The Transits of Extrasolar Planets with Moons by David M. Kipping

Author:David M. Kipping
Language: eng
Format: epub
Publisher: Springer Berlin Heidelberg, Berlin, Heidelberg

2.Multiply all flux values by

3.Subtract from all data points.

In practice, these steps are incorporated into the light curve fitting algorithm directly. In the case of using Monte Carlo based routines for error estimation, may be floated around its best-fit value and corresponding uncertainty. An example of this method is shown in Sect. 5.2.5 for the planet HD 189733b. Defining as the locally normalized flux measurement of the data point, one may explicitly write down the corrected data point using (5.8).

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