JADES-GS-z13-1

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JADES-GS-z13-1
JADES-GS-z13-1.png
Image of JADES-GS-z13-1 taken with the James Webb Space Telescope
Observation data
Constellation Fornax
Right ascension 03h 32m 15.57s
Declination −27° 53′ 23.29″
Redshift 13.0
Distance 13.47 billion light-years
(light travel distance)
33.31 billion light-years
(present proper distance)
Characteristics
Type Lyman-alpha emitter
Other designations
JADES-GS-z13-1-LA, JADES-GS+53.06475-27.89024

JADES-GS-z13-1 or JADES-GS-z13-1-LA (also known as JADES-GS+53.06475-27.89024) is a high-redshift Lyman-Break galaxy in the constellation Fornax that was observed with the NIRSpec instrument of the James Webb Space Telescope between 10 and 12 January 2024 as part of the JADES and JADES Origins Field (JOF) programmes.

Contents

It has a redshift of 13.0, making it one of the most distant galaxies discovered. According to current theory, this redshift corresponds to a time about 13.47 billion years ago, approximately 330 million years after the Big Bang, or about 2,4% of its current age. [1]

JADES-GS-z13-1-LA  and the onset of reionization

Cosmic reionization began when ultraviolet (UV) radiation produced in the first galaxies began illuminating the cold, neutral gas that filled the primordial Universe .

The spectroscopy of JADES-GS-z13-1-LA reveals a singular, bright emission line unambiguously identified as Lyman-α, as well as a smooth turnover. [1]

Smooth turnover of the UV continua has been interpreted as damping-wing absorption of Lyman-α (Ly-α), the principal hydrogen transition. [2]

It is observed in JADES-GS-z13-1-LA an equivalent width of EW Ly-α > 40 Å (rest frame), previously only seen at z < 9 where the intervening intergalactic medium becomes increasingly ionized. [3] Together with an extremely blue UV continuum, the unexpected Ly-α emission indicates that the galaxy is a prolific producer and leaker of ionizing photons. This suggests that massive, hot stars or an active galactic nucleus have created an early reionized region to prevent complete extinction of Ly-α. [1]

Whether the Ly-α emission of JADES-GS-z13-1-LA originates in stars or a supermassive black hole, it reveals the rather extreme character of one of the earliest galaxies known, despite having been found in a modest survey area examining a comoving volume of 50,000 Mpc3 between z = 11 and z = 15. [1]

At only 330 Myr after the Big Bang, the probable presence of a reionized region around this relatively UV-faint source readily constrains the timeline of cosmic reionization, favouring an early and gradual process driven (initially) by low-mass galaxies. [4]

References

  1. 1 2 3 4 Witstok, Joris; Jakobsen, Peter; Maiolino, Roberto; Helton, Jakob M.; Johnson, Benjamin D.; Robertson, Brant E.; Tacchella, Sandro; Cameron, Alex J.; Smit, Renske; Bunker, Andrew J.; Saxena, Aayush; Sun, Fengwu; et al. (26 March 2025). "Witnessing the onset of reionization through Lyman-α emission at redshift 13". Nature. 639 (8056): 897–901. arXiv: 2408.16608 . Bibcode:2025Natur.639..897W. doi:10.1038/s41586-025-08779-5. hdl:11384/152525. PMC   11946913 . PMID   40140594.
  2. ↑ Hainline, Kevin N.; et al. (1 December 2024). "Searching for Emission Lines at z>11: The Role of Damped Lyα and Hints About the Escape of Ionizing Photons". The Astrophysical Journal. 976 (2): 160. arXiv: 2404.04325 . Bibcode:2024ApJ...976..160H. doi: 10.3847/1538-4357/ad8447 .
  3. ↑ Witstok, Joris; et al. (2025). "JADES: primaeval Lyman αemitting galaxies reveal early sites of reionization out to redshift z ∼9". Monthly Notices of the Royal Astronomical Society. 536: 27–50. doi: 10.1093/mnras/stae2535 .
  4. ↑ Qin, Yuxiang; Wyithe, J. Stuart B. (6 January 2025). "Reionization morphology and intrinsic velocity offsets allow transmission of Lyman- αemission from JADES-GS-z13-1-LA". MNRAS. 538: L16 –L23. doi: 10.1093/mnrasl/slaf001 .
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