This JWebbinar — Exoplanet Time-Series Observations with MIRI: From Pixels to Transit/Eclipse Light Curves to Results — will begin with a brief overview of data processing using the JWST pipeline, with a focus on specific tuning and parameter settings that are optimized for handling exoplanet time-series observations (TSOs). We will then learn how to extract light curves from the data, fit those light curves with transit/eclipse models, and handle systematic noise. While the focus will be on MIRI Imaging and LRS Slitless spectroscopy TSOs, the data reduction and analysis methods presented in this webinar are broadly applicable to all TSOs obtained with JWST.

Registration closes May 1.