JWST Eyes on the Stars

JWST Legacy Archival Program Enabling Robust Stellar Context for Exoplanet Spectroscopy

Eyes on the Stars is a JWST archival research program focused on extracting and standardizing time-series spectroscopy products that help disentangle stellar and planetary signals in transmission spectra. The program emphasizes reproducible reductions, consistent assumptions across targets, and intentional consideration of stellar contamination as an astrophysical systematic to deliver products designed for downstream atmospheric inference.

Grant: JWST AR 5370   •   Last updated: —

Why “Eyes on the Stars”?

Stellar photospheres are not uniform. Spots, faculae, and other forms of heterogeneity can imprint wavelength-dependent signals that bias inferred planetary radii, spectral slopes, and molecular abundances. This is especially important for active K and M dwarfs and for the high-precision spectra enabled by JWST.

Eyes on the Stars provides uniform data products and stellar-contamination constraints that support robust interpretation of JWST transmission spectra and facilitate comparisons across targets, instruments, and observing modes.

Stellar contamination as an astrophysical systematic

Quantify the impact of unocculted and occulted photospheric heterogeneity on transmission spectra and provide products designed for atmospheric retrieval workflows.

Uniform, comparable reductions

Apply consistent reduction and modeling assumptions across a broad set of JWST time-series observations, enabling population-level and cross-instrument analyses.

Community-oriented JWST outputs

Deliver curated products and documentation that make it easier to incorporate stellar context into JWST-era atmospheric characterization.

Targets & Observations

Eyes on the Stars analyzes 37 JWST time-series visits spanning 17 planetary systems and 267.6 hours of observations with NIRISS/SOSS and NIRSpec/PRISM.

Together, these observations comprise the archival dataset analyzed by JWST AR 5370.

Target Spectral Type Instrument / Mode Visits Duration JWST Programs
WASP-189 A6V NIRISS/SOSS 1 13.2 hr 3279
HAT-P-14 F3V NIRISS/SOSS 1 7.1 hr 1541
WASP-17 F5V NIRISS/SOSS 1 12.7 hr 1353
HAT-P-1 F9V NIRISS/SOSS 1 8.4 hr 1201
Kepler-51 G2V NIRSpec/PRISM 1 15.0 hr 2454
WASP-96 G7V NIRISS/SOSS 1 7.5 hr 2734
WASP-39 G9V NIRISS/SOSS; NIRSpec/PRISM 2 21.2 hr 1366
WASP-52 K2V NIRISS/SOSS 1 6.1 hr 1201
HAT-P-18 K3V NIRISS/SOSS 1 8.2 hr 2734
HAT-P-12 K4V NIRISS/SOSS 1 8.3 hr 1281
HATS-72 K4V NIRISS/SOSS 1 8.3 hr 2594
WASP-107 K6V NIRISS/SOSS 1 8.3 hr 1201
K2-18 M2.5V NIRISS/SOSS 1 6.9 hr 2722
L 98-59 M3V NIRISS/SOSS 1 5.0 hr 1201
TOI-5205 M3.5V NIRSpec/PRISM 3 20.5 hr 3171
LP 791-18 M5.5V NIRSpec/PRISM 1 5.2 hr 1201
TRAPPIST-1 M8V NIRISS/SOSS; NIRSpec/PRISM 18 105.8 hr 1201 1331 1981 2420 2589

This target list reflects the observations included in JWST AR 5370 and may be updated as the program develops.

Contact

  • Email

    brackham@mit.edu
  • Resources