JWST COMPASS: Insights into the Systematic Noise Properties of NIRSpec/G395H from a Uniform Reanalysis of Seven Transmission Spectra
Authors:
- Tyler A. GordonTGTyler A. Gordon
- Natalie M. BatalhaNBNatalie M. Batalha
- Natasha E. BatalhaNBNatasha E. Batalha
- Artyom AguichineAAArtyom Aguichine
- Anna GagnebinAGAnna Gagnebin
- James KirkJKJames Kirk
- Mercedes López-MoralesMLMercedes López-Morales
- Annabella MeechAMAnnabella Meech
- Nicholas ScarsdaleNSNicholas Scarsdale
- Johanna TeskeJTJohanna Teske
- Nicole L. WallackNWNicole L. Wallack
- Nicholas WoganNWNicholas Wogan
Open Access
- 20 February 2026
- journal article
- Published by American Astronomical Society in The Astronomical Journal
- Vol. 171 (3) , 178
Abstract
JWST has already observed near-infrared transmission spectra of over a dozen super-Earths and sub-Neptunes. While some observations have allowed astronomers to characterize sub-Neptunes in unprecedented detail, small feature amplitudes and poorly understood systematics have led to ambiguous results for others. Using the first seven targets from the COMPASS program, which will survey 12 small planets using NIRSpec/G395H, we investigate timeseries systematics. We implement a model that uses the principle components of the normalized pixel fluxes to account for variations in the shape and position of the spectral trace. We find that observations with a smaller number of groups-per-integration benefit most profoundly from the use of this model, and that systematics are particularly strong between 2.8 and 3.5 μ m. Despite these systematics, pandexo is a relatively accurate predictor of the precision of the spectra, with real error bars on average 5% larger in NRS1 and 12% larger in NRS2 than predicted. We compute new limits on metallicity and opaque pressure level for each target and compare these to previous results from the COMPASS program. Next, we coadd spectra from multiple targets to reduce the effective noise in the combined spectra in hopes of detecting transmission features in common between the targets, but this exercise does not yield compelling evidence of any signals. We find that a handful of additional transits are sufficient to break the degeneracy between metallicity and aerosols for the majority of our targets, pointing towards the possibility of unraveling the mysteries of these worlds with future allocations of JWST time.Keywords
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Funding Information
- Heising-Simons Foundation (2021-3197)
- NASA ∣ NASA Astrobiology Institute (19-ICAR19 2-0041)
- National Aeronautics and Space Administration (80NSSC19K0290)
This publication has 95 references indexed in Scilit:
- Hydrogen escaping from a pair of exoplanets smaller than NeptuneNature, 2025
- A radius valley between migrated steam worlds and evaporated rocky coresNature Astronomy, 2024
- A JWST transmission spectrum of the nearby Earth-sized exoplanet LHS 475 bNature Astronomy, 2023
- A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18bNature, 2023
- A reflective, metal-rich atmosphere for GJ 1214b from its JWST phase curveNature, 2023
- Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395HNature, 2023
- SciPy 1.0: fundamental algorithms for scientific computing in PythonNature Methods, 2020
- Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterizationAstronomy & Astrophysics, 2019
- petitRADTRANSAstronomy & Astrophysics, 2019
- Potential biosignatures in super-Earth atmospheresAstronomy & Astrophysics, 2011