CCSNe Database for SIMPLE

This database contains 18 CCSNe models for use with SIMPLE, a Python tool that compares the isotopic composition of ejecta from nucleosynthetic models with meteorite data. The database is an HDF5 file and is meant to be used together with the Python tool SIMPLE (Stellar Interpretation of Meteoritic Data and Plotting for Everyone). The package is available on GitHub here, with documentation available here. The models come from 6 different datasets and have initial masses of 15, 20, and 25 solar masses, and all have solar metallicity. La22- Lawson et al. (2022) LC18 - Limongi & Chieffi (2018) Pi16 - Pignatari et al. (2016) Ra02 - Rauscher et al. (2002) Ri18 - Ritter et al. (2018) Si18 - Sieverding et al. (2018) Also included in the database are the solar abundances used for each model and the isotope masses. Citation and Use This database aggregates CCSN model outputs from multiple published studies for use with the SIMPLE framework. It serves as a curated access point and is not intended to replace the primary literature associated with the individual models. If data derived from one or more of these models are used in publications or scientific analyses, the original reference paper(s) corresponding to the relevant models must be cited, alongside this Zenodo record and the accompanying publication describing the SIMPLE framework and this database. Specific enquiries regarding the models, including their properties, underlying assumptions, applicability for data mining, or comparisons with observational data outside their application with SIMPLE, should be directed to the corresponding author(s) listed in the respective reference papers. Known Issues The Mo and Zr yields for the LC18 models are known to be incorrect. Therefore, these models should not be used to study those elements. The database will be updated once new model versions are available.