juliet
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A versatile modelling tool for transiting and non-transiting (single and multiple) exoplanetary systems
For fitting secondary eclipse, How could I set parameter of 'r1_p1','r2_p1" ?
Hi, I recently struggled a while because juliet wasn't running correctly to find out that the light curve file had a single nan point, maybe it could be useful for...
Currently, `juliet` runs but doesn't produce any samples if some parameters are fixed to unphysical values (e.g., `a_p1 < 1`). A good enhancement would be for `juliet` to check for...
I think it would be a good idea to add the derived parameters (e.g. p and b when using r1 and r2) to the results.posteriors dictionary, which can be a...
I found the automated plots that the older (command line) version of juliet made very helpful. Could these be ported over to commands or just part of some of the...
If I have a gaussian process where all parameters are fixed, it seems that currently the GP is recomputed. How can I disable this unnecessary and costly recomputation? I want...
I think there may be an error in the computation of the binned errors when errors are provided. The current formula is: ``` y_err_bins.append( np.sqrt( np.sum( yerr[i: i + n_bin...
- [ ] Put it in the code. - [ ] Raise error in the code. - [ ] Put it in the documentation.
I'm trying to fit a transit using r1, r2, and rho parameters. The posteriors.dat has an estimation of the semimajor axis (a) and the impact parameter (b), as well as...