Typo fixed in StarModel._make_samples() Bug fixed in StarModel.triangle() when distance is not being fit for. Apologies to anyone trying to keep up with all these rapid changes...hopefully this will settle down shortly
Important functional changes included here are that now priors on distance and metallicity are inclu...
Isochrone fitting can be used for estimating stellar parameters which are not directly observable. T...
We continue our series of papers on open cluster distances by comparing multicolor photometry of sin...
Fixed a few bugs from initial release. Isochrone object can now be called with distance and AV argu...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
New in this release: Added BinaryStarModel object, which enables fitting photometry to a model of ...
This is a minor bugfix release. Makes sure HDF files do not remain open after StarModel.load_hdf. A...
Fixed a bug with building the samples dataframes for BinaryStarModel and TripleStarModel. Add some f...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
This release fixes a bug in which photometric bands were sometimes not getting loaded appropriately ...
Big changes to how StarModel fits happen now---fitting now defaults to using MultiNest via PyMultiNe...
Support has now been added to include parallax (in miliarcsec) to the observable properties of a Sta...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
First release of version 1.0. Significant changes from previous versions. MIST models are now avai...
Important functional changes included here are that now priors on distance and metallicity are inclu...
Isochrone fitting can be used for estimating stellar parameters which are not directly observable. T...
We continue our series of papers on open cluster distances by comparing multicolor photometry of sin...
Fixed a few bugs from initial release. Isochrone object can now be called with distance and AV argu...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
New in this release: Added BinaryStarModel object, which enables fitting photometry to a model of ...
This is a minor bugfix release. Makes sure HDF files do not remain open after StarModel.load_hdf. A...
Fixed a bug with building the samples dataframes for BinaryStarModel and TripleStarModel. Add some f...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
This release fixes a bug in which photometric bands were sometimes not getting loaded appropriately ...
Big changes to how StarModel fits happen now---fitting now defaults to using MultiNest via PyMultiNe...
Support has now been added to include parallax (in miliarcsec) to the observable properties of a Sta...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
First release of version 1.0. Significant changes from previous versions. MIST models are now avai...
Important functional changes included here are that now priors on distance and metallicity are inclu...
Isochrone fitting can be used for estimating stellar parameters which are not directly observable. T...
We continue our series of papers on open cluster distances by comparing multicolor photometry of sin...
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