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A general photodynamical code for exoplanet light curves

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Currently four orders of magnitude (!!!) slower than the Mandel and Agol model because I'm solving for the points of intersection between the planet and the concentric circles numerically. This...

help wanted

I am using Ubuntu: $ uname -a Linux dl 4.13.0-36-generic #40~16.04.1-Ubuntu SMP Fri Feb 16 23:25:58 UTC 2018 x86_64 x86_64 x86_64 GNU/Linux When I tried to install planetplanet: $pip install...

There's actually a sign ambiguity in the expression on [this line](https://github.com/rodluger/planetplanet/blob/3887d4de4771e09249358507286d77298dc08092/planetplanet/photo/eyeball.c#L829)! This leads to the incorrect points of intersection with the occultor in some cases. Should have led to bugs,...

bug

I think my integration method is more general than I had realized. Currently, because I'm restricting my calculations to ellipses, I need the radiance map to be radially symmetric about...

v2

I'm currently working on this! It will be the *mcmc_example.py* script in *scripts/*.

todo

If we're interested in finding the next PPO among two planets, we need to integrate the system forward in time from the current state in order to plot its light...

v2

Currently I am passing tons of arguments to functions such as `NBody` and `OccultedFlux`. These should be folded into structs to make the code friendlier and easier to modify.

v2

Exomoons can now be modeled with the code, but there is still a small issue with the NBody integrator: my Keplerian subgrid isn't working, so the NBody code has to...

v2

We may wish to generalize the code to include reflected light, particularly for phase curve modeling. Shouldn't be too hard to do.

v2