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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Hints of point-symmetric structures in SN 1987A: the jittering jets explosion mechanism
Arxiv: GA-NIFS: JWST/NIRSpec IFU observations of HFLS3 reveal a dense galaxy group at z~6.3 Published: 8/31/2023 1:28:16 PM Updated: 12/1/2023 7:10:37 PM
Harvard ADS: Hints of point-symmetric structures in SN 1987A: The jittering jets explosion mechanism
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Harvard ADS: TransitFit: combined multi-instrument exoplanet transit fitting for JWST, HST, and ground-based transmission spectroscopy studies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
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A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
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A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
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A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
Harvard ADS: JADES: A large population of obscured, narrow line AGN at high redshift
Harvard ADS: A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies
IOP Science: XUE: Molecular Inventory in the Inner Region of an Extremely Irradiated Protoplanetary Disk
Arxiv: 2D disc modelling of the JWST line spectrum of EX Lupi Published: 11/30/2023 9:45:39 AM Updated: 11/30/2023 9:45:39 AM
Arxiv: A rest-frame near-IR study of clumps in galaxies at 1 < z < 2 using JWST/NIRCam: connection to galaxy bulges Published: 9/11/2023 9:03:10 PM Updated: 11/30/2023 3:21:32 AM
Harvard ADS: JOYS+: mid-infrared detection of gas-phase SO_2 emission in a low-mass protostar. The case of NGC 1333 IRAS2A: hot core or accretion shock?
Arxiv: A high incidence of dusty Hα emitters at z>3 among UltraVISTA dropout galaxies in COSMOS revealed by JWST Published: 11/29/2023 6:04:59 PM Updated: 11/29/2023 6:04:59 PM
Arxiv: JWST/NIRSpec Observations of the Coldest Known Brown Dwarf Published: 11/29/2023 4:11:17 AM Updated: 11/29/2023 4:11:17 AM
Arxiv: Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST Published: 10/27/2023 9:00:01 PM Updated: 11/29/2023 7:32:19 PM
High-contrast JWST-MIRI spectroscopy of planet-forming disks for the JDISC Survey
Arxiv: High-contrast JWST-MIRI spectroscopy of planet-forming disks for the JDISC Survey Published: 11/28/2023 8:19:47 PM Updated: 11/28/2023 8:19:47 PM
Arxiv: An Algorithm to Mitigate Charge Migration Effects in Data from the Near Infrared Imager and Slitless Spectrograph on the James Webb Space Telescope Published: 11/27/2023 10:27:05 PM Updated: 11/27/2023 10:27:05 PM
Arxiv: Optical Properties of Organic Haze Analogues in Water-rich Exoplanet Atmospheres Observable with JWST Published: 1/7/2023 1:14:19 AM Updated: 11/28/2023 3:51:54 PM
Arxiv: Galaxy formation catalyzed by gravastars and the JWST, revisited Published: 10/6/2022 11:50:30 PM Updated: 11/27/2023 9:42:33 PM
Harvard ADS: Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z=4 to 8 from CEERS
Arxiv: Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations Published: 11/27/2023 8:43:09 PM Updated: 11/27/2023 8:43:09 PM
Arxiv: A First Look with JWST Aperture Masking Interferometry (AMI): Resolving Circumstellar Dust around the Wolf-Rayet Binary WR 137 beyond the Rayleigh Limit Published: 11/27/2023 5:55:39 PM Updated: 11/27/2023 5:55:39 PM
Arxiv: Candidate Galaxies at z ~ 11.3--21.8 and beyond: results from JWST's public data taken in its first year Published: 11/25/2023 11:53:08 PM Updated: 11/25/2023 11:53:08 PM
Arxiv: Spherical Collapse Approach for Non-standard Cold Dark Matter Models and Enhanced Early Galaxy Formation in JWST Published: 11/25/2023 7:27:17 PM Updated: 11/25/2023 7:27:17 PM
Arxiv: JWST and ALMA discern the assembly of structural and obscured components in a high-redshift starburst galaxy Published: 11/24/2023 9:06:16 PM Updated: 11/24/2023 9:06:16 PM
PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
Harvard ADS: A MIRI Search for Planets and Dust Around WD 2149+02
IOP Science: PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
Arxiv: Feedback-Free Starbursts at Cosmic Dawn: Observable Predictions for JWST Published: 11/24/2023 8:50:39 PM Updated: 11/24/2023 8:50:39 PM
Arxiv: JWST's PEARLS: Improved Flux Calibration for NIRCam Published: 11/23/2023 3:02:17 AM Updated: 11/23/2023 3:02:17 AM
Arxiv: JWST spectroscopy of z\sim 5-8 UV-selected galaxies: New constraints on the evolution of the Lyα escape fraction in the reionization era Published: 11/22/2023 10:34:17 PM Updated: 11/22/2023 10:34:17 PM
Harvard ADS: Monthly Roundup: TRAPPIST-1 Through the Eyes of JWST
Arxiv: Spectral variability studies in Active Galactic Nuclei: Exploring continuum and emission line regions in the age of LSST and JWST Published: 11/22/2023 12:27:19 PM Updated: 11/22/2023 12:27:19 PM
MIDIS: The Relation between Strong (Hb+[OIII]) Emission, Star Formation and Burstiness Around the Epoch of Reionization
IOP Science: A Wolf 359 in Sheep's Clothing: Hunting for Substellar Companions in the Fifth-closest System Using Combined High-contrast Imaging and Radial Velocity Analysis
IOP Science: JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
Harvard ADS: MIDIS: The Relation between Strong (Hb+[OIII]) Emission, Star Formation and Burstiness Around the Epoch of Reionization
Harvard ADS: SO_2, silicate clouds, but no CH_4 detected in a warm Neptune
Harvard ADS: Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission
Harvard ADS: A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
Arxiv: High-precision astrometry and photometry with the JWST/MIRI imager Published: 11/20/2023 9:45:36 PM Updated: 11/20/2023 9:45:36 PM
IOP Science: CECILIA: The Faint Emission Line Spectrum of z ∼ 2–3 Star-forming Galaxies
