The detection of gravitational microlensing anomalies
Master Thesis
1999
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University of Cape Town
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Abstract
The detection and measurability of microlensing anomalies including planet detection, resolved source, blending and parallax effects are investigated by way of an extensive computer simulation as a function of the observation strategy. The most efficient strategy has a planet detection probability exceeding 753 for the most favourable binary geometry, while results for typical event follow up and survey observations agree well with previous work. A complex dependence of planet detection on the resolved source radius is discovered leading to a possible increase in the probability of detecting planets with mass ratios smaller than q = 10⁻³
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Bibliography: pages 100-104.
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Reference:
Vermaak, P. 1999. The detection of gravitational microlensing anomalies. University of Cape Town.