Detecting Extra-Solar Planets via Microlensing at High Magnification

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dc.creatorRattenbury, Nicholas J.
dc.creatorBond, Ian A.
dc.creatorSkuljan, Jovan
dc.creatorYock, Phil
dc.date2002-09-09
dc.date.accessioned2026-07-07T02:05:02Z
dc.date.available2026-07-07T02:05:02Z
dc.descriptionExtra-solar planets can be efficiently detected in gravitational microlensing events of high magnification. High accuracy photometry is required over a short, well-defined time interval only, of order 10-30 hours. Most planets orbiting the lens star are evidenced by perturbations of the microlensing light curve in this time.
dc.description4 pages, 2 figures. Presented at the Scientific Frontiers in Research on Extra-Solar Planets conference, Washginton D.C., June 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0209138
dc.identifierhttp://arxiv.org/abs/astro-ph/0209138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4983
dc.subjectAstrophysics
dc.titleDetecting Extra-Solar Planets via Microlensing at High Magnification
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