Identifying the most faithful reduction approach for exoplanet transmission spectroscopy data

Determine which data-reduction methodology—including specific choices for background subtraction, 1/f-noise mitigation, spectral extraction, and light-curve modeling—most accurately recovers the true planetary transmission spectrum from exoplanet transmission spectroscopy time-series, given that the planetary signal cannot be directly observed.

Background

Transmission spectroscopy reductions involve many methodological choices—such as how to subtract background and zodiacal light, mitigate 1/f noise, extract spectra from overlapping orders, and model light-curve systematics—that can materially affect the inferred atmospheric properties.

Because the ground truth planetary signal is not directly observable, assessing which combination of reduction steps and parameter choices yields the most faithful transmission spectrum is non-trivial; this study explores the issue by testing targeted tweaks to reduction steps rather than relying solely on comparisons between complete, independent pipelines.

References

Several methodological choices in this process can significantly affect the inferred atmospheric properties. As the true planetary signal cannot be directly observed, it is often unclear which reduction approach most faithfully recovers it.

— Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared  (2604.01219 - Heinke et al., 1 Apr 2026) in Section 3, NIRISS data reduction (first paragraph)