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Wide-Orbit Exoplanet Demographics

dc.contributor.authorBENNETT, David P.
dc.contributor.authorAKESON, Rachel
hal.structure.identifierLaboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) [LAOB]
dc.contributor.authorALIBERT, Yann
dc.contributor.authorANDERSON, Jay
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorBACHELET, Etienne
dc.contributor.authorBEAULIEU, Jean-Phillipe
dc.contributor.authorBELLINI, Andrea
dc.contributor.authorBHATTACHARYA, Aparna
dc.contributor.authorBOSS, Alan
dc.contributor.authorBOZZA, Valerio
dc.contributor.authorBRYSON, Stephen
dc.contributor.authorBUZASI, Derek
dc.contributor.authorCALCHI NOVATI, Sebastiano
dc.contributor.authorCHRISTIANSEN, Jessie
dc.contributor.authorDOMAGAL-GOLDMAN, Shawn D.
hal.structure.identifierMcDonald Observatory
dc.contributor.authorENDL, Michael
dc.contributor.authorFULTON, Benjamin J.
dc.contributor.authorHENDERSON, Calen B.
dc.contributor.authorGAUDI, B. Scott
dc.contributor.authorJOHNSON, Samson A.
dc.contributor.authorKOSHIMOTO, Naoki
hal.structure.identifierLiquides Ioniques et Interfaces Chargées [LI2C]
dc.contributor.authorMEYER, Michael
dc.contributor.authorMULDERS, Gijs D.
dc.contributor.authorMULLALLY, Susan
dc.contributor.authorMURRAY-CLAY, Ruth
dc.contributor.authorNATAF, David
dc.contributor.authorNIELSEN, Eric
dc.contributor.authorNGO, Henry
dc.contributor.authorPASCUCCI, Ilaria
dc.contributor.authorPENNY, Matthew
dc.contributor.authorPLAVCHAN, Peter
dc.contributor.authorPOLESKI, Radek
dc.contributor.authorRANC, Clement
hal.structure.identifierECLIPSE 2019
dc.contributor.authorRAYMOND, Sean N.
dc.contributor.authorROGERS, Leslie
dc.contributor.authorSAHLMANN, Johannes
dc.contributor.authorSAHU, Kailash C.
dc.contributor.authorSCHLIEDER, Joshua
dc.contributor.authorSHVARTZVALD, Yossi
dc.contributor.authorSOZZETTI, Alessandro
dc.contributor.authorSTREET, Rachel
dc.contributor.authorSUMI, Takahiro
dc.contributor.authorSUZUKI, Daisuke
dc.contributor.authorZIMMERMAN, Neil
dc.date.issued2019
dc.identifier.issn0002-7537
dc.description.abstractEnThe Kepler, K2 and TESS transit surveys are revolutionizing our understanding of planets orbiting close to their host stars and our understanding of exoplanet systems in general, but there remains a gap in our understanding of wide-orbit planets. This gap in our understanding must be filled if we are to understand planet formation and how it affects exoplanet habitability. We summarize current and planned exoplanet detection programs using a variety of methods: microlensing (including WFIRST), radial velocities, Gaia astrometry, and direct imaging. Finally, we discuss the prospects for joint analyses using results from multiple methods and obstacles that could hinder such analyses. We endorse the findings and recommendations published in the 2018 National Academy report on Exoplanet Science Strategy. This white paper extends and complements the material presented therein.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.title.enWide-Orbit Exoplanet Demographics
dc.typeArticle de revue
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.journalBulletin of the American Astronomical Society
bordeaux.pageid. 505
bordeaux.volume51
bordeaux.issue3
bordeaux.peerReviewedoui
hal.identifierhal-02078061
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02078061v1
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