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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Literature
Date: 1/7/2025

Arxiv: EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 46.5 < z < 13.5 using PEARLS and public JWST observations Published: 3/6/2024 8:14:21 PM Updated: 1/6/2025 6:45:50 PM
Literature
Date: 10/6/2024

Harvard ADS: JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4
Literature
Date: 9/2/2024

Arxiv: JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon Published: 5/13/2024 8:58:24 PM Updated: 8/30/2024 12:52:00 PM
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Literature
Date: 8/13/2024

Arxiv: JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4 Published: 12/18/2023 9:00:00 PM Updated: 8/12/2024 3:29:13 PM
Literature
Date: 7/23/2024

Harvard ADS: EPOCHS I. The Discovery and Star Forming Properties of Galaxies in the Epoch of Reionization at 6.5 < z < 18 with PEARLS and Public JWST data
Literature
Date: 7/23/2024

Arxiv: EPOCHS I. The Discovery and Star Forming Properties of Galaxies in the Epoch of Reionization at 6.5 < z < 18 with PEARLS and Public JWST data Published: 7/20/2024 11:18:59 PM Updated: 7/20/2024 11:18:59 PM
Literature
Date: 5/14/2024

Harvard ADS: JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
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EarlyReleases
Date: 5/14/2024

JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
EarlyReleases
Date: 5/14/2024

JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
Literature
Date: 5/14/2024

Arxiv: JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon Published: 5/13/2024 8:58:24 PM Updated: 5/13/2024 8:58:24 PM
Literature
Date: 4/23/2024

Arxiv: PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II Published: 2/21/2024 5:39:51 AM Updated: 4/21/2024 12:09:36 PM
Literature
Date: 4/17/2024

Arxiv: EPOCHS III: Unbiased UV continuum slopes at 6.5 < z < 13 from combined PEARLS GTO and public JWST NIRCam imaging Published: 4/16/2024 8:32:27 PM Updated: 4/16/2024 8:32:27 PM
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Literature
Date: 3/7/2024

Arxiv: EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations Published: 3/6/2024 8:14:21 PM Updated: 3/6/2024 8:14:21 PM
Literature
Date: 3/7/2024

Arxiv: EPOCHS Paper II: The Ultraviolet Luminosity Function from 7.5 < z < 13.5 using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data Published: 4/26/2023 8:57:02 PM Updated: 3/6/2024 5:08:08 PM
EarlyReleases
Date: 2/22/2024

PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II
Literature
Date: 2/22/2024

Arxiv: PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II Published: 2/21/2024 5:39:51 AM Updated: 2/21/2024 5:39:51 AM
Literature
Date: 2/15/2024

Arxiv: EPOCHS Paper II: The Ultraviolet Luminosity Function from 7.5 < z < 13.5 using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data Published: 4/26/2023 8:57:02 PM Updated: 2/14/2024 5:59:26 PM
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EarlyReleases
Date: 1/31/2024

PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc
EarlyReleases
Date: 1/31/2024

PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc
Literature
Date: 1/31/2024

IOP Science: PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc
Literature
Date: 1/18/2024

Arxiv: JWST's PEARLS: Improved Flux Calibration for NIRCam Published: 11/23/2023 3:02:17 AM Updated: 1/16/2024 5:46:53 PM
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
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EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
EarlyReleases
Date: 12/21/2023

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4
Literature
Date: 12/20/2023

Arxiv: JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z=0.4 Published: 12/18/2023 9:00:00 PM Updated: 12/18/2023 9:00:00 PM
EarlyReleases
Date: 11/27/2023

PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
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EarlyReleases
Date: 11/27/2023

PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
EarlyReleases
Date: 11/27/2023

JWST's PEARLS: Improved Flux Calibration for NIRCam
Literature
Date: 11/27/2023

IOP Science: PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
Literature
Date: 11/27/2023

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
Literature
Date: 11/22/2023

IOP Science: JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
EarlyReleases
Date: 11/10/2023

Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST
EarlyReleases
Date: 11/10/2023

Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST
Literature
Date: 11/10/2023

IOP Science: Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST
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GeneralNews
Date: 11/2/2023

Astronomy & Astrophysics highlight: JWST's PEARLS: Mothra, a new kaiju star at z=2.091 extremely magnified by MACS0416, and implications for dark matter models
Literature
Date: 11/2/2023

IOP Science: PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field
Literature
Date: 10/13/2023

Arxiv: JWST's PEARLS: Transients in the MACS J0416.1-2403 Field Published: 7/14/2023 10:05:24 PM Updated: 10/12/2023 12:16:46 AM
Twitter
Date: 10/5/2023

William Keel | and see as their central black holes grow. Still, our understanding that other galaxies exist goes back just one century. What is still to be found out there? (Image: JWST/NASA/ESA/CSA/PEARLS team}
EarlyReleases
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
EarlyReleases
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
EarlyReleases
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
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EarlyReleases
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
EarlyReleases
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
Literature
Date: 9/28/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field Published: 9/22/2023 8:16:35 PM Updated: 9/27/2023 3:04:32 AM
Literature
Date: 9/25/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
Literature
Date: 9/25/2023

PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field Published: 9/22/2023 8:16:35 PM Updated: 9/22/2023 8:16:35 PM
Mastodon
Date: 9/11/2023

Kelly Lepo | Neat results from Rogier Windhorst from JWST PEARLS. A type Ia supernova at a redshift of z=1.783 (about 3.7 billion years ago) showed up as multiple images in a galaxy warped by gravitational lensing. Webb's first deep field is rather close to the Magellanic clouds, so there are more stars in the foreground from the Magellanic stream than an area of the sky 180 degrees away. # JWSTYearOne


EarlyReleases
Date: 9/6/2023

PEARLS: Near Infrared Photometry in the JWST North Ecliptic Pole Time Domain Field
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Literature
Date: 9/6/2023

PEARLS: Near Infrared Photometry in the JWST North Ecliptic Pole Time Domain Field Published: 8/31/2023 7:29:17 PM Updated: 9/5/2023 3:35:49 PM
Literature
Date: 9/4/2023

PEARLS: Near Infrared Photometry in the JWST North Ecliptic Pole Time Domain Field Published: 8/31/2023 7:29:17 PM Updated: 8/31/2023 7:29:17 PM

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