{"@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/1360869854371806208.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1051/0004-6361/202348167"}},{"identifier":{"@type":"URI","@value":"https://www.aanda.org/10.1051/0004-6361/202348167/pdf"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"The size-luminosity relation of local active galactic nuclei from interferometric observations of the broad-line region"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>By using the GRAVITY instrument with the near-infrared (NIR) Very Large Telescope Interferometer (VLTI), the structure of the broad (emission-)line region (BLR) in active galactic nuclei (AGNs) can be spatially resolved, allowing the central black hole (BH) mass to be determined. This work reports new NIR VLTI/GRAVITY interferometric spectra for four type 1 AGNs (Mrk 509, PDS 456, Mrk 1239, and IC 4329A) with resolved broad-line emission. Dynamical modelling of interferometric data constrains the BLR radius and central BH mass measurements for our targets and reveals outflow-dominated BLRs for Mrk 509 and PDS 456. We present an updated radius-luminosity (R-L) relation independent of that derived with reverberation mapping (RM) measurements using all the GRAVITY-observed AGNs. We find our R-L relation to be largely consistent with that derived from RM measurements except at high luminosity, where BLR radii seem to be smaller than predicted. This is consistent with RM-based claims that high Eddington ratio AGNs show consistently smaller BLR sizes. The BH masses of our targets are also consistent with the standard <jats:italic>M</jats:italic><jats:sub>BH</jats:sub>-<jats:italic>σ</jats:italic><jats:sub>*</jats:sub> relation. Model-independent photocentre fitting shows spatial offsets between the hot dust continuum and the BLR photocentres (ranging from ∼17 μas to 140 μas) that are generally perpendicular to the alignment of the red- and blueshifted BLR photocentres. These offsets are found to be related to the AGN luminosity and could be caused by asymmetric <jats:italic>K</jats:italic>-band emission of the hot dust, shifting the dust photocentre. We discuss various possible scenarios that can explain this phenomenon.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380869854371806626","@type":"Researcher","foaf:name":[{"@value":"A. Amorim"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806731","@type":"Researcher","foaf:name":[{"@value":"G. Bourdarot"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806625","@type":"Researcher","foaf:name":[{"@value":"W. Brandner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806594","@type":"Researcher","foaf:name":[{"@value":"Y. Cao"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806745","@type":"Researcher","foaf:name":[{"@value":"Y. Clénet"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806345","@type":"Researcher","foaf:name":[{"@value":"R. Davies"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806736","@type":"Researcher","foaf:name":[{"@value":"P. T. de Zeeuw"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806748","@type":"Researcher","foaf:name":[{"@value":"J. Dexter"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806212","@type":"Researcher","foaf:name":[{"@value":"A. Drescher"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806749","@type":"Researcher","foaf:name":[{"@value":"A. Eckart"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806630","@type":"Researcher","foaf:name":[{"@value":"F. Eisenhauer"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806344","@type":"Researcher","foaf:name":[{"@value":"M. Fabricius"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806751","@type":"Researcher","foaf:name":[{"@value":"H. Feuchtgruber"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806502","@type":"Researcher","foaf:name":[{"@value":"N. M. Förster Schreiber"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806240","@type":"Researcher","foaf:name":[{"@value":"P. J. V. Garcia"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806488","@type":"Researcher","foaf:name":[{"@value":"R. Genzel"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806477","@type":"Researcher","foaf:name":[{"@value":"S. Gillessen"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806727","@type":"Researcher","foaf:name":[{"@value":"D. Gratadour"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806624","@type":"Researcher","foaf:name":[{"@value":"S. Hönig"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806739","@type":"Researcher","foaf:name":[{"@value":"M. Kishimoto"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806608","@type":"Researcher","foaf:name":[{"@value":"S. Lacour"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806208","@type":"Researcher","foaf:name":[{"@value":"D. Lutz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806233","@type":"Researcher","foaf:name":[{"@value":"F. Millour"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806340","@type":"Researcher","foaf:name":[{"@value":"H. Netzer"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806211","@type":"Researcher","foaf:name":[{"@value":"T. Ott"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806595","@type":"Researcher","foaf:name":[{"@value":"T. Paumard"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806216","@type":"Researcher","foaf:name":[{"@value":"K. Perraut"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806469","@type":"Researcher","foaf:name":[{"@value":"G. Perrin"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806635","@type":"Researcher","foaf:name":[{"@value":"B. M. Peterson"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806597","@type":"Researcher","foaf:name":[{"@value":"P. O. Petrucci"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806730","@type":"Researcher","foaf:name":[{"@value":"O. Pfuhl"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806640","@type":"Researcher","foaf:name":[{"@value":"M. A. Prieto"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806606","@type":"Researcher","foaf:name":[{"@value":"S. Rabien"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806473","@type":"Researcher","foaf:name":[{"@value":"D. Rouan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806470","@type":"Researcher","foaf:name":[{"@value":"D. J. D. Santos"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806482","@type":"Researcher","foaf:name":[{"@value":"J. Shangguan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806349","@type":"Researcher","foaf:name":[{"@value":"T. Shimizu"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806342","@type":"Researcher","foaf:name":[{"@value":"A. Sternberg"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806603","@type":"Researcher","foaf:name":[{"@value":"C. Straubmeier"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806484","@type":"Researcher","foaf:name":[{"@value":"E. Sturm"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806343","@type":"Researcher","foaf:name":[{"@value":"L. J. Tacconi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806234","@type":"Researcher","foaf:name":[{"@value":"K. R. W. Tristram"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806609","@type":"Researcher","foaf:name":[{"@value":"F. Widmann"}]},{"@id":"https://cir.nii.ac.jp/crid/1380869854371806623","@type":"Researcher","foaf:name":[{"@value":"J. Woillez"}]}],"contributor":[{"@id":"https://cir.nii.ac.jp/crid/1891147691550420622","@type":"Researcher","foaf:name":[{"@value":"POTHIER, Nathalie"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00046361"},{"@type":"EISSN","@value":"14320746"}],"prism:publicationName":[{"@value":"Astronomy & Astrophysics"}],"dc:publisher":[{"@value":"EDP Sciences"}],"prism:publicationDate":"2024-04","prism:volume":"684","prism:startingPage":"A167"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["https://creativecommons.org/licenses/by/4.0"],"url":[{"@id":"https://www.aanda.org/10.1051/0004-6361/202348167/pdf"}],"createdAt":"2024-01-25","modifiedAt":"2024-04-19","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=%5BSDU%5D%20Sciences%20of%20the%20Universe%20%5Bphysics%5D","dc:title":"[SDU] Sciences of the Universe [physics]"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040018351905259136","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"24K00679"},{"@type":"JGN","@value":"JP24K00679"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-24K00679/"}],"notation":[{"@language":"ja","@value":"超高空間分解能観測で捉える巨大ブラックホール系の正体と母銀河"},{"@language":"en","@value":"Supermassive black hole systems and their host galaxies as revealed by high spatial resolution observations"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360002220784922496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"BAT AGN Spectroscopic Survey. 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