Open taylorbell57 opened 9 months ago
Thanks for bringing this up! This was one of our top motivations for developing jaxoplanet in the first place and it's absolutely supported. Here we benefit from jax.vmap
, which means that any models written in JAX can be expressively vectorized over any of their input parameters.
@soichiro-hattori has been leading the work on applying jaxoplanet to real data with a specific eye towards transmission spectroscopy, and we're hoping to have a paper and tutorial "Soon™". In the meantime, we'd be very happy to help get you or anyone else up and running!
Wonderful, I'm very happy to hear it!! :rocket: You're welcome to close this issue if you want or keep it open to avoid others asking the same question until a tutorial is provided
Another issue I brough up on the starry repo is the ability to fit multi-wavelength lightcurves. With the advent of JWST, I and many others are wanting to simultaneously fit multi-wavelength data. This ends up being such a high-dimensional problem that my understanding is that HMC-based samplers like NUTS are likely the only option. While starry supported wavelength-dependent emission, it did not support wavelength-dependent radii (https://github.com/rodluger/starry/issues/286) or wavelength-dependent limb-darkening (https://github.com/rodluger/starry/issues/310) which are critical for transmission spectroscopy. While with starry one could make N systems for N wavelengths, this ends up being seriously inefficient and slow as the overhead of initializing objects and solving for geometric values (e.g., solving Kepler's equation) is repeated N times.
Again, I am really not well-versed in jaxoplanet yet and its possible that this is already supported, but I wanted to raise this issue early on to try to make sure it was considered before adding such a feature became too cumbersome.