_First ~~semi-stable~~ buggy release_
Changed
- Closed 72, 99, 37.
- Changed the way the IMF was [sampled](https://github.com/Gabriel-p/asteca/commit/0671e74c52fbecde6bcbb1afb1c2624875156e57), now it should be faster and more precise.
- Some speed improvements (moved things around mainly).
- Binary fraction is now a free parameter.
Known issues
- **Serious bug**: if the DA is set to run but the _Best fit method_ isn't, the final plot can't be produced since the `syn_cl_err` function isn't used ([fixed](https://github.com/Gabriel-p/asteca/commit/3e806bd0af5d7fcd7c8f2940716df880f4c1b67d) in next release).
- Forgotten `print` prints out mass values every time the E/I operator is applied ([fixed](https://github.com/Gabriel-p/asteca/commit/8b313ef60fddccc41fd6fb7b9746f75f3e867d39) in next release).
- If the number of points (`n_left`) in the radius finding function is smaller than 4, a very small radius is likely
to be selected. [Fixed](https://github.com/Gabriel-p/asteca/commit/c247fd7fa4cca4d6bb341263434a4a43a4778efd) in next release.
Caveats
- The total initial mass can be set as a free parameter but the likelihood function will select always synthetic clusters of high mass. Thus it is advised to leave this parameter fixed to 1000 solar masses.
- The binary fraction found is not stored in the output data file.
- Some density map plots for mass and binary fraction are missing.