{"@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/1361699996185260928.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1086/432571"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.astro-ph/0504555"}}],"dc:title":[{"@value":"Measurement of Spin‐Orbit Alignment in an Extrasolar Planetary System"}],"description":[{"notation":[{"@value":"We determine the stellar, planetary, and orbital properties of the transiting planetary system HD 209458, through a joint analysis of high-precision radial velocities, photometry, and timing of the secondary eclipse. Of primary interest is the strong detection of the Rossiter-McLaughlin effect, the alteration of photospheric line profiles that occurs because the planet occults part of the rotating surface of the star. We develop a new technique for modeling this effect, and use it to determine the inclination of the planetary orbit relative to the apparent stellar equator [lambda = (-4.4 +/- 1.4) degrees], and the line-of-sight rotation speed of the star [v*sin(I) = (4.70 +/- 0.16) km/s]. The uncertainty in these quantities has been reduced by an order of magnitude relative to the pioneering measurements by Queloz and collaborators. The small but nonzero misalignment is probably a relic of the planet formation epoch, because the expected timescale for tidal coplanarization is larger than the age of the star. Our determination of v*sin(I) is a rare case in which rotational line broadening has been isolated from other broadening mechanisms."}]},{"notation":[{"@value":"21 pages, 6 figures. To match the version accepted by ApJ. Errors have been corrected in Table 1. (In previous versions, some confidence limits were mistakenly 80% rather than 90% limits.)"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381699996185261058","@type":"Researcher","foaf:name":[{"@value":"Joshua N. Winn"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261059","@type":"Researcher","foaf:name":[{"@value":"Robert W. Noyes"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260933","@type":"Researcher","foaf:name":[{"@value":"Matthew J. Holman"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261057","@type":"Researcher","foaf:name":[{"@value":"David Charbonneau"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261060","@type":"Researcher","foaf:name":[{"@value":"Yasuhiro Ohta"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260931","@type":"Researcher","foaf:name":[{"@value":"Atsushi Taruya"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260929","@type":"Researcher","foaf:name":[{"@value":"Yasushi Suto"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261062","@type":"Researcher","foaf:name":[{"@value":"Norio Narita"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261056","@type":"Researcher","foaf:name":[{"@value":"Edwin L. Turner"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260930","@type":"Researcher","foaf:name":[{"@value":"John A. Johnson"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185261061","@type":"Researcher","foaf:name":[{"@value":"Geoffrey W. Marcy"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260928","@type":"Researcher","foaf:name":[{"@value":"R. Paul Butler"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699996185260932","@type":"Researcher","foaf:name":[{"@value":"Steven S. Vogt"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"},{"@type":"PISSN","@value":"https://id.crossref.org/issn/0004637X"},{"@type":"PISSN","@value":"http://id.crossref.org/issn/0004637X"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2005-10","prism:volume":"631","prism:number":"2","prism:startingPage":"1215","prism:endingPage":"1226"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","createdAt":"2005-09-21","modifiedAt":"2020-11-06","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20(astro-ph)","dc:title":"Astrophysics (astro-ph)"},{"@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","dc:title":"Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=520","dc:title":"520"}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360002217424953088","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"CHARACTERIZATION OF THE KOI-94 SYSTEM WITH TRANSIT TIMING VARIATION ANALYSIS: IMPLICATION FOR THE PLANET-PLANET ECLIPSE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004233713863168","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The GJ 504 system revisited"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004234384024960","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"TIDAL EVOLUTION OF THE SPIN-ORBIT ANGLE IN EXOPLANETARY SYSTEMS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142920684544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Obliquity measurement and atmospheric characterisation of the WASP-74 planetary system"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168748834176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Disentangling the stellar inclination of transiting planetary systems: Fully analytic approach to the Rossiter–McLaughlin effect incorporating the stellar differential rotation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692401079424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MEASUREMENTS OF STELLAR INCLINATIONS FOR KEPLER PLANET CANDIDATES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692401788416","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MEASUREMENTS OF STELLAR INCLINATIONS FOR<i>KEPLER</i>PLANET CANDIDATES. II. CANDIDATE SPIN-ORBIT MISALIGNMENTS IN SINGLE- AND MULTIPLE-TRANSITING SYSTEMS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283695760586368","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"THE K2-ESPRINT PROJECT IV. A HOT JUPITER IN A PROGRADE ORBIT WITH A POSSIBLE STELLAR COMPANION"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709356664192","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"HAT-P-30b: A TRANSITING HOT JUPITER ON A HIGHLY OBLIQUE ORBIT"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709443327360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"THE SPIN EFFECT ON PLANETARY RADIAL VELOCIMETRY OF EXOPLANETS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617683217152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Limits on the Spin–Orbit Angle and Atmospheric Escape for the 22 Myr Old Planet AU Mic b*"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643793061120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Tidal Effects on the Radial Velocities of V723 Mon: Additional Evidence for a Dark 3 M\n               <sub>⊙</sub> Companion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904391311872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Transit spectroscopy of K2-33b with subaru/IRD: Spin-Orbit alignment and tentative atmospheric helium"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565170737152768","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"SPIN–ORBIT ALIGNMENT OF EXOPLANET SYSTEMS: ENSEMBLE ANALYSIS USING ASTEROSEISMOLOGY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567189625967872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Asteroseismic Determination of the Stellar Rotation Period of the Kepler Transiting Planetary Systems and its Implications for the Spin–Orbit Architecture"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230594207360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Architecture of Planetary Systems Predicted from Protoplanetary Disks Observed with ALMA. II. Evolution Outcomes and Dynamical Stability"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846642354519424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"OBLIQUITIES OF HOT JUPITER HOST STARS: EVIDENCE FOR TIDAL INTERACTIONS AND PRIMORDIAL MISALIGNMENTS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846642402349824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"PLANET-PLANET ECLIPSE AND THE ROSSITER-McLAUGHLIN EFFECT OF A MULTIPLE TRANSITING SYSTEM: JOINT ANALYSIS OF THE SUBARU SPECTROSCOPY AND THE KEPLER PHOTOMETRY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659310338304","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"TWO UPPER LIMITS ON THE ROSSITER-MCLAUGHLIN EFFECT, WITH DIFFERING IMPLICATIONS: WASP-1 HAS A HIGH OBLIQUITY AND WASP-2 IS INDETERMINATE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593747694720","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Zodiacal exoplanets in time – XIII. Planet orbits and atmospheres in the V1298 Tau system, a keystone in studies of early planetary evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1361131419499814912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Star–disc alignment in the protoplanetary discs: SPH simulation of the collapse of turbulent molecular cloud cores"}]},{"@id":"https://cir.nii.ac.jp/crid/1521699228423540352","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"IRSF SIRIUS JHKs Simultaneous Transit Photometry of GJ 1214b"}]},{"@id":"https://cir.nii.ac.jp/crid/1522262180772655488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Determination of three-dimensional spin-orbit angle with joint analysis of asteroseismology, transit lightcurve, and the Rossiter-McLaughlin effect : Cases of HAT-P-7 and Kepler-25"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1086/432571"},{"@type":"OPENAIRE","@value":"doi_dedup___::0b8d52d0968efd335b998acb4eead1ab"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/778/2/185_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/pasj/psu069_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201832942_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/784/1/66_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202038703_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/pasj/psab102_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/756/1/66_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/783/1/9_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/pasj/65.2.27_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/0004-637x/825/1/53_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/735/1/24_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/2041-8205/760/1/l13_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/aba6eb_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/abecdc_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/mnras/stae998_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/0004-637x/819/1/85_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/1538-3881/ab0f33_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac68de_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/757/1/18_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/2041-8205/759/2/l36_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/738/1/50_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/mnras/stab3107_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"},{"@type":"CROSSREF","@value":"10.1093/mnras/staa179_references_DOI_McnNguAJSshQUUK2LsIwUsjEuzZ"}]}