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Hello! I am currently attempting to use BATMAN for light curve fitting using nonlinear limb darkening coefficients. In pursuit of this, I am doing an MCMC (thanks emcee) analysis which, of course, rel…
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Introduce a selection of stellar models surrounding the input values rather than the closest model. This will create a grid of 8 models, two for [M/H], two for Teff, and two for logg. Then use triline…
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I created a [new use case](https://github.com/rpoleski/MulensModel/blob/bce909412a676e15286d985a498db461ae6d0ca1/examples/example_25_LD.py) for passing limb-darkening coefficients to models and propos…
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Hi @hpparvi - I am trying to run your ldtk example notebook in Python 3.7. When I do so, I receive the attached errors. Also below are the dependencies of my ldtk python install. Could you help me…
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When there are a large number of limb-darkening coefficients, the computation becomes inaccurate. Not sure why, but some possible problems/solutions:
- [x] The `d_n` (now `g_n`) values become lar…
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Hi Ian, Ryan, and Jeff,
This is a follow-up to our meeting today. We discussed the idea of adding parametric models of solar system bodies to operate in series with the rest of the non-parametric …
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Submitting Author: JJ (@AUTHOR_GITHUB_HANDLE)
Repository: https://github.com/KathrynJones1/catwoman
Version submitted: 3.3
Editor: @xuanxu
Reviewers: @gemgon
Due date for @gemgon: 20…
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### Background
I'm working on simultaneously fitting optical transits, eclipses and reflected light phase curves of exoplanets via `exoplanet`, and `exoplanet` has been working beautifully (so than…
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### Instrument
Light curve fitting (Stages 4-6)
### What happened?
To me the reasonable thing would be to calculate limb darkening coefficients during stage 4, in order to "fix" the limb dark…
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### FAQ check
- [X] Yes, I checked the FAQ and my question has not been addressed.
### Instrument
Light curve fitting (Stages 4-6)
### What happened?
I installed the latest version:
…