{"push_id":634328065,"size":1,"distinct_size":1,"ref":"refs/heads/calculations","head":"2b1ed5f7b8e531413d1da5db1081d81e56a8848a","before":"feea64148174ad0ae8b520741ca695972cd5f1e4","commits":[{"sha":"2b1ed5f7b8e531413d1da5db1081d81e56a8848a","author":{"email":"a65e5d71c2fa087c831cba1d392bb8f43fc102a6@princeton.edu","name":"unknown"},"message":"Many updates!  This version of transitfunctions has had some corrections made: primaries for planetary systems are drawn from a Gaussian distribution centered about solar mass and radius for the primary masses and radii.  Randomization is now done using a bootstrap-ish technique (sampling with replacement). Tau has also been set to have a minimum value of 30 minutes.  Plotting has also been updated!  Can now plot a series of populations over varied period and/or eccentricity distributions.","distinct":true,"url":"https://api.github.com/repos/lavjams/VESPA/commits/2b1ed5f7b8e531413d1da5db1081d81e56a8848a"}]}