JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.
Estimating the Dimension of a Model.Ann
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A tutorial on Bayesian parameter estimation, model selection, and extrapolation with uncertainty for temperature-dependent diffusion and conductivity data from molecular dynamics.
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The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.
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Bayesian Methods for the Investigation of Temperature-Dependence in Conductivity
A tutorial on Bayesian parameter estimation, model selection, and extrapolation with uncertainty for temperature-dependent diffusion and conductivity data from molecular dynamics.