The James Webb Space Telescope Feed

Spatially Resolved Properties of High Redshift Galaxies in the SMACS0723 JWST ERO Field

MINDS. The detection of $^{13}$CO$_{2}$ with JWST-MIRI indicates abundant CO$_{2}$ in a protoplanetary disk

JWST catches the assembly of a $z\sim5$ ultra-low-mass galaxy

The first large catalogue of spectroscopic redshifts in Webb's First Deep Field, SMACS J0723.3$-$7327

PEARLS | Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

PEARLS | a new lens model for ACT-CL J0102-4915, “El Gordo”, and the first red supergiant star at cosmological distances discovered by JWST

PEARLS | More blue- and slightly green enhanced

PEARLS | Moderately blue-enhanced (likely your best bet)

PEARLS | Version of the same composite with additional explanatory markup. (Image credits as for the main image; composite with pull-outs by R. Jansen).

PEARLS | Nineteen objects and groupings of objects in the full image are highlighted to showcase the detail and variation in color and shape in both relatively nearby and extremely distant objects discernable in the first GTO target area within the JWST NEP Time-Domain Field. (Image credits as for the main image; composite with pull-outs by R. Jansen).

PEARLS | A swath of sky measuring 2% of the area covered by a Full Moon was deeply imaged with JWST/NIRCam in 8 filters and with Hubble in 3 filters that together span the 0.25—5 µm wavelength range. Most of this range is invisible to the human eye. For this color composite, the wavelength range was compressed and the colors were remapped to ones that span the visible rainbow. Thousands of galaxies over an enormous range in distance and time are seen in exquisite detail, many for the first time. Light from the most distant galaxies has traveled almost 13.5 billion years to reach us. The larger galaxies in this image are seen as they were when our own Sun first started shining 4.6 billion years ago, but were at that time already almost 9 billion years old. The Universe was a more violent and active place then, with galaxies still assembling. This is shown by the many colliding galaxies, tidal tails and bridges, by extended streams of stars from shredded smaller galaxies, and by bright galaxy cores that show evidence of supermassive black holes feeding and growing.

The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA

The gas and stellar content of a metal-poor galaxy at $z=8.496$ revealed by JWST and ALMA

JWST and ALMA Multiple-Line Study in and around a Galaxy at $z=8.496$: Optical to FIR Line Ratios and the Onset of an Outflow Promoting Ionizing Photon Escape

UV Luminosity Density Results at z>8 from the First JWST/NIRCam Fields: Limitations of Early Data Sets and the Need for Spectroscopy

PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA

Cosmological Model Tests with JWST

Cross Correlation of Pencil-Beam Galaxy Surveys and Line-Intensity Maps: An Application of the James Webb Space Telescope

Reconstructing the genesis of a globular cluster system at a look-back time of 9.1 Gyr with the JWST

GCM Constraints on the Detectability of the CO$_2$-CH$_4$ Biosignature Pair on TRAPPIST-1e with JWST

What if young z>9 JWST galaxies hosted massive black holes?

UNCOVER | UNCOVER_nircam_mosaic

UNCOVERing the extended strong lensing structures of Abell 2744 with the deepest JWST imaging

UNCOVER | UNCOVER_niriss_parallel_mosaic

The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization

JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources

Photometry and astrometry with JWST -- II. NIRCam geometric distortion correction

The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS

Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST

Interpreting ALMA non-detections of JWST super-early galaxies

PHANGS-JWST First Results: The 21 $μ$m Compact Source Population

PHANGS-JWST First Results: A statistical view on bubble evolution in NGC628

Cosmic Spring | WHL0137 A galaxy cluster magnifying distant galaxies and the individual star system Earendel, observed by JWST in 2022 July and December.

Cosmic Spring | The most distant star known seen as it was 13 billion years ago

PHANGS-JWST First Results: The Influence of Stellar Clusters on PAHs in Nearby Galaxies

PHANGS-JWST First Results: Spurring on Star Formation: JWST Reveals Localised Star Formation in a Spiral Arm Spur of NGC 628

The binary and the disk: the beauty is found within NGC3132 with JWST

JWST NIRCam Defocused Imaging: Photometric Stability Performance and How it Can Sense Mirror Tilts

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST

PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628

PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628

Water and an escaping helium tail detected in the hazy and methane-depleted atmosphere of HAT-P-18b from JWST NIRISS/SOSS

An Hα Impression of Lyα Galaxies at $z\simeq6$ with Deep JWST/NIRCam Imaging

PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3.3 $μ$m PAH emission

FOREVER22: the first bright galaxies with population III stars at redshifts $z \simeq 10-20$ and comparisons with JWST data

Witnessing a Galaxy Cluster Merger with JWST and a Chandra X-ray Temperature Map

Early Release Science of the exoplanet WASP-39b with JWST NIRISS

Early Release Science of the exoplanet WASP-39b with JWST NIRCam

Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM

UNCOVER | UNCOVER_nircam_mosaic_insets

Spectral Templates Optimal for Selecting Galaxies at z > 8 with JWST

CEERS | Spectral Templates Optimal for Selecting Galaxies at z > 8 with JWST

How dark the sky: the JWST backgrounds