The James Webb Space Telescope Feed
The most extensive source of information about James Webb Space Telescope. JWST Feed contains every single piece of data from the telescope, and is updating live every few minutes. Our goal is to make the full JWST data accessible for the public.
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Early results from GLASS-JWST. XVIII: A spectroscopically confirmed protocluster 650 million years after the Big Bang
EIGER II. first spectroscopic characterisation of the young stars and ionised gas associated with strong H$β$ and [OIII] line-emission in galaxies at z=5-7 with JWST
MACS0647–JD observed in the NIRCam SW color image (B=F115W, G=F150W, R=F200W) and in each NIRCam filter
Delensed images of JD1, 2, 3 based on our Zitrin-analytic lens model (Meena et al. in preparation) compared to a pair of merging galaxies in the Renaissance simulations (Barrow et al. 2017) shown at left on the same physical scale | MACS0647
Delensed images of JD1, 2, 3 based on our Zitrin-analytic lens model (Meena et al. in preparation) compared to a pair of merging galaxies in the Renaissance simulations (Barrow et al. 2017) shown at left on the same physical scale | MACS0647
GALFIT modeling (center) of JD1ABC in the F150W and F200W images (left) with residuals shown at right | MACS0647
Astroparticle Constraints from the Cosmic Star Formation Rate Density at High Redshift: Current Status and Forecasts for JWST
Evolution of the UV LF from z~15 to z~8 Using New JWST NIRCam Medium-Band Observations over the HUDF/XDF
The Near Infrared Imager and Slitless Spectrograph for JWST -- V. Kernel Phase Imaging and Data Analysis
The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope -- IV. Aperture Masking Interferometry
Kindling the First Stars: I. Dependence of Detectability of the First Stars with JWST on the Pop III Stellar Masses
First results from the JWST Early Release Science Program Q3D: Turbulent times in the life of a $z \sim 3$ extremely red quasar revealed by NIRSpec IFU
Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
Pulsations of primordial supermassive stars induced by a general relativistic instability; visible to JWST at z$>$12
JWST's PEARLS: a new lens model for ACT-CL J0102$-$4915, "EL Gordo'', and the first red supergiant star at cosmological distances discovered by JWST
PAH emission from star-forming galaxies in JWST mid-infrared imaging of the lensing cluster SMACS J0723.3$-$7327
WR DustERS | Normalized, continuum subtracted, and smoothed 6 - 9 µm spectrum of the C1 feature in Shell 2 around WR 140 from MIRI/MRS observations used in Lau et al. (2022).
WR DustERS | Reduced (non median-subtracted) JWST/MIRI Imager data of WR 140 used in Lau et al. (2022).
WR DustERS | Comparison of JWST/MIRI Imaging Observations of WR140 and a 20 shell geometric model (Lau et al. 2022, Han et al. 2022).