New Features csp subpackage: Create Complex Stellar Populations from the BPASS Simple Stellar Populations! Use them to predict transient rates originating from your population. data_compiler module: Includes the ModelDataCompiler which allows you to compile a subset of the BPASS stellar library into an pandas.DataFrame that is easy to search and operate on! This allows you to do some advances model searches to match your stellar population or your transient progenitor. New tutorials in hoki_tutorials repository Complex Stellar Populations: Shows you how to make Complex Stellar Populations Model Data Compiler: Shows you how to compile the data you're interested in from individual text files into a table Model Search: Shows you some of th...
This is a curated starter-kit that contains a subset of the full data in BPASSv2.2.1. For the full d...
Received; accepted Context. Constraints on stellar models can be obtained from observations of stell...
Context. Modeling a single star with theoretical stellar evolutionary tracks is a nontrivial problem...
Description This new version of hoki contains the data analysis pipelines used to fit BPASS SEDs to ...
Summary At the core of v1.5 is the age_utils module and the AgeWizard pipeline. The utilities provi...
This data set is made of 26 binary files (.pckl) that contain pandas DataFrames compiling all the BP...
The ever-expanding depth and quality of photometric and spectroscopic observations of stellar popula...
Astromodels is a very flexible framework to define models for likelihood or Bayesian analysis of ast...
We analyse the high-quality Hertzsprung–Russell diagram (HRD) derived from Gaia data release 2 for t...
The BPASS models of Eldridge & Stanway (2012, MNRAS, 419, 479); Eldridge, Langer & Tout (2011, MNRAS...
International audienceContext. The cornerstone mission of the European Space Agency, Gaia, together ...
International audienceStellar population synthesis (SPS) models are invaluable to study star cluster...
Patch for the submission of our revised manuscript of "A_systematic_aging_method_I: NGC 300 ...." Fe...
Context. Modeling a single star with theoretical stellar evolutionary tracks is a nontrivial problem...
Stellar models provide a vital basis for many aspects of astronomy and astrophysics. Recent advances...
This is a curated starter-kit that contains a subset of the full data in BPASSv2.2.1. For the full d...
Received; accepted Context. Constraints on stellar models can be obtained from observations of stell...
Context. Modeling a single star with theoretical stellar evolutionary tracks is a nontrivial problem...
Description This new version of hoki contains the data analysis pipelines used to fit BPASS SEDs to ...
Summary At the core of v1.5 is the age_utils module and the AgeWizard pipeline. The utilities provi...
This data set is made of 26 binary files (.pckl) that contain pandas DataFrames compiling all the BP...
The ever-expanding depth and quality of photometric and spectroscopic observations of stellar popula...
Astromodels is a very flexible framework to define models for likelihood or Bayesian analysis of ast...
We analyse the high-quality Hertzsprung–Russell diagram (HRD) derived from Gaia data release 2 for t...
The BPASS models of Eldridge & Stanway (2012, MNRAS, 419, 479); Eldridge, Langer & Tout (2011, MNRAS...
International audienceContext. The cornerstone mission of the European Space Agency, Gaia, together ...
International audienceStellar population synthesis (SPS) models are invaluable to study star cluster...
Patch for the submission of our revised manuscript of "A_systematic_aging_method_I: NGC 300 ...." Fe...
Context. Modeling a single star with theoretical stellar evolutionary tracks is a nontrivial problem...
Stellar models provide a vital basis for many aspects of astronomy and astrophysics. Recent advances...
This is a curated starter-kit that contains a subset of the full data in BPASSv2.2.1. For the full d...
Received; accepted Context. Constraints on stellar models can be obtained from observations of stell...
Context. Modeling a single star with theoretical stellar evolutionary tracks is a nontrivial problem...