{"@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/1360004234662579072.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1093/mnras/sty3464"}},{"identifier":{"@type":"URI","@value":"http://academic.oup.com/mnras/article-pdf/484/1/8/27507117/sty3464.pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1809.01968"}},{"identifier":{"@type":"HANDLE","@value":"1887/68858"}},{"identifier":{"@type":"HANDLE","@value":"1887/83154"}},{"identifier":{"@type":"HANDLE","@value":"2318/1711526"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"K2-264: a transiting multiplanet system in the Praesepe open cluster"}],"description":[{"notation":[{"@value":"Planet host stars with well-constrained ages provide a rare window to the time domain of planet formation and evolution. The NASA K2 mission has enabled the discovery of the vast majority of known planets transiting stars in clusters, providing a valuable sample of planets with known ages and radii. We present the discovery of two planets transiting K2-264, an M2 dwarf in the intermediate age (600-800 Myr) Praesepe open cluster (also known as the Beehive Cluster, M44, or NGC 2632), which was observed by K2 during Campaign 16. The planets have orbital periods of 5.8 and 19.7 days, and radii of $2.2 \\pm 0.2 $ and $2.7 \\pm 0.2$ $R_\\oplus$, respectively, and their equilibrium temperatures are $496 \\pm 10$ and $331 \\pm 7$ $K$, making this a system of two warm sub-Neptunes. When placed in the context of known planets orbiting field stars of similar mass to K2-264, these planets do not appear to have significantly inflated radii, as has previously been noted for some cluster planets. As the second known system of multiple planets transiting a star in a cluster, K2-264 should be valuable for testing theories of photoevaporation in systems of multiple planets. Follow-up observations with current near-infrared (NIR) spectrographs could yield planet mass measurements, which would provide information about the mean densities and compositions of small planets soon after photoevaporation is expected to have finished. Follow-up NIR transit observations using Spitzer or large ground-based telescopes could yield improved radius estimates, further enhancing the characterization of these interesting planets."}]},{"notation":[{"@value":"12 pages, 11 figures, 2 tables, published in MNRAS; see also secular dynamics at https://youtu.be/MSLodufHRes"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004234662579459","@type":"Researcher","foaf:name":[{"@value":"John H Livingston"}],"jpcoar:affiliationName":[{"@value":"Department of Astronomy, University of Tokyo, 7-3-1 Hongo, Bunkyo-ky, Tokyo 113-0033, Japan"},{"@value":"JSPS Fellow"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234662578826","@type":"Researcher","foaf:name":[{"@value":"Fei Dai"}],"jpcoar:affiliationName":[{"@value":"Dept. of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA"},{"@value":"Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1420001326228745600","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"10727449"},{"@type":"NRID","@value":"1000010727449"}],"foaf:name":[{"@value":"Teruyuki Hirano"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234662579076","@type":"Researcher","foaf:name":[{"@value":"Davide Gandolfi"}],"jpcoar:affiliationName":[{"@value":"Dipartimento di Fisica, Università di Torino, via P. 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Van Eylen"}],"jpcoar:affiliationName":[{"@value":"Leiden Observatory, Leiden University, NL-2333CA Leiden, the Netherlands"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234662578961","@type":"Researcher","foaf:name":[{"@value":"Joshua N Winn"}],"jpcoar:affiliationName":[{"@value":"Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00358711"},{"@type":"EISSN","@value":"13652966"}],"prism:publicationName":[{"@value":"Monthly Notices of the Royal Astronomical Society"}],"dc:publisher":[{"@value":"Oxford University Press 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detection"},{"@id":"https://cir.nii.ac.jp/all?q=Planets%20and%20satellites:%20detection;%20Techniques:%20high%20angular%20resolution;%20Techniques:%20photometric","dc:title":"Planets and satellites: detection; Techniques: high angular resolution; Techniques: photometric"},{"@id":"https://cir.nii.ac.jp/all?q=Leitungsbereich%20PF","dc:title":"Leitungsbereich PF"},{"@id":"https://cir.nii.ac.jp/all?q=imaging","dc:title":"imaging"},{"@id":"https://cir.nii.ac.jp/all?q=techniques:%20high%20angular%20resolution","dc:title":"techniques: high angular resolution"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=ddc:no","dc:title":"ddc:no"},{"@id":"https://cir.nii.ac.jp/all?q=520","dc:title":"520"},{"@id":"https://cir.nii.ac.jp/all?q=techniques:%20photometric","dc:title":"techniques: photometric"},{"@id":"https://cir.nii.ac.jp/all?q=observations","dc:title":"observations"},{"@id":"https://cir.nii.ac.jp/all?q=exoplanets","dc:title":"exoplanets"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20Planetary%20Astrophysics","dc:title":"Astrophysics - Earth and Planetary Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781958031744","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H04574"},{"@type":"JGN","@value":"JP17H04574"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17H04574/"}],"notation":[{"@language":"ja","@value":"太陽系近傍の小型トランジット系外惑星の発見と大気の系統的調査"},{"@language":"en","@value":"Search for Nearby, Small-sized Transiting Exoplanets and Study of Their 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