JWST/MIRI photometric detection at 7.7 microns 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 $z = 14.32_{-0.20}^{+0.08}$ with MIRI at $7.7\ \mu\mathrm{m}$ . 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 $7.7\ \mu\mathrm{m}$ comes from the rest-optical emission lines $\mathrm{H}\beta$ and/or $\mathrm{[OIII]}\lambda\lambda4959,5007$ . The inferred properties of JADES-GS-z14-0 suggest rapid mass assembly and metal enrichment during the earliest phases of galaxy formation.

eprint arXiv:2405.18462