{"@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/1360021394470327040.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/2041-8213/acec3e"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/2041-8213/acec3e"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/2041-8213/acec3e/pdf"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"IXPE and Multiwavelength Observations of Blazar PG 1553+113 Reveal an Orphan Optical Polarization Swing"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>The lower-energy peak of the spectral energy distribution of blazars has commonly been ascribed to synchrotron radiation from relativistic particles in the jets. Despite the consensus regarding jet emission processes, the particle acceleration mechanism is still debated. Here, we present the first X-ray polarization observations of PG 1553+113, a high-synchrotron-peak blazar observed by the Imaging X-ray Polarimetry Explorer (IXPE). We detect an X-ray polarization degree of (10 ± 2)% along an electric-vector position angle of <jats:italic>ψ</jats:italic>\n                  <jats:sub>X</jats:sub> = 86° ± 8°. At the same time, the radio and optical polarization degrees are lower by a factor of ∼3. During our IXPE pointing, we observed the first orphan optical polarization swing of the IXPE era, as the optical angle of PG 1553+113 underwent a smooth monotonic rotation by about 125°, with a rate of ∼17° day<jats:sup>–1</jats:sup>. We do not find evidence of a similar rotation in either radio or X-rays, which suggests that the X-ray and optically emitting regions are separate or, at most, partially cospatial. Our spectropolarimetric results provide further evidence that the steady-state X-ray emission in blazars originates in a shock-accelerated and energy-stratified electron population.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380021394470327189","@type":"Researcher","foaf:name":[{"@value":"Riccardo Middei"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327239","@type":"Researcher","foaf:name":[{"@value":"Matteo Perri"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327046","@type":"Researcher","foaf:name":[{"@value":"Simonetta Puccetti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327210","@type":"Researcher","foaf:name":[{"@value":"Ioannis Liodakis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327061","@type":"Researcher","foaf:name":[{"@value":"Laura Di Gesu"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327185","@type":"Researcher","foaf:name":[{"@value":"Alan P. Marscher"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327067","@type":"Researcher","foaf:name":[{"@value":"Nicole Rodriguez Cavero"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327205","@type":"Researcher","foaf:name":[{"@value":"Fabrizio Tavecchio"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327228","@type":"Researcher","foaf:name":[{"@value":"Immacolata Donnarumma"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327042","@type":"Researcher","foaf:name":[{"@value":"Herman L. Marshall"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327069","@type":"Researcher","foaf:name":[{"@value":"Víctor Casanova"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327181","@type":"Researcher","foaf:name":[{"@value":"Giacomo Bonnoli"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327068","@type":"Researcher","foaf:name":[{"@value":"Beatriz Agís-González"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327207","@type":"Researcher","foaf:name":[{"@value":"Carolina Casadio"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327063","@type":"Researcher","foaf:name":[{"@value":"Alfredo Sota"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327174","@type":"Researcher","foaf:name":[{"@value":"Ioannis Myserlis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327064","@type":"Researcher","foaf:name":[{"@value":"Juan Escudero"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327180","@type":"Researcher","foaf:name":[{"@value":"Pouya M. Kouch"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327188","@type":"Researcher","foaf:name":[{"@value":"Albrecht Sievers"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327050","@type":"Researcher","foaf:name":[{"@value":"Mark Gurwell"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327235","@type":"Researcher","foaf:name":[{"@value":"Elina Lindfors"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327223","@type":"Researcher","foaf:name":[{"@value":"Ramprasad Rao"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327208","@type":"Researcher","foaf:name":[{"@value":"Garrett K. Keating"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327079","@type":"Researcher","foaf:name":[{"@value":"Sincheol Kang"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327040","@type":"Researcher","foaf:name":[{"@value":"Sang-Sung Lee"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327193","@type":"Researcher","foaf:name":[{"@value":"Whee Yeon Cheong"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327049","@type":"Researcher","foaf:name":[{"@value":"Sang-Hyun Kim"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327062","@type":"Researcher","foaf:name":[{"@value":"Hyeon-Woo Jeong"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327213","@type":"Researcher","foaf:name":[{"@value":"Luigi Pacciani"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327083","@type":"Researcher","foaf:name":[{"@value":"Dawoon E. Kim"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327187","@type":"Researcher","foaf:name":[{"@value":"Marco Laurenti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327170","@type":"Researcher","foaf:name":[{"@value":"Francisco José Aceituno"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327186","@type":"Researcher","foaf:name":[{"@value":"Svetlana G. Jorstad"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327199","@type":"Researcher","foaf:name":[{"@value":"Iván Agudo"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327184","@type":"Researcher","foaf:name":[{"@value":"Emmanouil Angelakis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327232","@type":"Researcher","foaf:name":[{"@value":"Alexander Kraus"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327229","@type":"Researcher","foaf:name":[{"@value":"Lucio A. Antonelli"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327236","@type":"Researcher","foaf:name":[{"@value":"Matteo Bachetti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327219","@type":"Researcher","foaf:name":[{"@value":"Luca Baldini"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327074","@type":"Researcher","foaf:name":[{"@value":"Wayne H. Baumgartner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327058","@type":"Researcher","foaf:name":[{"@value":"Ronaldo Bellazzini"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327220","@type":"Researcher","foaf:name":[{"@value":"Stefano Bianchi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327084","@type":"Researcher","foaf:name":[{"@value":"Stephen D. Bongiorno"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327070","@type":"Researcher","foaf:name":[{"@value":"Raffaella Bonino"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327182","@type":"Researcher","foaf:name":[{"@value":"Alessandro Brez"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327222","@type":"Researcher","foaf:name":[{"@value":"Niccolò Bucciantini"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327060","@type":"Researcher","foaf:name":[{"@value":"Fiamma Capitanio"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327216","@type":"Researcher","foaf:name":[{"@value":"Elisabetta Cavazzuti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327066","@type":"Researcher","foaf:name":[{"@value":"Chien-Ting Chen"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327217","@type":"Researcher","foaf:name":[{"@value":"Simone Castellano"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327056","@type":"Researcher","foaf:name":[{"@value":"Stefano Ciprini"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327047","@type":"Researcher","foaf:name":[{"@value":"Enrico Costa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327044","@type":"Researcher","foaf:name":[{"@value":"Alessandra De Rosa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327198","@type":"Researcher","foaf:name":[{"@value":"Ettore Del Monte"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327071","@type":"Researcher","foaf:name":[{"@value":"Niccolò Di Lalla"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327055","@type":"Researcher","foaf:name":[{"@value":"Michal Dovčiak"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327214","@type":"Researcher","foaf:name":[{"@value":"Victor Doroshenko"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327043","@type":"Researcher","foaf:name":[{"@value":"Alessandro Di Marco"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327048","@type":"Researcher","foaf:name":[{"@value":"Steven R. Ehlert"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327175","@type":"Researcher","foaf:name":[{"@value":"Teruaki Enoto"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327059","@type":"Researcher","foaf:name":[{"@value":"Sergio Fabiani"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327238","@type":"Researcher","foaf:name":[{"@value":"Yuri Evangelista"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327191","@type":"Researcher","foaf:name":[{"@value":"Riccardo Ferrazzoli"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327171","@type":"Researcher","foaf:name":[{"@value":"Takao Kitaguchi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327077","@type":"Researcher","foaf:name":[{"@value":"Jeffery J. Kolodziejczak"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327073","@type":"Researcher","foaf:name":[{"@value":"Henric Krawczynski"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327237","@type":"Researcher","foaf:name":[{"@value":"Fabio La Monaca"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327086","@type":"Researcher","foaf:name":[{"@value":"Luca Latronico"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327206","@type":"Researcher","foaf:name":[{"@value":"Simone Maldera"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327221","@type":"Researcher","foaf:name":[{"@value":"Alberto Manfreda"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327087","@type":"Researcher","foaf:name":[{"@value":"Frédéric Marin"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327196","@type":"Researcher","foaf:name":[{"@value":"Andrea Marinucci"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327192","@type":"Researcher","foaf:name":[{"@value":"Javier A. García"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327195","@type":"Researcher","foaf:name":[{"@value":"Kiyoshi Hayashida"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327197","@type":"Researcher","foaf:name":[{"@value":"Shuichi Gunji"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327227","@type":"Researcher","foaf:name":[{"@value":"Wataru Iwakiri"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327173","@type":"Researcher","foaf:name":[{"@value":"Jeremy Heyl"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327052","@type":"Researcher","foaf:name":[{"@value":"Fabian Kislat"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327234","@type":"Researcher","foaf:name":[{"@value":"Vladimir Karas"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327076","@type":"Researcher","foaf:name":[{"@value":"Philip Kaaret"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327045","@type":"Researcher","foaf:name":[{"@value":"Francesco Massaro"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327201","@type":"Researcher","foaf:name":[{"@value":"Giorgio Matt"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327209","@type":"Researcher","foaf:name":[{"@value":"Ikuyuki Mitsuishi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327179","@type":"Researcher","foaf:name":[{"@value":"Tsunefumi Mizuno"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327080","@type":"Researcher","foaf:name":[{"@value":"Fabio Muleri"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327230","@type":"Researcher","foaf:name":[{"@value":"Michela Negro"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327212","@type":"Researcher","foaf:name":[{"@value":"Chi-Yung Ng"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327082","@type":"Researcher","foaf:name":[{"@value":"Stephen L. O’Dell"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327190","@type":"Researcher","foaf:name":[{"@value":"Nicola Omodei"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327078","@type":"Researcher","foaf:name":[{"@value":"Alessandro Papitto"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327178","@type":"Researcher","foaf:name":[{"@value":"Chiara Oppedisano"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327233","@type":"Researcher","foaf:name":[{"@value":"Brian D. Ramsey"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327183","@type":"Researcher","foaf:name":[{"@value":"Juri Poutanen"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327218","@type":"Researcher","foaf:name":[{"@value":"Ajay Ratheesh"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327202","@type":"Researcher","foaf:name":[{"@value":"John Rankin"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327041","@type":"Researcher","foaf:name":[{"@value":"Oliver J. Roberts"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327241","@type":"Researcher","foaf:name":[{"@value":"Roger W. Romani"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327072","@type":"Researcher","foaf:name":[{"@value":"Carmelo Sgrò"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327231","@type":"Researcher","foaf:name":[{"@value":"Patrick Slane"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327211","@type":"Researcher","foaf:name":[{"@value":"Paolo Soffitta"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327177","@type":"Researcher","foaf:name":[{"@value":"Gloria Spandre"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327054","@type":"Researcher","foaf:name":[{"@value":"Abel L. Peirson"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327057","@type":"Researcher","foaf:name":[{"@value":"Pierre-Olivier Petrucci"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327224","@type":"Researcher","foaf:name":[{"@value":"Melissa Pesce-Rollins"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327194","@type":"Researcher","foaf:name":[{"@value":"Maura Pilia"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327240","@type":"Researcher","foaf:name":[{"@value":"Andrea Possenti"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327051","@type":"Researcher","foaf:name":[{"@value":"George G. Pavlov"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327215","@type":"Researcher","foaf:name":[{"@value":"Douglas A. Swartz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327200","@type":"Researcher","foaf:name":[{"@value":"Toru Tamagawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327176","@type":"Researcher","foaf:name":[{"@value":"Roberto Taverna"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327085","@type":"Researcher","foaf:name":[{"@value":"Yuzuru Tawara"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327081","@type":"Researcher","foaf:name":[{"@value":"Allyn F. Tennant"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327225","@type":"Researcher","foaf:name":[{"@value":"Nicholas E. Thomas"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327065","@type":"Researcher","foaf:name":[{"@value":"Francesco Tombesi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327075","@type":"Researcher","foaf:name":[{"@value":"Alessio Trois"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327172","@type":"Researcher","foaf:name":[{"@value":"Sergey S. Tsygankov"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327169","@type":"Researcher","foaf:name":[{"@value":"Jacco Vink"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327203","@type":"Researcher","foaf:name":[{"@value":"Roberto Turolla"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327204","@type":"Researcher","foaf:name":[{"@value":"Silvia Zane"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327053","@type":"Researcher","foaf:name":[{"@value":"Martin C. Weisskopf"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327226","@type":"Researcher","foaf:name":[{"@value":"Kinwah Wu"}]},{"@id":"https://cir.nii.ac.jp/crid/1380021394470327168","@type":"Researcher","foaf:name":[{"@value":"Fei Xie"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"20418205"},{"@type":"EISSN","@value":"20418213"}],"prism:publicationName":[{"@value":"The Astrophysical Journal Letters"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2023-08-01","prism:volume":"953","prism:number":"2","prism:startingPage":"L28"},"reviewed":"false","dc:rights":["http://creativecommons.org/licenses/by/4.0/","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"https://iopscience.iop.org/article/10.3847/2041-8213/acec3e"},{"@id":"https://iopscience.iop.org/article/10.3847/2041-8213/acec3e/pdf"}],"createdAt":"2023-08-22","modifiedAt":"2024-01-08","project":[{"@id":"https://cir.nii.ac.jp/crid/1040003825673250816","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H05609"},{"@type":"JGN","@value":"JP19H05609"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19H05609/"}],"notation":[{"@language":"ja","@value":"X線・ガンマ線偏光観測で開拓する中性子星超強磁場の物理"},{"@language":"en","@value":"Elucidation of ultra-strong magnetic field of neutron stars with highly-sensitive X-ray and Gamma-ray polarimetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1040014327101994368","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"23H04895"},{"@type":"JGN","@value":"JP23H04895"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-23H04895/"}],"notation":[{"@language":"ja","@value":"X線が届ける突発天体の目覚め"},{"@language":"en","@value":"Astronomical transients investigated by X-ray"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360011144496260352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Optical polarization of high-energy BL Lacertae objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146436393728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths – III. Characterization of total flux density and polarization variability of relativistic jets"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017280640694400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The X-Ray Polarization View of Mrk 421 in an Average Flux State as Observed by the Imaging X-Ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017286639164416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Kink-driven magnetic reconnection in relativistic jets: consequences for X-ray polarimetry of BL Lacs"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021394473179264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Uncovering the geometry of the hot X-ray corona in the Seyfert galaxy NGC 4151 with IXPE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021395463822208","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Fermi-LAT Lightcurve Repository*"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021395464866944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Full-Stokes polarimetry with circularly polarized feeds"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021396148460544","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Two Flares with One Shock: The Interesting Case of 3C 454.3"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025434743612928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A parsec-scale wobbling jet in the high-synchrotron peaked blazar PG 1553+113"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025434743921536","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"OUP accepted manuscript"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025434744675072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Modeling the Time-Dependent Polarization of Blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619256997760","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An efficient photoelectric X-ray polarimeter for the study of black holes and neutron stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619972397056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MONITORING OF GAMMA-RAY BRIGHT AGN: THE MULTI-FREQUENCY POLARIZATION OF THE FLARING BLAZAR 3C 279"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620922012928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PROBING THE INNER JET OF THE QUASAR PKS 1510–089 WITH MULTI-WAVEBAND MONITORING DURING STRONG GAMMA-RAY ACTIVITY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292621353141632","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RoboPol: the optical polarization of gamma-ray-loud and gamma-ray-quiet blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643773489792","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Design, construction, and test of the Gas Pixel Detectors for the IXPE mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298757177588864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Limits on X-Ray Polarization at the Core of Centaurus A as Observed with the Imaging X-Ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298761826234752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ixpeobssim: A simulation and analysis framework for the imaging X-ray polarimetry explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298761845919616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Frequency and Time Dependence of Linear Polarization in Turbulent Jets of Blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298762721794560","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Novel gaseous x-ray polarimeter: data analysis and simulation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905161413760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Periodic Gamma-Ray Modulation of the Blazar PG 1553+113 Confirmed by Fermi-LAT and Multiwavelength Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306910247405952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Multifrequency observations of a sample of very low frequency peaked BL Lacertae objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565167386755968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>FERMI</i>\n                    LARGE AREA TELESCOPE THIRD SOURCE CATALOG"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184334466176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PG 1553+113: FIVE YEARS OF OBSERVATIONS WITH MAGIC"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095014518016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Doppler factors, Lorentz factors and viewing angles  for quasars, BL Lacertae objects and radio galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095032896896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE SPECTRAL ENERGY DISTRIBUTION OF<i>FERMI</i>BRIGHT BLAZARS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095572744064","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for a multizone warm absorber in the<i>XMM-Newton</i>spectrum of Markarian 304"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576120153272192","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Relativistic Jets of Blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122012902400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Multiwavelength cross-correlations and flaring activity in bright blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580232390828544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-Ray Polarization Observations of BL Lacertae"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580234604843776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing Blazar Emission Processes with Optical/Gamma-Ray Flare Correlations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580235881956352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Constraining the Limiting Brightness Temperature and Doppler Factors for the Largest Sample of Radio-bright Blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580235893657728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing dissipation mechanisms in BL Lac jets through X-ray polarimetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580236935325952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Weighted Analysis to Improve the X-Ray Polarization Sensitivity of the Imaging X-ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580237005557504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-ray spectra, light curves and SEDs of blazars frequently observed by Swift"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584343746809728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"First-principles-integrated Study of Blazar Synchrotron Radiation and Polarization Signatures from Magnetic Turbulence"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380600972544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"IXPE observation of PKS 2155–304 reveals the most highly polarized blazar"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588385569767168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Blazar PG 1553+113 as a Binary System of Supermassive Black Holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588387672107136","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Physical Origins of the Identified and Still Missing Components of the Warm–Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568839894272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Unified Schemes for Radio-Loud Active Galactic Nuclei"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570181000576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Models for high-frequency radio outbursts in extragalactic sources, with application to the early 1983 millimeter-to-infrared flare of 3C 273"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570772636288","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Optical and Infrared Polarization of Active Extragalactic Objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861704764480896","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Polarized blazar X-rays imply particle acceleration in shocks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861704766629760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Polarization constraints on the X-ray corona in Seyfert Galaxies: MCG-05-23-16"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861704766675584","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mapping the circumnuclear regions of the Circinus galaxy with the Imaging X-ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861710856163968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An observation-simulation and analysis framework for the Imaging X-ray Polarimetry Explorer (IXPE)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861711783120512","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The first hard X-ray spectral catalogue of Blazars observed by <i>NuSTAR</i>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861711783420928","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Imaging X-ray Polarimetry Explorer: prelaunch"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861711969569920","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Handling the Background in IXPE Polarimetric Data"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815493282816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815498940800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Discovery of X-ray polarization angle rotation in the jet from blazar Mrk 421"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815674596224","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetic field properties inside the jet of Mrk 421"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865816806034944","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-Ray Polarization of BL Lacertae in Outburst"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869854358640640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"IXPE observation of the low-synchrotron peaked blazar S4 0954+65 during an optical-X-ray flare"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869854363825152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observations of Low and Intermediate Spectral Peak Blazars with the Imaging X-Ray Polarimetry Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869854363881600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"X-Ray and Multiwavelength Polarization of Mrk 501 from 2022 to 2023"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869863358663808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A First-principle Model for Polarization Swings during Reconnection-powered Flares"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043633658880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A jet model for the gamma-ray emitting blazar 3C 279"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044332492160","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Total Flux Density Variations in Extragalactic Radio Sources. III. Doppler Boosting Factors, Lorentz Factors, and Viewing Angles for Active Galactic Nuclei"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044738745088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Optical and Radio Polarimetry of the M87 Jet at 0[farcs]2 Resolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044892240128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A theoretical unifying scheme for gamma-ray bright blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044939411584","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EGRET Observations of the Extragalactic Gamma‐Ray Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045188497920","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"3C 286: a bright, compact, stable, and highly polarized calibrator for millimeter-wavelength observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045970421504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations of the missing baryons in the warm–hot intergalactic medium"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046026367616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"HI4PI: a full-sky H i survey based on EBHIS and GASS"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046125177216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The<i>Swift</i>Gamma‐Ray Burst Mission"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993934612864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A unifying view of the spectral energy distributions of blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994190844416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Intraday variability in compact extragalactic radio sources"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699996238755840","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RoboPol: optical polarization-plane rotations and flaring activity in blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943393371776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The inner jet of an active galactic nucleus as revealed by a radio-to-γ-ray outburst"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943549687040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"XMM-Newton observatory"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943778522112","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Unified Models for Active Galactic Nuclei and Quasars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418982676352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The submillimeter array polarimeter"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420452685056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The X‐Ray Emissions from the M87 Jet: Diagnostics and Physical Interpretation"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893832526720","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Log-parabolic spectra and particle acceleration in the BL Lac object Mkn 421: Spectral \nanalysis of the complete BeppoSAX wide band X-ray data set"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368365259264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Active galactic nuclei: what’s in a name?"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368987495936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"LOCATION OF γ-RAY FLARE EMISSION IN THE JET OF THE BL LACERTAE OBJECT OJ287 MORE THAN 14 pc FROM THE CENTRAL ENGINE"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369359237888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Submillimeter Array"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369615976960","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369684021632","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The European Photon Imaging Camera on XMM-Newton: The pn-CCD camera"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370544606848","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths – II. Widespread circular polarization"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370724382592","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RoboPol: connection between optical polarization plane rotations and gamma-ray flares in blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843757377152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Long-term optical monitoring of TeV emitting blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844451396864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RoboPol: first season rotations of optical polarization plane in blazars"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845528056448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The connection between x-ray- and radio-selected BL Lacertae objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845656483072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"POLAMI: Polarimetric Monitoring of AGN at Millimetre Wavelengths – I. The programme, calibration and calibrator data products"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319262687104","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"When is pile-up important in the<i>XMM-Newton</i>EPIC cameras?"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794099588224","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794357197312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MULTIWAVELENGTH EVIDENCE FOR QUASI-PERIODIC MODULATION IN THE GAMMA-RAY BLAZAR PG 1553+113"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794396200832","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A hadronic origin for ultra-high-frequency-peaked BL Lac objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269287998464","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>RoboPol</i>: do optical polarization rotations occur in all blazars?"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269488263936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Relativistic Jets from Active Galactic Nuclei"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270313702272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SWARM: A 32 GHz Correlator and VLBI Beamformer for the Submillimeter Array"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270930524288","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ON THE LOCATION OF THE γ-RAY OUTBURST EMISSION IN THE BL LACERTAE OBJECT AO 0235+164 THROUGH OBSERVATIONS ACROSS THE ELECTROMAGNETIC SPECTRUM"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.3847/2041-8213/acec3e"},{"@type":"KAKEN","@value":"PRODUCT-25339975"},{"@type":"KAKEN","@value":"PRODUCT-25342114"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad64c5_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202449166_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad1ce4_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202347408_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202453127_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad5671_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad63a1_references_DOI_13Q54H4283G56GFSeV9wgQbvxR1"}]}