@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix dc: <http://purl.org/dc/terms/> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<http://astrothesaurus.org/uat/1768>
  skos:prefLabel "Very long baseline interferometers"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/1769> .

<http://astrothesaurus.org/uat/1346>
  skos:prefLabel "Radio interferometry"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1769> .

<http://astrothesaurus.org/uat/1769>
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie> ;
  dc:modified "2020-11-19T16:55:46.453Z"^^xsd:dateTime, "2020-11-19T16:55:57.216Z"^^xsd:dateTime ;
  skos:prefLabel "Very long baseline interferometry"@en ;
  skos:broader <http://astrothesaurus.org/uat/1346> ;
  skos:altLabel "VLBI"@en, "VLB interferometry"@en ;
  a skos:Concept ;
  skos:definition "A technique in radio interferometry in which the individual telescopes are not directly connected together, but instead make their observations separately with very accurate timings. The data are later sent to a central correlator to be combined. With this technique the individual telescopes can be arbitrarily far apart, and so the technique provides the highest resolution images in astronomy, typically down to a few milliarcseconds."@en ;
  skos:related <http://astrothesaurus.org/uat/1768> ;
  skos:editorialNote [ ] .