v0.1.7
Changed
(Warning: this release breaks compatibility with the previous version of the params_input.dat
file)
- Re-write
lowexp
error rejection method, now uses prediction bands instead of confidence intervals. - Force
matplotlib
's backend to make the code work in servers . - Fixed
eyefit
method for error rejection. It changed after fixing #169. - Added SDSS CMDs
g vs (u-g)
&g vs (g-r)
, at the request of Tjibaria Pijloo (Department of Astrophysics, Radboud University Nijmegen). - Fixed bug in binarity generation for the CMDs of the form
X vs (X-Y)
(#181). - Smarter selection of stars to be used by the best fit function, improvements in several plots (#171, #172).
- Best fit function can now accept a minimum magnitude value instead of just a minimum probability value (#115).
- Added a
memb_par
parameter to compare the number of approximate cluster members obtained via the structural analysis and via the decontamination algorithm (#162). - Code is now able to correctly read the names of files with more than one dot in it's name.
- Fixed bad alphabetical ordering of input cluster files.
- Better limits for photometric diagram (#173).
- Fixed
DeprecationWarning
issue. - Invert x axis when RA cords are used (improved here).
- Several fixes and improvements made to plotted diagrams (5c7dc7f; 1642349; b57028c; 240178a; 9ec0ab8; fef14c4; db0df2a; 575ebe7; #177; #178).
Caveats
- Same as version 0.1.2.