Changed
* Generalized code to accept an arbitrary CMD in any _single_ photometric system supported by the [CMD service](http://stev.oapd.inaf.it/cgi-bin/cmd) ([#24][15]).
* Identify binary systems in synthetic clusters ([199][16]).
* Plots are now produced per blocks, instead of all together at the end ([271][17])
* Switch dependency requirement from astroML to astropy ([303][18]).
* Remove unused error rejection modes ([331][1])
* Simplify params_input.dat file ([217][2])
* Check that all metallicity files contain the same number of age values ([218][19])
* Add density maps analysis for center function ([164][3])
* Remove weight added to the observed cluster CMD's histogram ([308][4])
* Fix bad parameter rounding ([248][5])
* Add 'max mag' cut for synthetic clusters ([302][6], [264][7])
* Simplify installation steps ([88][8], [315][9])
* Plot results of brute force minimization ([100][10])
* Make extinction parameter Rv a manual input parameter ([314][11])
* Use numpy's binning methods ([317][12])
* Modify RDP limit ([294][13])
* Store extra data from theoretical isochrones ([201][14])
[1]: https://github.com/asteca/ASteCA/issues/331
[2]: https://github.com/asteca/ASteCA/issues/217
[3]: https://github.com/asteca/ASteCA/issues/164
[4]: https://github.com/asteca/ASteCA/issues/308
[5]: https://github.com/asteca/ASteCA/issues/248
[6]: https://github.com/asteca/ASteCA/issues/302
[7]: https://github.com/asteca/ASteCA/issues/264
[8]: https://github.com/asteca/ASteCA/issues/88
[9]: https://github.com/asteca/ASteCA/issues/315
[10]: https://github.com/asteca/ASteCA/issues/100
[11]: https://github.com/asteca/ASteCA/issues/314
[12]: https://github.com/asteca/ASteCA/issues/317
[13]: https://github.com/asteca/ASteCA/issues/294
[14]: https://github.com/asteca/ASteCA/issues/201
[15]: https://github.com/asteca/ASteCA/issues/24
[16]: https://github.com/asteca/ASteCA/issues/199
[17]: https://github.com/asteca/ASteCA/issues/271
[18]: https://github.com/asteca/ASteCA/issues/303
[19]: https://github.com/asteca/ASteCA/issues/218