dc.date.accessioned | 2020-03-11T20:32:22Z | |
dc.date.accessioned | 2022-10-18T22:53:44Z | |
dc.date.available | 2020-03-11T20:32:22Z | |
dc.date.available | 2022-10-18T22:53:44Z | |
dc.date.created | 2020-03-11T20:32:22Z | |
dc.date.issued | 2009 | |
dc.identifier | http://hdl.handle.net/10533/239704 | |
dc.identifier | 15010003 | |
dc.identifier | WOS:000271149700002 | |
dc.identifier | no scielo | |
dc.identifier | eid=2-s2.0-70450200209 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4471043 | |
dc.description.abstract | To 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.language | eng | |
dc.relation | https://doi.org/10.1088/0004-637X/705/2/1116 | |
dc.relation | 10.1088/0004-637X/705/2/1116 | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
dc.title | Interpretation of Strong Short-Term Central Perturbations in the Light Curves of Moderate-Magnification Microlensing Events | |
dc.type | Articulo | |