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To tie photometry or direct images to radial velocity or proper motion measurements, we need to connect the brightness of a planet to mass given the age of the system.
We currently support the Sonora Bobcat cooling tracks, but we should have a library of a few other models like BT-Settl.
The first steps are:
register the tracks as a DataDep
interpolate over them on a fine grid using e.g. simpleinterpolations.jl
Write a function that goes from (age, photometry) -> mass or (age,mass) -> photometry (whichever is easier, or both) using Interpolations.jl so that autodiff continues to work.
Document them.
The text was updated successfully, but these errors were encountered:
To tie photometry or direct images to radial velocity or proper motion measurements, we need to connect the brightness of a planet to mass given the age of the system.
We currently support the Sonora Bobcat cooling tracks, but we should have a library of a few other models like BT-Settl.
The first steps are:
The text was updated successfully, but these errors were encountered: