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Hi I'm a student working with @stephtdouglas measuring periods for binaries. For stars of short periods, the original rejection sampling (without MCMC) is resulting in short eccentricities which is what we are expecting. However, when MCMC is done on stars with 1 rejection sample and with short periods, the orbits are being pushed towards higher eccentricities. This is occurring on 7 stars in our sample.
Below is an example of this, a star with a Gaia ID of 2128124963389008384.
This is the period vs eccentricity plot after rejection sampling

This is the period vs eccentricity after MCMC

Here is the script I am using
https://github.com/ella918/Summer-Research/blob/main/RunTheJokerOnePrior.py
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