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Detecting Exoplanets by Gravitational Microlensing using a Small Telescope

2006/09/21 by G. W. Christie, Christie, G. W.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0609599

8 pages, 4 figures, Society for Astronomical Science (May 2006)

arxiv created 2006/09/21 · arxiv updated 2009/12/01

Abstract

Gravitational 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.

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