ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:2006.016] SPISEA: Stellar Population Interface for Stellar Evolution and Atmospheres

SPISEA (Stellar Population Interface for Stellar Evolution and Atmospheres) generates single-age, single-metallicity populations (i.e., star clusters). The software (formerly called PyPopStar) provides control over different parameters, including cluster characteristics (age, metallicity, mass, distance); total extinction, differential extinction, and extinction law; stellar evolution and atmosphere models; stellar multiplicity and Initial Mass Function; and photometric filters. SPISEA can be used to create a cluster isochrone in many filters using different stellar models, generate a star cluster at any age with an unusual IMF and unresolved multiplicity, and make a spectrum of a star cluster in integrated light.

Code site:
https://github.com/astropy/SPISEA https://spisea.readthedocs.io/en/latest/
Described in:
https://ui.adsabs.harvard.edu/abs/2020arXiv200606691H
Bibcode:
2020ascl.soft06016H

Views: 518

ascl:2006.016
Add this shield to your page
Copy the above HTML to add this shield to your code's website.