allen Family Foundation
fundingModel public–private partnership
infrastructure fiber-optic data links from antennas to central correlator
initialOperationalAntennas 42
instanceOf SETI instrument
instanceOf interferometric array
instanceOf radio telescope array
locatedAt Hat Creek Radio Observatory
locatedIn California, United States
surface form: California
mountType alt-azimuth
namedAfter Paul Allen
surface form: Paul G. Allen
notableFor first radio telescope built specifically for SETI and radio astronomy together
observatoryCode ATA self-linksurface differs
operator SETI Institute
operator University of California, Berkeley
originalDesignNumberOfAntennas 350
primaryUse SETI observations
primaryUse astronomical observations
scientificGoal detect narrowband radio signals from extraterrestrial civilizations
scientificGoal study radio emission from galaxies
scientificGoal study radio emission from planets
scientificGoal study radio emission from stars
scientificGoal study transient radio sources
scientificGoal survey large areas of the sky
telescopeType LNSD array