Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q1558495> ?p ?o }
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- Q1558495 subject Q7009590.
- Q1558495 subject Q8965739.
- Q1558495 abstract "PSR J2007+2722 is a 40.8-hertz isolated pulsar in the Vulpecula constellation, 5.3 kpc (17,000 ly) distant in the plane of the Galaxy, and is most likely a disrupted recycled pulsar (DRP).J2007+2722 was found on data taken by the Arecibo radio telescope in February 2007, and analyzed by volunteers Chris and Helen Colvin (Ames, Iowa,USA) and Daniel Gebhardt (Universität Mainz, Musikinformatik, Germany) via the distributed computing project Einstein@Home.".
- Q1558495 wikiPageWikiLink Q10519.
- Q1558495 wikiPageWikiLink Q1060565.
- Q1558495 wikiPageWikiLink Q12129.
- Q1558495 wikiPageWikiLink Q180634.
- Q1558495 wikiPageWikiLink Q39379.
- Q1558495 wikiPageWikiLink Q4360.
- Q1558495 wikiPageWikiLink Q44547.
- Q1558495 wikiPageWikiLink Q531.
- Q1558495 wikiPageWikiLink Q7009590.
- Q1558495 wikiPageWikiLink Q8965739.
- Q1558495 type Place.
- Q1558495 type CelestialBody.
- Q1558495 type Location.
- Q1558495 type Place.
- Q1558495 type Star.
- Q1558495 type Thing.
- Q1558495 comment "PSR J2007+2722 is a 40.8-hertz isolated pulsar in the Vulpecula constellation, 5.3 kpc (17,000 ly) distant in the plane of the Galaxy, and is most likely a disrupted recycled pulsar (DRP).J2007+2722 was found on data taken by the Arecibo radio telescope in February 2007, and analyzed by volunteers Chris and Helen Colvin (Ames, Iowa,USA) and Daniel Gebhardt (Universität Mainz, Musikinformatik, Germany) via the distributed computing project Einstein@Home.".
- Q1558495 label "PSR J2007+2722".
- Q1558495 name "PSR J2007+2722".