Abstract
If stars were uniformly bright across their surfaces, then the analysis of transit observations would require only the subtraction of this bright background from the observed data in order to obtain the transit light curve and the absorption spectrum produced by atoms and molecules in the exoplanet’s atmosphere. Even this unrealistically simple observing scenario is a data analysis challenge because the area of a transiting planet may be only 1% or smaller compared to that of the host star, and the area of a terrestrial exoplanet’s atmosphere seen in absorption against the stellar disk emission may be only 0.01% that of the stellar disk area. Thus high signal/noise data are essential to minimize random noise.
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Linsky, J. (2019). The Effects of Heterogeneous Stellar Surfaces on the Analysis of Exoplanet Transit Light Curves and Spectra. In: Host Stars and their Effects on Exoplanet Atmospheres . Lecture Notes in Physics, vol 955. Springer, Cham. https://doi.org/10.1007/978-3-030-11452-7_13
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