Webb and atmospheres

Observing is not detecting. Detecting is not explaining.

James Webb status is split into approved program, observation, public data, archived spectrum, paper and contested result.

Automated sourceNExoList + spectra

The catalog reads approved JWST observation and archived-spectrum counts from NASA Exoplanet Archive.

Files and criteria →
Editorial snapshot

The targets shaping the current search

The catalog’s automated counts come from PSCompPars/NExoList. This panel adds scientific context to the most important cases.

Published result

LHS 1140 b

NIRISS + NIRSpec

A hydrogen-rich H₂ atmosphere was ruled out; a heavy atmosphere remains possible. The 2026 helium evidence came from ground-based telescopes.

Published result

TRAPPIST-1 e

NIRSpec/PRISM

A primary H₂-rich atmosphere was ruled out; a secondary atmosphere remains unconfirmed. The star dominates the error budget.

Contested result

K2-18 b

NIRISS + NIRSpec + MIRI

CH₄ and CO₂ are robust; DMS/DMDS depend on the reduction and model. No biosignature has been confirmed.

Program in progress

LP 890-9 c

NIRSpec/PRISM · 18 transits

The Cosmic Shoreline campaign has been approved to search for atmospheric retention; results have not yet been published.

Photometry, not atmosphere

TOI-700 d / e

JWST

The system was observed to refine ephemerides and search for exomoons; this is not atmospheric characterization.