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[ascl:2206.018] MADYS: Isochronal parameter determination for young stellar and substellar objects

MADYS (Manifold Age Determination for Young Stars) determines the age and mass of young stellar and substellar objects. The code automatically retrieves and cross-matches photometry from several catalogs, estimates interstellar extinction, and derives age and mass estimates for individual objects through isochronal fitting. MADYS harmonizes the heterogeneity of publicly-available isochrone grids and the user can choose amongst several models, some of which have customizable astrophysical parameters. Particular attention has been dedicated to the categorization of these models, labeled through a four-level taxonomical classification.

Code site:
https://github.com/vsquicciarini/madys
Used in:
https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.1381S
Described in:
https://ui.adsabs.harvard.edu/abs/2022arXiv220602446S
Bibcode:
2022ascl.soft06018S

Views: 1458

ascl:2206.018
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