Detecting Exoplanets by Gravitational Microlensing using a Small Telescope

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dc.creatorChristie, G. W.
dc.date2006-09-21
dc.date.accessioned2026-07-07T07:23:18Z
dc.date.available2026-07-07T07:23:18Z
dc.descriptionGravitational microlensing is a new technique that allows low-mass exoplanets to be detected at large distances of ~7kpc. This paper briefly outlines the principles of the method and describes the observational techniques. It shows that small (e.g. 0.35m) telescopes with a CCD camera can make unexpectedly useful observations of these events.
dc.description8 pages, 4 figures, Society for Astronomical Science (May 2006)
dc.identifierhttps://arxiv.org/abs/astro-ph/0609599
dc.identifierhttp://arxiv.org/abs/astro-ph/0609599
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115933
dc.subjectAstrophysics
dc.titleDetecting Exoplanets by Gravitational Microlensing using a Small Telescope
dc.typetext

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