v0.2.4

Changed

• Extend support for up to two colors.
• Improved performance (#357):
  • Make mass sampling optional (#373)
  • Move binarity assignment outside of the synthetic cluster generation
  • Move isochrone sorting outside of the synthetic cluster generation
  • Move random floats for photometric errors outside of the synthetic cluster generation
  • Move random floats for completeness outside of the synthetic cluster generation. Code is now ~3.3X faster

v0.2.3

Changed

• Improved performance of synthetic cluster generation (#227). Code is now ~4X faster.
• Fix excessive use of memory by Rbf interpolation (#350)
• Use equal bin widths in LF and completeness function (#300)
• Faster star separation by errors (#351)
• Generalize Bayesian DA to N-dimensions, fix statistical issues, improve performance (#352)

v0.2.2

Changed

• Add weights to binned likelihood (#216)
• Fix bug in progress bar.
• Identify binaries in plotted HR diagram.
• Modify the information presented by the 2-parameters density plots. Takes care of #71.
• Smarter empty field region around cluster region (#345).
• Detect stars with duplicate IDs in data file (#212).

v0.2.1

Changed

• Fix issue with tolstoy likelihood estimation (#340)
• Fix a couple of issues with the error curve fitting (#338)
• Add 'fixed' MPs algorithm (useful when no field region is available) (#326)
• Fix crash when obtaining error curve (#256)

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)

v0.1.9.5

Changed

• Remove forgotten print line.
• Print relevant information when data con not be read (#262).
• Fix bad range issue (#226).

v0.1.9.4

Changed

• Add support for five tracks from the CMD service (#276).
• Read metallicity files with underscores instead of decimal dots (#277).
• Several important structural changes (#273): add first_run check, re-arrange and re-name modules, and move almost every part of the code into the packages/ folder.

v0.1.9.3

Changed

• Add support for CMD in the HST/ACS WFC photometric system (requested by Daniel Arbeláez).

v0.1.9.2

Changed

• Add support for three CMDs in the Strömgren photometric system (requested by J. Hughes Clark).
• Change likelihood density plots to scatter plots which show more information.
• Add extra condition for DA break: minimum 10% of the runs must have passed.
• Fix bug with 'mag' mode in 'Reduced membership', wouldn't run if the Bayesian DA was skipped.
• Fix minor bug (#241) when printing KP results to screen.

v0.1.9.1

Changed

• Fixed rounding of errors that returned 0. values if error was larger than value (#213).
• Check if pip module is installed + search for installed packages globally, not locally.
• Catch badly formatted input data file.
• Restructure King radii obtention.
• Correctly plot stars in cluster region, not used in best fit function.