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dc.contributor.authorMarcy, Geoffrey W.
dc.contributor.authorIsaacson, Howard
dc.contributor.authorHoward, Andrew W.
dc.contributor.authorRowe, Jason F.
dc.contributor.authorJenkins, Jon M.
dc.contributor.authorBryson, Stephen T.
dc.contributor.authorLatham, David W.
dc.contributor.authorHowell, Steve B.
dc.contributor.authorGautier, Thomas N.
dc.contributor.authorBatalha, Natalie M.
dc.contributor.authorRogers, Leslie
dc.contributor.authorCiardi, David
dc.contributor.authorFischer, Debra A.
dc.contributor.authorGilliland, Ronald L.
dc.contributor.authorKjeldsen, H.
dc.contributor.authorChristensen-Dalsgaard, J.
dc.contributor.authorHuber, Daniel
dc.contributor.authorChaplin, William J.
dc.contributor.authorBasu, S.
dc.contributor.authorBuchhave, Lars A.
dc.contributor.authorQuinn, Samuel N.
dc.contributor.authorBorucki, William J.
dc.contributor.authorKoch, David G.
dc.contributor.authorHunter, Roger
dc.contributor.authorCaldwell, Douglas A.
dc.contributor.authorVan Cleve, Jeffrey
dc.contributor.authorKolbl, Rea
dc.contributor.authorWeiss, Lauren M.
dc.contributor.authorPetigura, Erik
dc.contributor.authorSeager, Sara
dc.contributor.authorMorton, Timothy
dc.contributor.authorJohnson, John Asher
dc.contributor.authorBallard, Sarah
dc.contributor.authorBurke, Chris
dc.contributor.authorCochran, William D.
dc.contributor.authorEndl, Michael
dc.contributor.authorMacQueen, Phillip
dc.contributor.authorEverett, Mark E.
dc.contributor.authorLissauer, Jack J.
dc.contributor.authorFord, Eric B.
dc.contributor.authorTorres, Guillermo
dc.contributor.authorFressin, Francois
dc.contributor.authorBrown, Timothy M.
dc.contributor.authorSteffen, Jason H.
dc.contributor.authorCharbonneau, David
dc.contributor.authorBasri, G.
dc.contributor.authorSasselov, Dimitar D.
dc.contributor.authorWinn, Joshua
dc.contributor.authorSanchis-Ojeda, Roberto
dc.contributor.authorChristiansen, Jessie
dc.contributor.authorAdams, Elisabeth
dc.contributor.authorHenze, Christopher
dc.contributor.authorDupree, Andrea
dc.contributor.authorFabrycky, Daniel C.
dc.contributor.authorFortney, Jonathan J.
dc.contributor.authorTarter, Jill
dc.contributor.authorHolman, Matthew J.
dc.contributor.authorTenenbaum, Peter
dc.contributor.authorShporer, Avi
dc.contributor.authorLucas, P.W.
dc.contributor.authorWelsh, William F.
dc.contributor.authorOrosz, Jerome A.
dc.contributor.authorBedding, T.R.
dc.contributor.authorCampante, T.L.
dc.contributor.authorDavies, G.R.
dc.contributor.authorElsworth, Y.
dc.contributor.authorHandberg, R.
dc.contributor.authorHekker, S.
dc.contributor.authorKaroff, C.
dc.contributor.authorKawaler, S.D.
dc.contributor.authorLund, M.N.
dc.contributor.authorLundkvist, M.
dc.contributor.authorMetcalfe, T.S.
dc.contributor.authorMiglio, A.
dc.contributor.authorSilva Aguirre, V.
dc.contributor.authorStello, D.
dc.contributor.authorWhite, T.R.
dc.contributor.authorBoss, Alan
dc.contributor.authorDeVore, E.
dc.contributor.authorGould, Alan
dc.contributor.authorPrsa, A.
dc.contributor.authorAgol, Eric
dc.contributor.authorBarclay, Thomas
dc.contributor.authorCoughlin, Jeff
dc.contributor.authorBrugamyer, Erik
dc.contributor.authorMullally, Fergal
dc.contributor.authorQuintana, Elisa V.
dc.contributor.authorStill, Martin
dc.contributor.authorThompson, Susan E.
dc.contributor.authorMorrison, David
dc.contributor.authorTwicken, Joseph D.
dc.contributor.authorDesert, Jean-Michel
dc.contributor.authorCarter, Josh
dc.contributor.authorCrepp, Justin R.
dc.contributor.authorHebrard, Guillaume
dc.contributor.authorSanterne, Alexandre
dc.contributor.authorMoutou, Claire
dc.contributor.authorSobeck, Charlie
dc.contributor.authorHudgins, Douglas
dc.contributor.authorHaas, Michael R.
dc.contributor.authorRobertson, Paul
dc.contributor.authorLillo-Box, Jorge
dc.contributor.authorBarrado, David
dc.date.accessioned2014-08-28T12:00:46Z
dc.date.available2014-08-28T12:00:46Z
dc.date.issued2014-02-01
dc.identifier.citationMarcy , G W , Isaacson , H , Howard , A W , Rowe , J F , Jenkins , J M , Bryson , S T , Latham , D W , Howell , S B , Gautier , T N , Batalha , N M , Rogers , L , Ciardi , D , Fischer , D A , Gilliland , R L , Kjeldsen , H , Christensen-Dalsgaard , J , Huber , D , Chaplin , W J , Basu , S , Buchhave , L A , Quinn , S N , Borucki , W J , Koch , D G , Hunter , R , Caldwell , D A , Van Cleve , J , Kolbl , R , Weiss , L M , Petigura , E , Seager , S , Morton , T , Johnson , J A , Ballard , S , Burke , C , Cochran , W D , Endl , M , MacQueen , P , Everett , M E , Lissauer , J J , Ford , E B , Torres , G , Fressin , F , Brown , T M , Steffen , J H , Charbonneau , D , Basri , G , Sasselov , D D , Winn , J , Sanchis-Ojeda , R , Christiansen , J , Adams , E , Henze , C , Dupree , A , Fabrycky , D C , Fortney , J J , Tarter , J , Holman , M J , Tenenbaum , P , Shporer , A , Lucas , P W , Welsh , W F , Orosz , J A , Bedding , T R , Campante , T L , Davies , G R , Elsworth , Y , Handberg , R , Hekker , S , Karoff , C , Kawaler , S D , Lund , M N , Lundkvist , M , Metcalfe , T S , Miglio , A , Silva Aguirre , V , Stello , D , White , T R , Boss , A , DeVore , E , Gould , A , Prsa , A , Agol , E , Barclay , T , Coughlin , J , Brugamyer , E , Mullally , F , Quintana , E V , Still , M , Thompson , S E , Morrison , D , Twicken , J D , Desert , J-M , Carter , J , Crepp , J R , Hebrard , G , Santerne , A , Moutou , C , Sobeck , C , Hudgins , D , Haas , M R , Robertson , P , Lillo-Box , J & Barrado , D 2014 , ' Masses, radii, and orbits of small Kepler planets : The transition from gaseous to rocky planets ' , Astrophysical Journal, Supplement Series , vol. 210 , no. 2 , 20 . https://doi.org/10.1088/0067-0049/210/2/20
dc.identifier.issn0067-0049
dc.identifier.otherPURE: 7399843
dc.identifier.otherPURE UUID: b80c77ef-d956-4102-8e35-42436673a1c2
dc.identifier.otherScopus: 84893173199
dc.identifier.otherORCID: /0000-0002-8872-4462/work/62748833
dc.identifier.urihttp://hdl.handle.net/2299/14406
dc.description.abstractWe report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by precise Doppler measurements of the host stars. Based on an analysis of the Kepler brightness measurements, along with high-resolution imaging and spectroscopy, Doppler spectroscopy, and (for 11 stars) asteroseismology, we establish low false-positive probabilities (FPPs) for all of the transiting planets (41 of 42 have an FPP under 1%), and we constrain their sizes and masses. Most of the transiting planets are smaller than three times the size of Earth. For 16 planets, the Doppler signal was securely detected, providing a direct measurement of the planet's mass. For the other 26 planets we provide either marginal mass measurements or upper limits to their masses and densities; in many cases we can rule out a rocky composition. We identify six planets with densities above 5 g cm-3, suggesting a mostly rocky interior for them. Indeed, the only planets that are compatible with a purely rocky composition are smaller than 2 R ⊕. Larger planets evidently contain a larger fraction of low-density material (H, He, and H2O).en
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal, Supplement Series
dc.titleMasses, radii, and orbits of small Kepler planets : The transition from gaseous to rocky planetsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/0067-0049/210/2/20
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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