Releases
v0.2.0
Changed
Generalized code to accept an arbitrary CMD in any single photometric system supported by the CMD service (#24 ).
Identify binary systems in synthetic clusters (#199 ).
Plots are now produced per blocks, instead of all together at the end (#271 )
Switch dependency requirement from astroML to astropy (#303 ).
Remove unused error rejection modes (#331 )
Simplify params_input.dat file (#217 )
Check that all metallicity files contain the same number of age values (#218 )
Add density maps analysis for center function (#164 )
Remove weight added to the observed cluster CMD's histogram (#308 )
Fix bad parameter rounding (#248 )
Add 'max mag' cut for synthetic clusters (#302 , #264 )
Simplify installation steps (#88 , #315 )
Plot results of brute force minimization (#100 )
Make extinction parameter Rv a manual input parameter (#314 )
Use numpy's binning methods (#317 )
Modify RDP limit (#294 )
Store extra data from theoretical isochrones (#201 )
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