Prospects from TESS and Gaia to constrain the flatness of planetary systems

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dc.catalogadorpau
dc.contributor.authorEspinoza Retamal, Juan
dc.contributor.authorZhu, Wei
dc.contributor.authorPetrovich, Cristobal
dc.date.accessioned2023-09-29T19:11:40Z
dc.date.available2023-09-29T19:11:40Z
dc.date.issued2023
dc.description.abstractThe mutual inclination between planets orbiting the same star provides key information to understand the formation and evolution of multi-planet systems. In this work, we investigate the potential of Gaia astrometry in detecting and characterizing cold Jupiters in orbits exterior to the currently known TESS planet candidates. According to our simulations, out of the $\sim 3350$ systems expected to have cold Jupiter companions, Gaia, by its nominal 5-year mission, should be able to detect $\sim 200$ cold Jupiters and measure the orbital inclinations with a precision of $\sigma_{\cos i}
dc.fechaingreso.objetodigital2023-09-27
dc.format.extent11 páginas
dc.fuente.origenORCID
dc.identifier.doi10.48550/arXiv.2309.08665
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/74805
dc.information.autorucInstituto de Astrofísica; Espinoza Retamal, Juan; S/I; 1025598
dc.information.autorucInstituto de Física; Petrovich, Cristobal; S/I; 131196
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.subjectExoplanets
dc.subjectExoplanet catalogs
dc.subjectSpace astrometry
dc.subjectExoplanet migration
dc.subjectExtrasolar gaseous planets
dc.subject.ddc510
dc.subject.deweyMatemática física y químicaes_ES
dc.titleProspects from TESS and Gaia to constrain the flatness of planetary systems
dc.typedocumento de trabajo
sipa.codpersvinculados1025598
sipa.codpersvinculados131196
sipa.trazabilidadORCID;2023-09-25
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