{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1362262944199957504.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1051/0004-6361/201219880"}},{"identifier":{"@type":"URI","@value":"http://www.aanda.org/10.1051/0004-6361/201219880/pdf"}}],"dc:title":[{"@value":"GOODS-<i>Herschel</i>: radio-excess signature of hidden AGN activity in distant star-forming galaxies"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382262944199957514","@type":"Researcher","foaf:name":[{"@value":"A. Del Moro"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957520","@type":"Researcher","foaf:name":[{"@value":"D. M. Alexander"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957517","@type":"Researcher","foaf:name":[{"@value":"J. R. Mullaney"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957635","@type":"Researcher","foaf:name":[{"@value":"E. Daddi"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957504","@type":"Researcher","foaf:name":[{"@value":"M. Pannella"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957519","@type":"Researcher","foaf:name":[{"@value":"F. E. Bauer"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957523","@type":"Researcher","foaf:name":[{"@value":"A. Pope"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957509","@type":"Researcher","foaf:name":[{"@value":"M. Dickinson"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957521","@type":"Researcher","foaf:name":[{"@value":"D. Elbaz"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957633","@type":"Researcher","foaf:name":[{"@value":"P. D. Barthel"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957518","@type":"Researcher","foaf:name":[{"@value":"M. A. Garrett"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957522","@type":"Researcher","foaf:name":[{"@value":"W. N. Brandt"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957506","@type":"Researcher","foaf:name":[{"@value":"V. Charmandaris"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957516","@type":"Researcher","foaf:name":[{"@value":"R. R. Chary"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957508","@type":"Researcher","foaf:name":[{"@value":"K. Dasyra"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957505","@type":"Researcher","foaf:name":[{"@value":"R. Gilli"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957632","@type":"Researcher","foaf:name":[{"@value":"R. C. Hickox"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957510","@type":"Researcher","foaf:name":[{"@value":"H. S. Hwang"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957634","@type":"Researcher","foaf:name":[{"@value":"R. J. Ivison"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957513","@type":"Researcher","foaf:name":[{"@value":"S. Juneau"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957524","@type":"Researcher","foaf:name":[{"@value":"E. Le Floc’h"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957511","@type":"Researcher","foaf:name":[{"@value":"B. Luo"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957507","@type":"Researcher","foaf:name":[{"@value":"G. E. Morrison"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957515","@type":"Researcher","foaf:name":[{"@value":"E. Rovilos"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957636","@type":"Researcher","foaf:name":[{"@value":"M. T. Sargent"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944199957512","@type":"Researcher","foaf:name":[{"@value":"Y. Q. Xue"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00046361"},{"@type":"EISSN","@value":"14320746"}],"prism:publicationName":[{"@value":"Astronomy & Astrophysics"}],"dc:publisher":[{"@value":"EDP Sciences"}],"prism:publicationDate":"2012-12-18","prism:volume":"549","prism:startingPage":"A59"},"reviewed":"false","url":[{"@id":"http://www.aanda.org/10.1051/0004-6361/201219880/pdf"}],"createdAt":"2012-10-01","modifiedAt":"2025-04-09","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050846637961376640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"BAT AGN Spectroscopic Survey. XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei"}]},{"@id":"https://cir.nii.ac.jp/crid/1050848249841741312","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical, Infrared, and Radio Data"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168824420480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643775180032","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IV. Rapidly Growing (Super)Massive Black Holes in Extremely Radio-loud Galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567189632182912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Near-infrared Emission Lines in Starburst Galaxies at 0.5 < z < 0.9: Discovery of a Merger Sequence of Extreme Obscurations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659314186240","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A TALE OF TWO FEEDBACKS: STAR FORMATION IN THE HOST GALAXIES OF RADIO AGNs"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1051/0004-6361/201219880"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac1b26_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/aad33e_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ab238d_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202142352_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/784/2/137_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aaef8f_references_DOI_DKxGGf8aD0cwRcdkVSO1dNUuRIv"}]}