@prefix dcat: <http://www.w3.org/ns/dcat#> .
@prefix dct: <http://purl.org/dc/terms/> .
@prefix foaf: <http://xmlns.com/foaf/0.1/> .
@prefix org: <http://www.w3.org/ns/org#> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix vcard: <http://www.w3.org/2006/vcard/ns#> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<https://data.nasa.gov/dataset/38d3043b-8fd0-499e-8381-198a70505918> a dcat:Dataset ;
    dct:description "Numerically-generated  gravitational waveforms for circular inspiral into Kerr black holes. These waveforms were developed using Scott Hughes' black hole perturbation theory code (the 'Teukolsky code')." ;
    dct:identifier "NASA-0000021" ;
    dct:issued "2018-06-25"^^xsd:date ;
    dct:modified "2024-08-16"^^xsd:date ;
    dct:publisher <https://data.nasa.gov/organization/dbb294e4-8597-44f5-aaf4-c0baac12cdbc> ;
    dct:title "Waveform Catalog, Extreme Mass Ratio Binary (Capture)" ;
    dcat:contactPoint [ a vcard:Organization ;
            vcard:fn "Scott Hughes" ;
            vcard:hasEmail <mailto:sahughes@mit.edu> ] ;
    dcat:distribution <https://data.nasa.gov/dataset/38d3043b-8fd0-499e-8381-198a70505918/resource/13b47394-7f5a-417a-9728-ab1f53e9c1ac> ;
    dcat:keyword "astronomy",
        "binary",
        "black-hole",
        "gravitational-waves",
        "ligo",
        "neutron-stars",
        "space-science" .

<https://data.nasa.gov/dataset/38d3043b-8fd0-499e-8381-198a70505918/resource/13b47394-7f5a-417a-9728-ab1f53e9c1ac> a dcat:Distribution ;
    dct:format "HTML" ;
    dct:identifier "13b47394-7f5a-417a-9728-ab1f53e9c1ac" ;
    dct:issued "2025-03-31T17:18:11.150227"^^xsd:dateTime ;
    dct:modified "2025-03-31T17:18:11.128831"^^xsd:dateTime ;
    dcat:accessURL <https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#emrbc> ;
    dcat:mediaType "text/html" .

<https://data.nasa.gov/organization/dbb294e4-8597-44f5-aaf4-c0baac12cdbc> a org:Organization ;
    skos:prefLabel "NASA" ;
    foaf:name "NASA" .

