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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Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/GRISM Filters: F444W;GRISMR Start Time: 11/6/2024 2:14:37 PM Obs Time: 203.999(s) Proposal ID: 5398
Target Name: UNKNOWN Title: POPPIES: The Public Observation Pure Parallel Infrared Emission-Line Survey Instrument: NIRCAM/IMAGE Filters: F200W Start Time: 11/6/2024 2:14:37 PM Obs Time: 815.996(s) Proposal ID: 5398
Target Name: ADF22.A1 Title: Revealing the early phase of the co-evolution of galaxies and super-massive black holes at a z=3 proto-cluster core Instrument: MIRI/IMAGE Filters: F560W Start Time: 11/7/2023 9:07:24 PM Obs Time: 15480.672(s) Proposal ID: 3547
Target Name: ADF22.A1 Title: Revealing the early phase of the co-evolution of galaxies and super-massive black holes at a z=3 proto-cluster core Instrument: MIRI/IFU Filters: CH4-SHORT Start Time: 11/7/2023 9:07:25 PM Obs Time: 15480.672(s) Proposal ID: 3547
Target Name: ADF22.A1 Title: Revealing the early phase of the co-evolution of galaxies and super-massive black holes at a z=3 proto-cluster core Instrument: MIRI/IFU Filters: CH3-SHORT Start Time: 11/7/2023 9:07:25 PM Obs Time: 15480.672(s) Proposal ID: 3547
Target Name: ADF22.A1 Title: Revealing the early phase of the co-evolution of galaxies and super-massive black holes at a z=3 proto-cluster core Instrument: MIRI/IFU Filters: CH2-SHORT Start Time: 11/7/2023 9:07:25 PM Obs Time: 15480.672(s) Proposal ID: 3547
Target Name: ADF22.A1 Title: Revealing the early phase of the co-evolution of galaxies and super-massive black holes at a z=3 proto-cluster core Instrument: MIRI/IFU Filters: CH1-SHORT Start Time: 11/7/2023 9:07:25 PM Obs Time: 15480.672(s) Proposal ID: 3547
Target Name: SQ-MRS-BRIDGE-ALMAFIELD5 Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F560W Start Time: 11/7/2023 12:55:45 PM Obs Time: 2102.312(s) Proposal ID: 3445
Target Name: SQ-MRS-BRIDGE-ALMAFIELD5 Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1130W Start Time: 11/7/2023 2:28:31 PM Obs Time: 2102.312(s) Proposal ID: 3445
Target Name: SQ-MRS-BRIDGE-ALMAFIELD5 Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1000W Start Time: 11/7/2023 1:42:44 PM Obs Time: 2102.312(s) Proposal ID: 3445
Kelly Lepo | JWST's primary mirror is made up of 18 hexagonal, gold-coated segments. A new blog post is out today from the team that keeps the mirror segments perfectly aligned so that they function as one big mirror. So far, everything is going great. The overall performance of the telescope is far better than expected, and the alignment needs fewer corrections than expected. https:// blogs.nasa.gov/webb/2024/11/08 /monitoring-webbs-mirrors-for-optimal-optics/ # JWST # NASA # Astronomy
Harvard ADS: Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at z = 4.5 - 8.5
Harvard ADS: Mapping reionization bubbles in the JWST era I: empirical edge detection with Lyman alpha emission from galaxies
Daniel Pomarède | in the # arXiv J1721+8842: The first Einstein zig-zag lens by Frédéric Dux and co-authors https:// arxiv.org/abs/2411.04177 # Cosmology # galaxies # quasars # lensing # astronomy # astrophysics # astrodon # JWST # Webb # telescope # space # science # STEM
Arxiv: Mapping reionization bubbles in the JWST era I: empirical edge detection with Lyman alpha emission from galaxies Published: 11/6/2024 9:00:01 PM Updated: 11/6/2024 9:00:01 PM
Target Name: TOI-421 Title: Unshrouding the Sub-Neptune Population: The Case of TOI-421b Instrument: NIRISS/SOSS Filters: CLEAR;GR700XD Start Time: 11/6/2023 2:05:01 PM Obs Time: 10368.162(s) Proposal ID: 1935
Target Name: SQ-MRS-COS-P5-BRIDGE Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F560W Start Time: 11/7/2023 9:29:30 AM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SQ-MRS-COS-P5-BRIDGE Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1130W Start Time: 11/7/2023 11:38:54 AM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SQ-MRS-COS-P5-BRIDGE Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1000W Start Time: 11/7/2023 10:34:24 AM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SQ-MRS-SKY-BACKGROUND Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F560W Start Time: 11/7/2023 3:27:51 PM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SQ-MRS-SKY-BACKGROUND Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1130W Start Time: 11/7/2023 5:36:52 PM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SQ-MRS-SKY-BACKGROUND Title: Shaken and Stirred: Shocks and Turbulence in the Stephans Quintet Warm Molecular Filament Instrument: MIRI/IMAGE Filters: F1000W Start Time: 11/7/2023 4:32:45 PM Obs Time: 3153.468(s) Proposal ID: 3445
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F770W Start Time: 11/7/2023 7:17:53 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F560W Start Time: 11/7/2023 7:08:49 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F2550W Start Time: 11/7/2023 8:21:28 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F2100W Start Time: 11/7/2023 8:11:59 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F1800W Start Time: 11/7/2023 8:03:07 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F1500W Start Time: 11/7/2023 7:54:17 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F1280W Start Time: 11/7/2023 7:45:24 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F1130W Start Time: 11/7/2023 7:36:34 PM Obs Time: 111(s) Proposal ID: 3295
Target Name: SN2022WSP Title: Is there enough? Cosmic dust formation in normal core-collapse supernovae in the first ~5 years post-explosion Instrument: MIRI/IMAGE Filters: F1000W Start Time: 11/7/2023 7:27:38 PM Obs Time: 111(s) Proposal ID: 3295
David Meyer | "Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A), which has been annotated to highlight key structures. At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W)." 1987A is an awesome thing... https:// webbtelescope.org/contents/med ia/images/2023/136/01H8Q0YNFRGYKJC8JM90V1WHSG # astronomy # supernova # 1987A # physics # NASA # JWST