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dc.contributor.authorAlonso, Roi
dc.contributor.authorBrown, Timothy M.
dc.contributor.authorTorres, Guillermo
dc.contributor.authorLatham, David W.
dc.contributor.authorSozzetti, Alessandro
dc.contributor.authorMandushev, Georgi
dc.contributor.authorBelmonte, Juan A.
dc.contributor.authorCharbonneau, David
dc.contributor.authorDeeg, Hans J.
dc.contributor.authorDunham, Edward W.
dc.contributor.authorO'Donovan, Francis T.
dc.contributor.authorStefanik, Robert P.
dc.date.accessioned2019-09-24T17:25:21Z
dc.date.issued2004
dc.identifier.citationAlonso, Roi, Timothy M. Brown, Guillermo Torres, David W. Latham, Alessandro Sozzetti, Georgi Mandushev, Juan A. Belmonte, et al. 2004. “TrES-1: The Transiting Planet of a Bright K0 V Star.” The Astrophysical Journal 613 (2): L153–56. https://doi.org/10.1086/425256.
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41397424*
dc.description.abstractWe report the detection of a transiting Jupiter-sized planet orbiting a relatively bright (V = 11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES multisite transiting planet survey and confirmed the planetary nature of the companion via multicolor photometry and precise radial velocity measurements. We designate the planet TrES-1; its inferred mass is (0.75 +/- 0.07) M-Jup, its radius is 1.08(-0.04)(+0.18) R-Jup, and its orbital period is 3.030065 +/- 0.000008 days. This planet has an orbital period similar to that of HD 209458b but about twice as long as those of the OGLE transiting planets. Its mass is indistinguishable from that of HD 209458b, but its radius is significantly smaller and fits the theoretical models without the need for an additional source of heat deep in the atmosphere, as has been invoked by some investigators for HD 209458b.
dc.language.isoen_US
dc.publisherAmerican Astronomical Society
dash.licenseLAA
dc.titleTrES-1: The Transiting Planet of a Bright K0 V Star
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalThe Astrophysical Journal
dash.depositing.authorCharbonneau, David::a0e3ca75d3fb8511f2f554ed69428108::600
dc.date.available2019-09-24T17:25:21Z
dash.workflow.comments1Science Serial ID 96866
dc.identifier.doi10.1086/425256
dash.source.volume613;2
dash.source.pageL153-L156


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