First release of version 1.0. Significant changes from previous versions. MIST models are now available (much broader coverage in mass, age, and metallicity), in addition to Dartmouth. Book-keeping is much more organized with the new ModelGrid object, which takes the model grids exactly as published and does all the parsing as part of the package. This should make it easier to extend to using other model grids. BinaryStarModel and TripleStarModel no longer exist; now you can just provide an N=2 keyword argument to StarModel. Support for non-trivial collection of photometric bands for multiple stars: e.g., pair of stars unresolved in 2MASS but resolved in high-resolution imaging. Isochrone object can now predict density, nu_max, and del...
Fixed a bug with building the samples dataframes for BinaryStarModel and TripleStarModel. Add some f...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
Current generation stellar isochrone models exhibit non-negligible discrepancies due to variations i...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
This release both makes MIST version 1.1 default (notably including the new Gaia G, BP, and RP bands...
<p>Dartmouth stellar model grids, used by the 'isochrones' python package (github.com/timothydmorton...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Fixed a few bugs from initial release. Isochrone object can now be called with distance and AV argu...
Abstract. We present the current status of an effort to create an updated grid of low-mass stellar e...
<p>These are the data files that get downloaded by the "isochrones" Python package. "mist.tgz" and ...
New in this release: Added BinaryStarModel object, which enables fitting photometry to a model of ...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
Fixed a bug with building the samples dataframes for BinaryStarModel and TripleStarModel. Add some f...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
Current generation stellar isochrone models exhibit non-negligible discrepancies due to variations i...
Isochrones 2.0 contains the following major updates and improvements: All-new documentation: https:...
Note, this is the final incremental release of the isochrones v1.x series implementing some very min...
This release both makes MIST version 1.1 default (notably including the new Gaia G, BP, and RP bands...
<p>Dartmouth stellar model grids, used by the 'isochrones' python package (github.com/timothydmorton...
The biggest update in this release is the addition of the populations submodule (thanks to the reque...
Fixed a few bugs from initial release. Isochrone object can now be called with distance and AV argu...
Abstract. We present the current status of an effort to create an updated grid of low-mass stellar e...
<p>These are the data files that get downloaded by the "isochrones" Python package. "mist.tgz" and ...
New in this release: Added BinaryStarModel object, which enables fitting photometry to a model of ...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model an...
Fixed a bug with building the samples dataframes for BinaryStarModel and TripleStarModel. Add some f...
Bug fix: When creating the StarModel.samples attribute, there used to be a hard-coded cut on lnpr...
Current generation stellar isochrone models exhibit non-negligible discrepancies due to variations i...