{"@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/1360021390559287296.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1051/0004-6361/202245726"}},{"identifier":{"@type":"URI","@value":"https://www.aanda.org/10.1051/0004-6361/202245726/pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.2301.01388"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Which galaxies in the general population turn into active galactic nuclei (AGNs) is a keystone of galaxy formation and evolution. Thanks to SRG/eROSITA’s contiguous 140 square degree pilot survey field, we constructed a large, complete, and unbiased soft X-ray flux-limited (<jats:italic>F</jats:italic><jats:sub>X</jats:sub> > 6.5 × 10<jats:sup>−15</jats:sup>erg s<jats:sup>−1</jats:sup>cm<jats:sup>−2</jats:sup>) AGN sample at low redshift, 0.05 < <jats:italic>z</jats:italic> < 0.55. Two summary statistics, the clustering using spectra from SDSS-V and galaxy-galaxy lensing with imaging from HSC, are measured and interpreted with halo occupation distribution and abundance matching models. Both models successfully account for the observations. We obtain an exceptionally complete view of the AGN halo occupation distribution. The population of AGNs is broadly distributed among halos with a mean mass of 3.9<jats:sub>−2.4</jats:sub><jats:sup>+2.0</jats:sup> × 10<jats:sup>12</jats:sup> <jats:italic>M</jats:italic><jats:sub>⊙</jats:sub>. This corresponds to a large-scale halo bias of<jats:italic>b</jats:italic>(<jats:italic>z</jats:italic> = 0.34) = 0.99<jats:sub>−0.10</jats:sub><jats:sup>+0.08</jats:sup>. The central occupation has a large transition parameter,<jats:italic>σ</jats:italic><jats:sub>log<jats:sub>10</jats:sub>(<jats:italic>M</jats:italic>)</jats:sub> = 1.28 ± 0.2. The satellite occupation distribution is characterized by a shallow slope,<jats:italic>α</jats:italic><jats:sub>sat</jats:sub> = 0.73 ± 0.38. We find that AGNs in satellites are rare, with<jats:italic>f</jats:italic><jats:sub>sat</jats:sub> < 20%. Most soft X-ray-selected AGNs are hosted by central galaxies in their dark matter halo. A weak correlation between soft X-ray luminosity and large-scale halo bias is confirmed (3.3<jats:italic>σ</jats:italic>). We discuss the implications of environmental-dependent AGN triggering. This study paves the way toward fully charting, in the coming decade, the coevolution of X-ray AGNs, their host galaxies, and dark matter halos by combining eROSITA with SDSS-V, 4MOST, DESI, LSST, and<jats:italic>Euclid</jats:italic>data.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380021390559287446","@type":"Researcher","foaf:name":[{"@value":"Johan Comparat"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287320","@type":"Researcher","foaf:name":[{"@value":"Wentao Luo"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287453","@type":"Researcher","foaf:name":[{"@value":"Andrea Merloni"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287425","@type":"Researcher","foaf:name":[{"@value":"Surhud More"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287424","@type":"Researcher","foaf:name":[{"@value":"Mara Salvato"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287313","@type":"Researcher","foaf:name":[{"@value":"Mirko Krumpe"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287185","@type":"Researcher","foaf:name":[{"@value":"Takamitsu Miyaji"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287338","@type":"Researcher","foaf:name":[{"@value":"William Brandt"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287201","@type":"Researcher","foaf:name":[{"@value":"Antonis Georgakakis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287179","@type":"Researcher","foaf:name":[{"@value":"Masayuki Akiyama"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287325","@type":"Researcher","foaf:name":[{"@value":"Johannes Buchner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287448","@type":"Researcher","foaf:name":[{"@value":"Tom Dwelly"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287331","@type":"Researcher","foaf:name":[{"@value":"Toshihiro Kawaguchi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287314","@type":"Researcher","foaf:name":[{"@value":"Teng Liu"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287195","@type":"Researcher","foaf:name":[{"@value":"Tohru Nagao"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287582","@type":"Researcher","foaf:name":[{"@value":"Kirpal Nandra"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287202","@type":"Researcher","foaf:name":[{"@value":"John Silverman"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287170","@type":"Researcher","foaf:name":[{"@value":"Yoshiki Toba"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287566","@type":"Researcher","foaf:name":[{"@value":"Scott F. Anderson"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021390559287445","@type":"Researcher","foaf:name":[{"@value":"Juna Kollmeier"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00046361"},{"@type":"EISSN","@value":"14320746"}],"prism:publicationName":[{"@value":"Astronomy & Astrophysics"}],"dc:publisher":[{"@value":"EDP Sciences"}],"prism:publicationDate":"2023-05","prism:volume":"673","prism:startingPage":"A122"},"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/10.1051/0004-6361/202245726/pdf"}],"createdAt":"2023-04-03","modifiedAt":"2024-10-17","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Cosmology%20and%20Nongalactic%20Astrophysics%20(astro-ph.CO)","dc:title":"Cosmology and Nongalactic Astrophysics (astro-ph.CO)"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20of%20Galaxies%20(astro-ph.GA)","dc:title":"Astrophysics of Galaxies (astro-ph.GA)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Astrophysics%20of%20Galaxies","dc:title":"Astrophysics - Astrophysics of Galaxies"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Cosmology%20and%20Nongalactic%20Astrophysics","dc:title":"Astrophysics - Cosmology and Nongalactic Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040285300660740480","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19KK0076"},{"@type":"JGN","@value":"JP19KK0076"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19KK0076/"}],"notation":[{"@language":"ja","@value":"HSC-SSP光学サーベイとeROSTIA X線サーベイによる精密宇宙論"},{"@language":"en","@value":"Precision Cosmology from the HSC-SSP optical and eROSITA X-ray surveys"}]},{"@id":"https://cir.nii.ac.jp/crid/1040299826880320128","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"23K25911"},{"@type":"JGN","@value":"JP23K25911"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-23K25911/"}],"notation":[{"@language":"ja","@value":"多波長高感度超広域サーベイによる電波銀河観測が紐解く、初期宇宙での大質量銀河進化"},{"@language":"en","@value":"Evolution of massive galaxies in the early Universe revealed through observations of massive galaxies searched by multi-wavelength wide and deep surveys"}]},{"@id":"https://cir.nii.ac.jp/crid/1040850857202441856","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"21H04496"},{"@type":"JGN","@value":"JP21H04496"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-21H04496/"}],"notation":[{"@language":"ja","@value":"活動銀河核構造の全波長域新パラダイムの確立"},{"@language":"en","@value":"A Physically-motivated Multi-wavelength Paradigm for the Central Structure of AGNs"}]},{"@id":"https://cir.nii.ac.jp/crid/1040862776832132992","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"23K22537"},{"@type":"JGN","@value":"JP23K22537"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-23K22537/"}],"notation":[{"@language":"ja","@value":"Euclid・eROSITA・すばるで探る銀河と超巨大ブラックホールの共進化史"},{"@language":"en","@value":"Growth history of galaxies and supermassive black holes explored by Euclid, eROSITA, and Subaru Telescope"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050282813791797504","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey"}]},{"@id":"https://cir.nii.ac.jp/crid/1050850475691412864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Dark Quest. 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