[{"data": {"name": "Three observational differences for binary black holes detections with second- and third-generation gravitational-wave detectors", "@type": "ScholarlyArticle", "genre": "journal-article", "author": [{"name": "Salvatore Vitale", "@type": "Person"}], "license": "publisher-specific, author manuscript: http://link.aps.org/licenses/aps-default-accepted-manuscript-license", "@context": "http://schema.org/", "encoding": [{"@type": "MediaObject", "contentUrl": "https://link.aps.org/accepted/10.1103/PhysRevD.94.121501", "encodingFormat": "application/pdf"}], "publisher": {"name": "American Physical Society (APS)", "@type": "Organization"}, "identifier": [{"@type": "PropertyValue", "value": "10.1103/physrevd.94.121501", "propertyID": "DOI"}, {"@type": "PropertyValue", "value": "CChJu3cAy8LUt-CTY6kEGEdgRie-CDbCiytwrXhoH-CRdzVFSBUsqfG", "propertyID": "ISCC"}], "datePublished": "2016-12-15"}, "schema": "schema.org", "mediatype": "application/ld+json"}]