New in this release: Added BinaryStarModel object, which enables fitting photometry to a model of two stars at the same distance, Fe/H, and age. Changed StarModel.triangle() such that if truths is provided, then extents adjust so truths can be seen even if outside requested extent range
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Eclipsing Binaries (EBs) are known to be the source of most accurate stellar parameters, which are i...
This is a minor bugfix release. Makes sure HDF files do not remain open after StarModel.load_hdf. A...
Typo fixed in StarModel._make_samples() Bug fixed in StarModel.triangle() when distance is not bein...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
First release of version 1.0. Significant changes from previous versions. MIST models are now avai...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
Support has now been added to include parallax (in miliarcsec) to the observable properties of a Sta...
Big changes to how StarModel fits happen now---fitting now defaults to using MultiNest via PyMultiNe...
Important functional changes included here are that now priors on distance and metallicity are inclu...
Existing but largely unused binary star model capabilities are examined. An easily implemented schem...
Isochrone fitting can be used for estimating stellar parameters which are not directly observable. T...
The mass of a star determines how it evolves throughout its lifetime from beginning to end. Understa...
Eclipsing Binary Stars focuses on the mathematical formulation of astrophysical models for the light...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Eclipsing Binaries (EBs) are known to be the source of most accurate stellar parameters, which are i...
This is a minor bugfix release. Makes sure HDF files do not remain open after StarModel.load_hdf. A...
Typo fixed in StarModel._make_samples() Bug fixed in StarModel.triangle() when distance is not bein...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
First release of version 1.0. Significant changes from previous versions. MIST models are now avai...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
Support has now been added to include parallax (in miliarcsec) to the observable properties of a Sta...
Big changes to how StarModel fits happen now---fitting now defaults to using MultiNest via PyMultiNe...
Important functional changes included here are that now priors on distance and metallicity are inclu...
Existing but largely unused binary star model capabilities are examined. An easily implemented schem...
Isochrone fitting can be used for estimating stellar parameters which are not directly observable. T...
The mass of a star determines how it evolves throughout its lifetime from beginning to end. Understa...
Eclipsing Binary Stars focuses on the mathematical formulation of astrophysical models for the light...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Eclipsing Binaries (EBs) are known to be the source of most accurate stellar parameters, which are i...
This is a minor bugfix release. Makes sure HDF files do not remain open after StarModel.load_hdf. A...
DOI
Add to ORKG