JWST

Using JWST's sensitivity and broad wavelength coverage, researchers reconstructed Alaknanda's intrinsic properties.

JWST spectra show signatures of water vapor, carbon monoxide, carbon dioxide, and ammonia in WASP-107b's atmosphere.

Using JWST's infrared capabilities, researchers measured how WASP-107b and its extended atmosphere absorb the light of its host star during transit.

Images and spectra obtained with the NIRCam instrument on JWST revealed BiRD as an unusual bright point not present in previous X-ray and radio catalogs.

The new 3D map utilized many wavelengths from JWST's Near-Infrared Imager and Slitless Spectrograph (NIRISS), with each wavelength corresponding to a distinct temperature and altitude.

JWST's observations confirmed regions with different temperatures and probably different compositions on WASP-18b's dayside due to tidal locking.

Danhaive wrote new code to analyze the grism data and matched it with images from other JWST surveys to measure gas movement within each galaxy.

The results demonstrate the capability of JWST to probe galaxy dynamics at a previously impossible scale.

The researchers used JWST's NIRCam instrument in a 'grism mode' to capture faint light from ionised hydrogen gas in distant galaxies.

Phosphine was detected in the atmosphere of the brown dwarf Wolf 1130C using observations from the James Webb Space Telescope (JWST).

The team easily spotted phosphine in JWST's infrared spectral data of Wolf 1130C.

JWST could operate for 20 years or more, but faces near-term budget challenges.

NASA and STScI predict JWST could operate for more than two decades.

JWST's oversubscription rate in the latest proposal cycle was over nine.

JWST's prime mission is officially five years long.

STScI is considering a significant 20% cut to JWST's operating budget.

NASA requested $127 million for JWST operations and $60 million for science grants in its 2025 budget proposal.

JWST was successfully launched at the end of 2021.