Improved measurements of the age of JWST galaxies at z=6-10
M. Lopez-Corredoira, C. M. Gutierrez

TL;DR
This study refines the age estimates of high-redshift JWST galaxies using combined photometry and spectroscopy, revealing some galaxies may be older than the universe's age, indicating potential model uncertainties.
Contribution
It provides improved age measurements of z=6-10 galaxies by integrating spectroscopic and photometric data with advanced SED fitting, highlighting possible tensions with cosmological models.
Findings
Average galaxy age: 0.61 Gyr, close to universe age
Some galaxies appear older than the universe, indicating model issues
Most galaxies have minimal AGN contribution at red wavelengths
Abstract
From James Webb Space Telescope (JWST) surveys, 31 galaxies with average redshift 7.3 are selected containing large Balmer break, Lyman- break (V-shaped SED versus ). Apart from Hubble Space Telescope (HST) and JWST-NIRCam (Near-infrared camera) photometry for these galaxies, there are JWST-NIRSpec (Near-infrared spectrograph) spectra for 13 galaxies and mid-infrared photometry (mostly JWST-MIRI) for 15 of them. Spectroscopical analyses included Balmer emission lines, Balmer + 4000 angstroms breaks or CaII lines. Spectral energy distribution (SED) fitting with photometry include old and young stellar populations, emission lines associated to HII regions, AGN, interstellar dust extinction and intergalactic extinction from neutral hydrogen. By adopting realistic extinction curves and taking into account the V-shaped SED and low emission at near infrared at rest, the…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Space Technology and Applications
