The James Webb Space Telescope Feed

Harvard ADS: JADES Ultrared Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations

Harvard ADS: Detection of [OIII]88\mum in JADES-GS-z14-0 at z=14.1793

Harvard ADS: JADES: Measuring reionization properties using Lyman-alpha emission

Harvard ADS: JADES: Measuring reionization properties using Lyman-alpha emission

Harvard ADS: The star-forming and ionizing properties of dwarf z 6-9 galaxies in JADES: insights on bursty star formation and ionized bubble growth

Harvard ADS: Ionising properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionising photon budget crisis at the Epoch of Reionisation

Harvard ADS: Ionising properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionising photon budget crisis at the Epoch of Reionisation

Harvard ADS: The star-forming and ionizing properties of dwarf z 6-9 galaxies in JADES: insights on bursty star formation and ionized bubble growth

Scientific European | Early Universe: The Most Distant Galaxy “JADES-GS-z14-0" Challenges Galaxy Formation Models   Spectral analysis of luminous galaxy JADES-GS-z14-0 based on observations made in January 2024 revealed a redshift of 14.32........... # earlyuniverse # galaxy # galaxyformation # JADES # JADESGSz140 # jameswebb # JamesWebbSpaceTelescope # JWST # Universe Umesh Prasa https://www. scientificeuropean.co.uk/scien ces/space/early-universe-the-most-distant-galaxy-jades-gs-z14-0-challenges-galaxy-formation-models/

Harvard ADS: JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations

Harvard ADS: JADES: Spectroscopic Confirmation and Proper Motion for a T-Dwarf at 2 Kiloparsecs

Harvard ADS: JADES -- The Rosetta Stone of JWST-discovered AGN: deciphering the intriguing nature of early AGN

Arxiv: JADES -- The Rosetta Stone of JWST-discovered AGN: deciphering the intriguing nature of early AGN Published: 7/11/2024 7:23:28 PM Updated: 7/11/2024 7:23:28 PM

Harvard ADS: A spectroscopic analysis of the ionizing photon production efficiency in JADES and CEERS: implications for the ionizing photon budget

Harvard ADS: JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy

JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy

Arxiv: JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy Published: 7/2/2024 9:00:32 PM Updated: 7/2/2024 9:00:32 PM

Harvard ADS: A NIRCam-dark Galaxy Detected with the MIRI/F1000W Filter in the MIDIS/JADES Hubble Ultra Deep Field

earthling | JADES-GS-z14-0: A New Farthest Object # JWST image that includes the most distant object yet discovered. Most # galaxies formed at about 3 billion years after the Big Bang, but some formed earlier. Pictured in the inset box is JADES-GS-z14-0, a faint smudge of a galaxy that formed only 300 million years after the universe started. The galaxy existed when the universe was only one fiftieth of the its present age. Practically all of the objects in the featured photograph are galaxies. # APOD

Harvard ADS: JADES: Physical properties of Ly\alpha and non-Ly\alpha emitters at z ~ 4.8-9.6

Arxiv: Detection of New Galaxy Candidates at z\ > 11 in the JADES Field Using JWST NIRCam Published: 6/8/2024 3:18:13 AM Updated: 6/16/2024 6:01:07 PM

Harvard ADS: Detection of New Galaxy Candidates at z\ > 11 in the JADES Field Using JWST NIRCam

Harvard ADS: The Star-Forming Main Sequence in JADES and CEERS at z>1.4: Investigating the Burstiness of Star Formation

Arxiv: Detection of New Galaxy Candidates at z\ > 11 in the JADES Field Using JWST NIRCam Published: 6/8/2024 3:18:13 AM Updated: 6/8/2024 3:18:13 AM

JADES Transients (NIRCam Image)

Three JADES galaxies with supernovae (2023 vs. 2022)

Transients in JADES field

Harvard ADS: The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field

Arxiv: JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy Published: 6/4/2023 11:44:23 PM Updated: 5/31/2024 7:07:03 PM

AkaSci 🛰️ | The following graphic illustrates the timeline in the early Universe when galaxy JADES-GS-z14-0 existed. 290 million years after the Big Bang, its light started the 13.5 light year journey to the JWST telescope. The first stars had just started to emerge ~200 million years after the Big Bang. It might require some modifications to current models to explain how JADES-GS-z14-0 grew so massive and voluminous so quickly, that too with multi-generational stars. https://www. snexplores.org/article/what-ha ppened-since-big-bang-physics-universe-cosmic-timeline # JWST 6/n

AkaSci 🛰️ | Redshift for distant objects can be estimated from their light spectra and noting the wavelengths of known emission and absorption lines. The Lyman-α break at 0.1215 µm is a distinct ultra-UV wavelength in astronomy; wavelengths shorter than it are absorbed by H in the source galaxy and in inter-galactic space. Redshift causes these wavelengths to get stretched. For JADES-GS-z14-0, Lyman-α was detected at 1.867 µm, i.e., z = (1.867 - 0.1215) / 0.1215 = 14.32. https:// webbtelescope.org/contents/med ia/images/01HZ0AGNJ96R1GSR956QYMFCRE # JWST 3/n

AkaSci 🛰️ | This week, a science team announced the discovery of JADES-GS-z14-0, a galaxy that existed just 290 million years after the big bang. JADES-GS-z14-0 now holds the record for the most distant known galaxy, with redshift z=14.32. The discovery is based on spectroscopic measurements made using the Webb telescope of light from this distant galaxy that has traveled for over 13.5 billion years. https:// webbtelescope.org/contents/ear ly-highlights/nasas-james-webb-space-telescope-finds-most-distant-known-galaxy # JWST # Webb 1/n

Webb finds most distant known galaxy (JADES-GS-z14-0 environment NIRCam image)

Webb finds most distant known galaxy (JADES-GS-z14-0 annotated pullout NIRCam image)

Harvard ADS: JADES - The small blue bump in GN-z11: insights into the nuclear region of a galaxy at z=10.6

Arxiv: JWST-JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11 Published: 6/1/2023 8:50:00 PM Updated: 4/16/2024 6:18:16 PM

Searching for Emission Lines at z > 11: The Role of Damped Lyman-a and Hints About the Escape of Ionizing Photons (JADES-GS-z13-0)

Searching for Emission Lines at z > 11: The Role of Damped Lyman-a and Hints About the Escape of Ionizing Photons (JADES-GS-z11-0)

Spatially resolved emission lines in galaxies at 4 <= z < 10 from the JADES survey: evidence for enhanced central star formation

Spatially resolved emission lines in galaxies at 4 <= z < 10 from the JADES survey: evidence for enhanced central star formation

Spatially resolved emission lines in galaxies at 4 <= z < 10 from the JADES survey: evidence for enhanced central star formation

Harvard ADS: Spatially resolved emission lines in galaxies at 4\leq z < 10 from the JADES survey: evidence for enhanced central star formation

A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/JADES Hubble Ultra Deep Field

A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/JADES Hubble Ultra Deep Field

A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/JADES Hubble Ultra Deep Field

The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S

The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI

A new census of dust and PAHs at z=0.7-2 with JWST MIRI