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Astrophysics Source Code Library

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Searching for codes credited to 'Hardegree-Ullman, Kevin K.'

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[ascl:2202.010] EDIVU: Exoplanet Detection Identifier Vetter Unplugged
Zink, Jon K.; Hardegree-Ullman, Kevin K.; Christiansen, Jessie L.,; Dressing, Courtney D.; Crossfield, Ian J.M.; Petigura, Erik A.; Schlieder, Joshua E.; Ciardi, David R.

The EDI (Exoplanet Detection Identifier) Vetter Unplugged software identifies false positive transit signals using Transit Least Squares (TLS) information and has been simplified from the full EDI-Vetter algorithm (ascl:2202.009) for easy implementation with the TLS output.

[ascl:2202.009] EDIV: Exoplanet Detection Identifier Vetter
Zink, Jon K.; Hardegree-Ullman, Kevin K.; Christiansen, Jessie L.,; Dressing, Courtney D.; Crossfield, Ian J.M.; Petigura, Erik A.; Schlieder, Joshua E.; Ciardi, David R.

EDI (Exoplanet Detection Identifier) Vetter identifies false positive transit signal in the K2 data set. It combines the functionalities of Terra (ascl:2202.008) and RoboVetter (ascl:2012.006) and is optimized to test single transiting planet signals. An easily implemented suite of vetting metrics built to run alongside TLS of EDI Vetter, EDI-Vetter Unplugged (ascl:2202.010), is also available.

[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.