juliet
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A versatile modelling tool for transiting and non-transiting (single and multiple) exoplanetary systems
Hi @nespinoza, If I try to use `nthreads` option in `juliet.fit` for using multiprocessing with `dynesty`, I would get the following error: ``` RuntimeError: An attempt has been made to...
In more recent Python versions, checking `var is "string"` raises a warning (you should use `==` for string comparison). This fixes the two places that were raising this warning when...
I am analyzing some new detections with Juliet and one of them is in grazing transit. As a result the depth and impact parameter are correlated and they look kind...
Hello, I came across the same error as in Issue #81 that occurs when fitting more than one planet with TTVs. In setting the lightcurve prior dict, when a transit...
Hi Nestor, There is an error when trying to use juliet to fit transit times of more than one planet. The issue is in line 568 of fit.py. This line...
Hola Nestor! I got the following error when doing the fit using a free eccentricity but a fixed omega: `~/anaconda3/envs/juliet/lib/python3.8/site-packages/juliet/utils.py in writepp(fout, posteriors, priors) 582 elif 'ecc_'+planet in posteriors['posterior_samples']: 583...
After a fit is done, I would like to have access to the typical parameters which are derived from the fit, that is, a/R*, inclination, orbital semimajor axis, transit duration...
Dear Nestor Is it possible to reach every single transit depth, in order to every single r_1 and r_2? thank you Mohammad
With added caveat for `zeus`: https://github.com/minaskar/zeus/issues/18