Statements (53)
Predicate | Object |
---|---|
gptkbp:instanceOf |
Radio Observatory
|
gptkbp:availableFormats |
FITS
|
gptkbp:collaborations |
gptkb:LOFAR
ALMA Event Horizon Telescope SKA |
gptkbp:completed |
1980
|
gptkbp:constructionMaterial |
$78 million
|
gptkbp:dataUsage |
Open data policy
Very Large Array Data Archive Digital_signal_processing |
gptkbp:educationalPrograms |
Outreach_and_Tours
|
gptkbp:engineConfiguration |
A, B, C, D
|
gptkbp:firstAwarded |
1980
|
gptkbp:firstMatch |
1980-10-01
|
gptkbp:frequency |
1 to 50 GHz
|
gptkbp:futurePlans |
Increased sensitivity
Continued upgrades Expanded frequency coverage |
gptkbp:hasFunding |
gptkb:National_Science_Foundation
|
https://www.w3.org/2000/01/rdf-schema#label |
VLA
|
gptkbp:location |
gptkb:New_Mexico
|
gptkbp:maintenance |
Regular inspections
|
gptkbp:majorIndustry |
Expanded Very Large Array
|
gptkbp:notableEvent |
Dark Energy Survey
Galactic Center Survey Hubble_Space_Telescope_Follow-up |
gptkbp:notableFeature |
Quasars
Cosmic Microwave Background Pulsars |
gptkbp:numberOfEpisodes |
27
|
gptkbp:officialResidence |
High-resolution imaging
Continuum_and_Spectral |
gptkbp:operatedBy |
gptkb:National_Radio_Astronomy_Observatory
|
gptkbp:partOf |
gptkb:National_Radio_Astronomy_Observatory
|
gptkbp:powers |
Electricity
|
gptkbp:publicAccess |
Yes
|
gptkbp:recordings |
0.1 arcseconds
|
gptkbp:researchField |
Astrophysics
|
gptkbp:researchInterest |
Numerous peer-reviewed articles
Understanding galaxy formation Significant contributions to cosmology Studying exoplanets |
gptkbp:rotorDiameter |
25 meters
22,000 meters |
gptkbp:scientificName |
Global
|
gptkbp:technology |
Data analysis software
Radio frequency technology Interferometry techniques |
gptkbp:timePeriod |
Proposal-based
|
gptkbp:type |
Interferometer
|
gptkbp:usedFor |
Radio Astronomy
|
gptkbp:website |
https://public.nrao.edu/vla/
|