ASCL Code Record
[ascl:2411.028]
SMINT: Structure Model INTerpolator
Piaulet, Caroline; Benneke, Björn; Rubenzahl, Ryan A.; Howard, Andrew W.; Lee, Eve J.; Thorngren, Daniel; Angus, Ruth; Peterson, Merrin; Schlieder, Joshua E.; Werner, Michael; Kreidberg, Laura; Jaouni, Tareq; Crossfield, Ian J. M.; Ciardi, David R.; Petigura, Erik A.; Livingston, John; Dressing, Courtney D.; Fulton, Benjamin J.; Beichman, Charles; Christiansen, Jessie L.; Gorjian, Varoujan; Hardegree-Ullman, Kevin K.; Krick, Jessica; Sinukoff, Evan
SMINT (Structure Model INTerpolator) obtains posterior distributions on the H/He or H2O mass fraction of a planet; its interface is user-friendly. The parameters of the planet of interest are input with specifications on the priors that should be used. SMINT returns publication-ready plots presenting the joint parameters constraints obtained from interpolating the interior models grid of interest as well as confidence intervals for each parameter.
- Code site:
- https://github.com/cpiaulet/smint
- Described in:
- https://ui.adsabs.harvard.edu/abs/2021AJ....161...70P
- Bibcode:
- 2024ascl.soft11028P
Preferred citation method:
Please see citation information here: https://github.com/cpiaulet/smint#smint
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