Abstract James Webb Space Telescope (JWST) MIRI 15 μ m time-series eclipse photometry presents a powerful way to probe for the presence of atmospheres on low-temperature rocky exoplanets orbiting nearby stars. Here, we introduce a novel technique, frame-normalized principal component analysis (FN-PCA), to analyze and detrend these MIRI time-series observations. Using the FN-PCA technique, we perform a uniform reanalysis of the published MIRI 15 μ m observations of LHS 1478 b, TOI-1468 b, LHS 1140c, TRAPPIST-1 b, and TRAPPIST-1 c using our new data reduction pipeline ( Erebus ) and compare them to different potential atmospheric and surface compositions. We also investigate additional public data sets with the sole purpose of understanding the instrument systematics affecting MIRI. We identify and categorize important detector-level systematics in the observations that are generally present across all 17 analyzed eclipse observations, which we illustrate as eigenimage/eigenvalue pairs in the FN-PCA. One of these eigenimage/eigenvalue pairs corresponds to the prominent ramp effect at the beginning of the time-series observations, which has widely been reported for JWST and Spitzer photometry. For JWST/MIRI, we show that the detector settling timescales exponentially with the apparent magnitude of the target star T set hr = 0.063 exp 0.427 · m K − 0.657 . This uniform reanalysis and investigation of JWST/MIRI systematics is done in preparation for the 500 hr Rocky Worlds Director’s Discretionary Time survey to demonstrate a data-driven systematic model usable across all MIRI 15 μ m data sets.
Connors et al. (Wed,) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: