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dc.contributor.authorCagigas García, Miguel Ángel 
dc.contributor.authorPérez Cagigal, Manuel 
dc.contributor.authorValle Herrero, Pedro José 
dc.contributor.authorFernández Canales, Vidal 
dc.contributor.authorFuentes, Antonio
dc.contributor.authorLópez, Roberto
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-03-07T14:47:04Z
dc.date.available2024-03-07T14:47:04Z
dc.date.issued2019-07
dc.identifier.issn0035-8711
dc.identifier.otherAYA2016-78773-C2-1-P
dc.identifier.urihttps://hdl.handle.net/10902/32121
dc.description.abstractIn this paper, we review two different methods to increase image contrast and propose the combination of both to detect faint companions surrounding a host star. Coronagraphy allows us to block light coming from the host star so that the residual star light can be reduced by several orders of magnitude. On the other hand, estimating the Covariance of Lucky Images (COELI) is a proven method to detect faint companions from ground-based telescope images. The dynamic range of the detection camera limits this technique. Hence, the application of COELI to coronagraphic images may increase the magnitude range of the detectable companions. COELI only requires the existence of a reference, which can be obtained using an existing stellar companion or using a coronagraphic mask designed to create a faint image of the host star.We provide an analysis of the combination of the techniques by processing coronagraphic images obtained by the William Herschel Telescope.es_ES
dc.description.sponsorshipWe acknowledge funding from Ministerio de Economía y Competitividad, project AYA2016-78773-C2-1-P.es_ES
dc.format.extent6es_ES
dc.language.isoenges_ES
dc.rights© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societyes_ES
dc.sourceMNRAS, 2019, 488(3), 3262-3267es_ES
dc.subject.otherMethods: statisticales_ES
dc.subject.otherTechniques: image processinges_ES
dc.subject.otherTelescopeses_ES
dc.titlePlanetary system detection by estimating the covariance of coronagraphic lucky imageses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1093/mnras/stz1954es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOIhttps://doi.org/10.1093/mnras/stz1954
dc.type.versionpublishedVersiones_ES


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