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Authordc.contributor.authorMeshkat, Tiffany 
Authordc.contributor.authorMawet, Dimitri 
Authordc.contributor.authorBryan, Marta L. 
Authordc.contributor.authorHinkley, Sasha 
Authordc.contributor.authorBowler, Brendan P. 
Authordc.contributor.authorStapelfeldt, Karl R. 
Authordc.contributor.authorBatygin, Konstantin 
Authordc.contributor.authorPadgett, Deborah 
Authordc.contributor.authorMorales, Farisa Y. 
Authordc.contributor.authorSerabyn, Eugene 
Authordc.contributor.authorChristiaens, Valentin 
Authordc.contributor.authorBrandt, Timothy D. 
Authordc.contributor.authorWahhaj, Zahed 
Admission datedc.date.accessioned2018-05-30T13:30:24Z
Available datedc.date.available2018-05-30T13:30:24Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationThe Astronomical Journal, 154:245 (21pp), 2017 Decemberes_ES
Identifierdc.identifier.other10.3847/1538-3881/aa8e9a
Identifierdc.identifier.urihttp://repositorio.uchile.cl/handle/2250/148332
Abstractdc.description.abstractWe describe a joint high-contrast imaging survey for planets at the Keck and Very Large Telescope of the last large sample of debris disks identified by the Spitzer Space Telescope. No new substellar companions were discovered in our survey of 30 Spitzer-selected targets. We combine our observations with data from four published surveys to place constraints on the frequency of planets around 130 debris disk single stars, the largest sample to date. For a control sample, we assembled contrast curves from several published surveys targeting 277 stars that do not show infrared excesses. We assumed a double power-law distribution in mass and semimajor axis (SMA) of the form f(m, a) = Cm(alpha)a(beta), where we adopted power-law values and logarithmically flat values for the mass and SMA of planets. We find that the frequency of giant planets with masses 5-20 M-Jup and separations 10-1000 au around stars with debris disks is 6.27% (68% confidence interval 3.68%-9.76%), compared to 0.73% (68% confidence interval 0.20%-1.80%) for the control sample of stars without disks. These distributions differ at the 88% confidence level, tentatively suggesting distinctness of these samples.es_ES
Patrocinadordc.description.sponsorshipExoplanetary Science Initiative at the Jet Propulsion Laboratory, California Institute of Technology / Jet Propulsion Laboratory (JPL) - NASA through the Sagan Fellowship Program / NASA through Hubble Fellowship grant - Space Telescope Science Institute, HST-HF2-51369.001-A / NASA, NAS5-26555 / W.M. Keck Foundationes_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherIOP Publishing Ltd.es_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceThe Astrophysical Journales_ES
Keywordsdc.subjectCircumstellar matteres_ES
Keywordsdc.subjectMethods statisticales_ES
Keywordsdc.subjectPlanets and satellites detectiones_ES
Keywordsdc.subjectTechniques high angular resolutiones_ES
Títulodc.titleA direct imaging survey of spitzer-detected debris disks: occurrence of giant planets in dusty systemses_ES
Document typedc.typeArtículo de revistaes_ES
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile