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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Strategy for Dynamic Wisp Removal in James Webb Space Telescope NIRCam Images Published: 5/2/2023 6:20:31 AM Updated: 5/2/2023 6:20:31 AM
Primordial power spectrum in light of JWST observations of high redshift galaxies Published: 5/1/2023 9:00:02 PM Updated: 5/1/2023 9:00:02 PM
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/TARGACQ Filters: F210M;MASKRND Start Time: 5/2/2023 6:35:52 PM Obs Time: 96.631(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/IMAGE Filters: F210M;MASKRND Start Time: 5/2/2023 6:40:32 PM Obs Time: 96.631(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/IMAGE Filters: F210M;MASKRND Start Time: 5/2/2023 6:35:53 PM Obs Time: 96.631(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/IMAGE Filters: F210M;MASKRND Start Time: 5/2/2023 6:35:53 PM Obs Time: 96.631(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/CORON Filters: F210M;MASKRND Start Time: 5/2/2023 6:40:31 PM Obs Time: 96.631(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/CORON Filters: F335M;MASKRND Start Time: 5/2/2023 7:24:56 PM Obs Time: 107.368(s) Proposal ID: 1482
Target Name: K5-2MASS-16235565+2823024 Title: Coronagraphic PSF Characterization & TA Verification Instrument: NIRCAM/TARGACQ Filters: F335M;MASKRND Start Time: 5/2/2023 7:20:06 PM Obs Time: 107.368(s) Proposal ID: 1482
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F150W Start Time: 5/2/2023 2:44:29 AM Obs Time: 483.155(s) Proposal ID: 1571
Target Name: 2MASS-12114924+5856270 Title: JWST Routine Wavefront Sensing and Control for Cycle 1 - Part 4 Instrument: NIRCAM/IMAGE Filters: F356W Start Time: 5/2/2023 4:10:50 PM Obs Time: 96.631(s) Proposal ID: 4431
Target Name: 2MASS-12114924+5856270 Title: JWST Routine Wavefront Sensing and Control for Cycle 1 - Part 4 Instrument: NIRCAM/IMAGE Filters: F356W Start Time: 5/2/2023 4:03:30 PM Obs Time: 96.631(s) Proposal ID: 4431
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F150W Start Time: 5/2/2023 10:00:10 AM Obs Time: 483.155(s) Proposal ID: 1571
Saturn's rings are disappearing. The James Webb Space Telescope may reveal how much time they have left.
High Tide or Riptide on the Cosmic Shoreline? A Water-Rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ~486b from JWST Observations Published: 5/1/2023 6:10:34 PM Updated: 5/1/2023 6:10:34 PM
Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History From 25 Galaxies at z_\mathrm{spec}=8.61-13.20 Confirmed with JWST/NIRSpec Published: 4/13/2023 7:45:41 PM Updated: 4/30/2023 4:51:55 PM
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F150W Start Time: 5/1/2023 7:32:20 PM Obs Time: 483.155(s) Proposal ID: 1571
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F150W Start Time: 5/1/2023 7:32:20 PM Obs Time: 483.155(s) Proposal ID: 1571
The galaxy UV luminosity function at z~11 from a suite of public JWST ERS, ERO and Cycle-1 programs Published: 4/27/2023 10:12:17 PM Updated: 4/27/2023 10:12:17 PM
A physically derived eddy parameterization for giant planet atmospheres with application on hot-Jupiter atmospheres
Star formation rate and stellar mass calibrations based on infrared photometry and their dependence on stellar population age and extinction
Target Name: UNKNOWN Title: NIRCam Subarray Dark Current and Read-Noise Monitor Instrument: NIRCAM/IMAGE Filters: N/A Start Time: 4/30/2023 12:43:25 AM Obs Time: 1079.935(s) Proposal ID: 1483
Target Name: 2MASS-12114924+5856270 Title: JWST Routine Wavefront Sensing and Control for Cycle 1 - Part 4 Instrument: NIRCAM/IMAGE Filters: F356W Start Time: 4/29/2023 11:02:01 PM Obs Time: 96.631(s) Proposal ID: 4431
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F200W Start Time: 4/28/2023 6:52:35 AM Obs Time: 2866.718(s) Proposal ID: 1571
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F200W Start Time: 4/28/2023 6:03:03 AM Obs Time: 2866.718(s) Proposal ID: 1571
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F200W Start Time: 4/28/2023 4:24:10 AM Obs Time: 2866.718(s) Proposal ID: 1571
Target Name: UNKNOWN Title: PASSAGE--Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution Instrument: NIRISS/IMAGE Filters: CLEAR;F200W Start Time: 4/28/2023 5:13:42 AM Obs Time: 2866.718(s) Proposal ID: 1571
PRIMER | The power of fully-sampled NIRCam imaging. Left: simulated NIRCam image of a clumpy z = 2 galaxy in the F277W filter with the native NIRCam-LW pixel scale (0.063 arcsec). Right: NIRCam image of the same galaxy in the same filter but this time with sub-pixel sampling, and image reconstruction with 50% smaller pixels. Not only are the structural details much clearer, but several compact clumps are simply not detected in the left-hand undersampled image: properly sampled imaging enhances the detection of faint compact objects (such as extreme redshift galaxies), as well as improving the precision of morphological studies
PRIMER | The transformational power of JWST imaging longward of ~ 2.5 micron Left: a 44 x 34 arcsec region of the deepest available Spitzer IRAC 3.6 micron imaging. Right: a prediction of how the same region will appear with the PRIMER NIRCam F356W imaging using the empirically based EGG simulations (Schreiber et al. 2017). These simulations predict that PRIMER will reveal ~ 120,000 galaxies, ~ 70% of which are new (i.e. undetected by HST or Spitzer)