Detecting Extra-Solar Planets via Microlensing at High Magnification

Details Detecting Extra-Solar Planets via Microlensing at High Magnification Detecting Extra-Solar Planets via Microlensing at High Magnification

2002-09-09

arxiv.org/abs/astro-ph/0209138v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures. Presented at the Scientific Frontiers in Research on Extra-Solar Planets conference, Washginton D.C., June

Scientific paper

Extra-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.

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