Releases: asteca/ASteCA
Releases · asteca/ASteCA
v0.1.0
First semi-stable buggy release
Changed
- Closed #72, #99, #37.
- Changed the way the IMF was sampled, 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_errfunction isn't used (fixed in next release). - Forgotten
printprints out mass values every time the E/I operator is applied (fixed 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 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.
v4.0.0-beta
v3.0.0-beta
v2.0.1-beta
Changed
- Correct version number.
v2.0.0-beta
Changed
- Closed issues: #15, #73, #53, #24, #75, #79, #81, #59, #83, #78, #69, #74.
- Changed name of package (OCAAT --> ASteCA).
- Added separate function to handle the spatial 2D histogram.
- Changes to
get_centerfunction (now hopefully simpler) - Added UBVI support for V vs (U-V).
- Added 2MASS CMD support for J vs (J-H), H vs (J-H) and K vs (H-K).
- Improve field star regions integrated magnitudes curve averaging.
- Simplify process of adding a new CMD.
- Added details on how the integrated magnitude calculation is done in the manual.
- Lots of minor edits/corrections.
v1.0.0-beta
First beta release
Version used (with some small changes) in the original article.