A new statistical method for characterizing the atmospheres of extrasolar planets
Henderson et al
By detecting light from extrasolar planets,we can measure their compositions and bulk physical properties. The technologies used to make these measurements are still in their infancy, and a lack of self-consistency suggests that previous observations have underestimated their systemic errors.We demonstrate a statistical method, newly applied to exoplanet characterization, which uses a Bayesian formalism to account for underestimated errorbars. We use this method to compare photometry of a substellar companion, GJ 758b, with custom atmospheric models. Our method produces a probability distribution of atmospheric model parameters including temperature, gravity, cloud model (fsed), and chemical abundance for GJ 758b. This distribution is less sensitive to highly variant data, and appropriately reflects a greater uncertainty on parameter fits.
Friday, September 29, 2017
A new statistical method for characterizing the atmospheres applied to brown dwarf GJ 758B
Posted by Will Baird at 8:00 AM
Labels: brown dwarf, exoatmosphere, GJ 758B, gliese 758B, T class, T Dwarf
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