October 6, 2021 Poster Open Access

Smith, Leigh C.

DCAT Export

<?xml version='1.0' encoding='utf-8'?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:adms="http://www.w3.org/ns/adms#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dct="http://purl.org/dc/terms/" xmlns:dctype="http://purl.org/dc/dcmitype/" xmlns:dcat="http://www.w3.org/ns/dcat#" xmlns:duv="http://www.w3.org/ns/duv#" xmlns:foaf="http://xmlns.com/foaf/0.1/" xmlns:frapo="http://purl.org/cerif/frapo/" xmlns:geo="http://www.w3.org/2003/01/geo/wgs84_pos#" xmlns:gsp="http://www.opengis.net/ont/geosparql#" xmlns:locn="http://www.w3.org/ns/locn#" xmlns:org="http://www.w3.org/ns/org#" xmlns:owl="http://www.w3.org/2002/07/owl#" xmlns:prov="http://www.w3.org/ns/prov#" xmlns:rdfs="http://www.w3.org/2000/01/rdf-schema#" xmlns:schema="http://schema.org/" xmlns:skos="http://www.w3.org/2004/02/skos/core#" xmlns:vcard="http://www.w3.org/2006/vcard/ns#" xmlns:wdrs="http://www.w3.org/2007/05/powder-s#">
  <rdf:Description rdf:about="https://doi.org/10.5281/zenodo.5552616">
    <rdf:type rdf:resource="http://www.w3.org/ns/dcat#Dataset"/>
    <dct:type rdf:resource="http://purl.org/dc/dcmitype/Text"/>
    <dct:identifier rdf:datatype="http://www.w3.org/2001/XMLSchema#anyURI">https://doi.org/10.5281/zenodo.5552616</dct:identifier>
    <foaf:page rdf:resource="https://doi.org/10.5281/zenodo.5552616"/>
    <dct:creator>
      <rdf:Description rdf:about="http://orcid.org/0000-0002-3259-2771">
        <rdf:type rdf:resource="http://xmlns.com/foaf/0.1/Agent"/>
        <dct:identifier rdf:datatype="http://www.w3.org/2001/XMLSchema#string">0000-0002-3259-2771</dct:identifier>
        <foaf:name>Smith, Leigh C.</foaf:name>
        <foaf:givenName>Leigh C.</foaf:givenName>
        <foaf:familyName>Smith</foaf:familyName>
        <org:memberOf>
          <foaf:Organization>
            <foaf:name>University of Cambridge</foaf:name>
          </foaf:Organization>
        </org:memberOf>
      </rdf:Description>
    </dct:creator>
    <dct:title>The detectability of Saturn-like exoplanetary rings by PLATO</dct:title>
    <dct:publisher>
      <foaf:Agent>
        <foaf:name>Zenodo</foaf:name>
      </foaf:Agent>
    </dct:publisher>
    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#gYear">2021</dct:issued>
    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#date">2021-10-06</dct:issued>
    <owl:sameAs rdf:resource="https://zenodo.org/record/5552616"/>
    <adms:identifier>
      <adms:Identifier>
        <skos:notation rdf:datatype="http://www.w3.org/2001/XMLSchema#anyURI">https://zenodo.org/record/5552616</skos:notation>
        <adms:schemeAgency>url</adms:schemeAgency>
      </adms:Identifier>
    </adms:identifier>
    <dct:isVersionOf rdf:resource="https://doi.org/10.5281/zenodo.5552615"/>
    <dct:isPartOf rdf:resource="https://zenodo.org/communities/plato2021"/>
    <dct:description>&lt;p&gt;Abstract: All long-period gas giant planets (and at least one minor planet) in the Solar System host rings. PLATO&amp;#39;s superb photometric sensitivity and long dwell time make it ideal for study of the (presumed) population of similar such exoplanets. Inspired by the work of Barnes and Fortney (2004), I consider the detectability of Saturn-like exoplanetary rings by PLATO. I introduce a software package in development, capable of simulating the transits of exoplanets hosting complex ring systems, and which can take advantage of the parallel processing power of GPUs. Finally, I highlight the potential impact on extracted planetary radii, and by extension densities, under the assumption of no rings.&lt;/p&gt;</dct:description>
    <dct:accessRights rdf:resource="http://publications.europa.eu/resource/authority/access-right/PUBLIC"/>
    <dct:accessRights>
      <dct:RightsStatement rdf:about="info:eu-repo/semantics/openAccess">
        <rdfs:label>Open Access</rdfs:label>
      </dct:RightsStatement>
    </dct:accessRights>
    <dcat:distribution>
      <dcat:Distribution>
        <dct:license rdf:resource="https://creativecommons.org/licenses/by/4.0/legalcode"/>
        <dcat:accessURL rdf:resource="https://doi.org/10.5281/zenodo.5552616"/>
      </dcat:Distribution>
    </dcat:distribution>
    <dcat:distribution>
      <dcat:Distribution>
        <dcat:accessURL rdf:resource="https://doi.org/10.5281/zenodo.5552616"/>
        <dcat:byteSize>1128642</dcat:byteSize>
        <dcat:downloadURL rdf:resource="https://zenodo.org/record/5552616/files/The detectability of Saturn-like exoplanetary rings by PLATO.pdf"/>
        <dcat:mediaType>application/pdf</dcat:mediaType>
      </dcat:Distribution>
    </dcat:distribution>
  </rdf:Description>
</rdf:RDF>