dc.date.accessioned2020-03-11T20:32:22Z
dc.date.accessioned2022-10-18T22:53:44Z
dc.date.available2020-03-11T20:32:22Z
dc.date.available2022-10-18T22:53:44Z
dc.date.created2020-03-11T20:32:22Z
dc.date.issued2009
dc.identifierhttp://hdl.handle.net/10533/239704
dc.identifier15010003
dc.identifierWOS:000271149700002
dc.identifierno scielo
dc.identifiereid=2-s2.0-70450200209
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4471043
dc.description.abstractTo improve the planet detection efficiency, current planetary microlensing experiments are focused on high-magnification events searching for planetary signals near the peak of lensing light curves. However, it is known that central perturbations can also
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/705/2/1116
dc.relation10.1088/0004-637X/705/2/1116
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleInterpretation of Strong Short-Term Central Perturbations in the Light Curves of Moderate-Magnification Microlensing Events
dc.typeArticulo


Este ítem pertenece a la siguiente institución