Next up, we‘ve got Kazumasa Ohno on the hazy sub-Neptune GJ1214 b.

Previous observations show pretty flat lines, likely due to hazes and clouds. The JWST phase curve with MIRI shows a large amplitude indicative of high metallicity, but the spectrum is still consistent with a flat line. It is though predicted to have CO2 and CH4 features so they observed with #G395H. And??? 🧐 #ExSSV