Since we'll have PHOENIX model spectra of HAT-P-11 and TRAPPIST-1, it would be fun to model their count rates through a second telescope 🔠. I'm thinking perhaps we can use Kepler, since (1) Kepler observed both HAT-P-11 (Kepler) and TRAPPIST-1 (K2); (2) it's a space telescope and therefore shouldn't depend on our atmosphere model, making it a good sanity check.
Since we'll have PHOENIX model spectra of HAT-P-11 and TRAPPIST-1, it would be fun to model their count rates through a second telescope 🔠. I'm thinking perhaps we can use Kepler, since (1) Kepler observed both HAT-P-11 (Kepler) and TRAPPIST-1 (K2); (2) it's a space telescope and therefore shouldn't depend on our atmosphere model, making it a good sanity check.
Here's some of the info you'll need to do Kepler:
astropy.units.data.download_file
to grab this file rather than including it in the PR