z=14 galaxies have arrived #225
Replies: 13 comments 46 replies
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I'll just tack this paper on here (rather than a different thread): Do high redshift QSOs and GRBs corroborate JWST?
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This is historic
They says, on average that those galaxies were estimated by current astrophysical models to be born at minimum, between 300 to 1800 millions years before the big bang. Note: I do not understand what takes JWST so long, the high redshift candidates were almost all, already discovered photometrically in 2022, many at Z=16, and even one at Z=20!! |
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https://arxiv.org/abs/2405.21054 The First Billion Years, According to JWST With stunning clarity, JWST has revealed the Universe's first billion years. The scientific community is analyzing a wealth of JWST imaging and spectroscopic data from that era, and is in the process of rewriting the astronomy textbooks. Here, 1.5 years into the JWST science mission, we provide a snapshot of the great progress made towards understanding the initial chapters of our cosmic history. We highlight discoveries and breakthroughs, topics and issues that are not yet understood, and questions that will be addressed in the coming years, as JWST continues its revolutionary observations of the Early Universe. |
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In addition to @mikehelland's reasons, 'Exoplanet research' and 'Spectroscopic confirmation is difficult', what makes it a slow process is that spectroscopic confirmations use emission lines but also the overall shape of the spectrum to fit star populations. The spectra of galaxies at z = 14 are fitted to spectra of galaxies at z = 13 with some changes to account for evolution. Astronomers don't understand the evolution of galaxies, so they must proceed incrementally from low redshift to high redshift, hence the sequential discovery of galaxies at higher and higher redshifts instead of a direct confirmation of the redshift of a z = 20 candidate. This paper contains twenty candidates at z >20, even some at z = 22! See pages 54-56. |
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First paper about GS-z14-0 (Z= 14.32) |
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Not as important as my last comment but new paper on the topic: |
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Discovery of a black hole disc "fully ‘mature’ less than 760 Myr after the Big Bang." I don't believe ? this is the same black hole as the recently discovered z=10 quasar here what is new is that not only the black hole, but its halo is resolved and considered mature.
So basically this is a falsification of all fast growth models except maybe the direct collapse ? If so the age of the universe is falsified. see also anomalously early spiral galaxies |
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Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang (at z=10.2) Those are I believe the earliest observed globular star clusters (thanks to lensing)
I wonder if their record high density is merely a product of them applying the expandist universe angular distance zoom factor, would be nice to compute @mikehelland and to check wether a static universe assumption leads to density close to local globular clusters. |
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The case for a younger universeI have always thought that the idea that the universe is in equilibrium and recycling, is albeit complex and requiring some new physics, more credible than the idea our universe drift towards its eternal non viability. One argument for this is to consider we are a random statistical sample, e.g. it is well understood that the idea that we live in a very highly preferential place spatially (geocentrism) is unlikely and unparcimonous. While I believed the universe is eternal or at least older than LCDM, there is one extremely potent argument that makes me consider having a younger universe than LCDM more likely. The thing that most cosmologists don't realize is that however unlikely you believe life appearance is, if the universe is eternal in time or infinite in space, in both scenarios it is an absolute certainty that an infinite number of intelligent aliens will have existed. Literally infinite independently of the base probability, that a basic and absolutely certain consequence when you have infinite iterations (time) or parallelism. So since we assume an infinite number of aliens, however how distant in space and time from us, some of them might not want to expand and conquer the universe, for philosophical, economical or military reasons (e.g the idea they are hiding from each others to avoid being invaded). The best tentative explanation is to consider that while the universe is eternal, we are not. And the planet earth might be relatively recent. While believe it or not, this is the strongest argument in cosmology, there has been a lack of empirical evidence for a younger universe. It goes without saying that a younger universe to explain observed formation history would require an altered dust attenuation model and mechanisms that catalyze star formation (MOND, super Eddington, altered IMF, etc) The situation has recently changed via two groundbreaking studies that indicate a younger universe (except maybe via some new physics) And the motions of satellite galaxies match a younger universe |
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Highest (?) redshift balmer break found and empirical evidence for a rejuvenation mechanism of galaxies
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https://arxiv.org/abs/2410.14671 Rapid Dust Formation in the Early Universe Interstellar dust links the formation of the first stars to the rocky planet we inhabit by playing a pivotal role in the cooling and fragmentation of molecular clouds, and catalyzing the formation of water and organic molecules. Despite its central role, the origin of dust and its formation timescale remain unknown. Some models favor rapid production in supernova ejecta as the primary origin of dust, while others invoke slower production by evolved asymptotic giant branch stars or grain growth in the interstellar medium (ISM). The dust content of young early-universe galaxies is highly sensitive to the dust formation timescales. Here, we evaluate the dust content of 631 galaxies at 3<zspec<14 based on rest-UV to optical spectroscopy obtained with JWST NIRSpec. We find that dust appears rapidly. Attenuation immediately follows star formation on timescales shorter than ∼30 Myr, favoring dust production by supernovae. The degree of attenuation is ∼30 times lower than expected if the entire supernova dust yield were preserved in the ISM, and had Milky Way-like grain properties. This can be reconciled if the early-universe dust is composed mostly of silicate or grains much larger than those in the Milky Way, and if significant dust destruction or ejection by outflows takes place. |
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unrelated to high Z but still the historic first imaging of extragalactic brown dwarf cluster |
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JWST/MIRI photometric detection at 7.7 μm of the stellar continuum and nebular emission in a galaxy at z>14
The James Webb Space Telescope (JWST) has spectroscopically confirmed numerous galaxies at z>10. While weak rest-ultraviolet emission lines have only been seen in a handful of sources, the stronger rest-optical emission lines are highly diagnostic and accessible at mid-infrared wavelengths with the Mid-Infrared Instrument (MIRI) of JWST. We report the photometric detection of the most distant spectroscopically confirmed galaxy JADES-GS-z14-0 at z=14.32+0.08−0.20 with MIRI at 7.7 μm. The most plausible solution for the stellar population properties is that this galaxy contains half a billion solar masses in stars with a strong burst of star formation in the most recent few million years. For this model, at least one-third of the flux at 7.7 μm comes from the rest-optical emission lines Hβ and/or [OIII]λλ4959,5007. The inferred properties of JADES-GS-z14-0 suggest rapid mass assembly and metal enrichment during the earliest phases of galaxy formation.
https://arxiv.org/abs/2405.18462
A shining cosmic dawn: spectroscopic confirmation of two luminous galaxies at z∼14
The discovery by JWST of an abundance of luminous galaxies in the very early Universe suggests that galaxies developed rapidly, in apparent tension with many standard models. However, most of these galaxies lack spectroscopic confirmation, so their distances and properties are uncertain. We present JADES JWST/NIRSpec spectroscopic confirmation of two luminous galaxies at redshifts of z=14.32+0.08−0.20 and z=13.90±0.17. The spectra reveal ultraviolet continua with prominent Lyman-α breaks but no detected emission lines. This discovery proves that luminous galaxies were already in place 300 million years after the Big Bang and are more common than what was expected before JWST. The most distant of the two galaxies is unexpectedly luminous (Muv=−20.81±0.16) and is spatially resolved with a radius of 260 parsecs. Considering also the steep ultraviolet slope of the second galaxy (β=−2.71±0.19), we conclude that both are dominated by stellar continuum emission, showing that the excess of luminous galaxies in the early Universe cannot be entirely explained by accretion onto black holes. Galaxy formation models will need to address the existence of such large and luminous galaxies so early in cosmic history.
https://arxiv.org/abs/2405.18485
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