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Supernova lightCURVE POPulation Synthesis

The Supernova lightCURVE POPulation Synthesis project combines the BPASSv2 stellar models and the SuperNova Explosion Code (SNEC, to understand the variety of supernova lightcurves that arise from a stellar population. For each paper in the series we release the input and outputs calculated by SNEC as well as summary details of the models. Thus others are able to use our results and calculate new supernova models if desired.

CURVEPOPS1 - including interacting binaries is key to understanding the diversity of type II supernova lightcurves.
[Paper on arxiv] 2018, PASA, 35, 49: Eldridge, Xiao, Stanway, Rodrigues, Guo
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CURVEPOPS2 - Validation against supernovae with an observed progenitor.
[Paper on arxiv] 2019, PASA 36 41: Eldridge, Guo, Rodrigues, Stanway, Xiao
[Download models]

License: The results from BPASS and CURVEPOPS available on this site licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.

Creative Commons License

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