Release 3.1
Bug fixes:
- Multinesting previously used ln_prob while nestle expected ln_like, causing posteriors to be narrower and closer to the prior for parameters with Gaussian priors.
- For multinesting, the previously reported best fit was the fit with the highest likelihood, not the one with the highest posterior probability. The latter is correct.
- set_from_arrays in T/P profile was previously broken
Improvements:
- Fixed problem in opacities for HITRAN molecules (C2H2, C2H6, CO2, HF, N2, NO2, O2, O3, OCS) plus carbon monoxide where the Voigt cutoff was 25 cm^-1 even for high pressures. It is now 100 cm^-1 for 10 and 100 bar, and 1000 cm^-1 for 1000 bar. Also, HITRAN opacities now include all isotopologues.
- Na and K opacities are now calculated from NIST line data.
- The radius used in eclipse depth calculations is now the radius where the radial optical depth is 1. Previously, it was the radius where P = 1 bar.
- Unbinned transit and eclipse depths are now plotted with alpha=0.2, to prevent blocking everything else from view