James Webb Space Telescope Feed Post

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: 6/1/2023 8:50:00 PM

Paper abstract: Finding the first generation of stars formed out of pristine gas in the early Universe, known as Population III (PopIII) stars, is one of the most important goals of modern astrophysics. Recent models suggest that PopIII stars may form in pockets of pristine gas in the halo of more evolved galaxies. Here we present NIRSpec-IFU and NIRSpec-MSA observations of the region around GN-z11, an exceptionally luminous galaxy at z=10.6, which reveal a >5\sigma detection of a feature consistent with being HeII\lambda1640 emission at the redshift of GN-z11. The very high equivalent width of the putative HeII emission in this clump (170 A), and the lack of metal lines, can be explained in terms of photoionisation by PopIII stars, while photoionisation by PopII stars is inconsistent with the data. It would also indicate that the putative PopIII stars likely have a top-heavy initial mass function (IMF), with an upper cutoff reaching at least 500 M_\odot. The PopIII bolometric luminosity inferred from the HeII line would be ~ 2\times 10^{10}~L_\odot, which (with a top-heavy IMF) would imply a total stellar mass formed in the burst of ~ 6\times 10^{5}~M_\odot. We find that photoionisation by the Active Galactic Nucleus (AGN) in GN-z11 cannot account for the HeII luminosity observed in the clump, but can potentially be responsible for additional HeII emission observed closer to GN-z11. We also consider the possibility of in-situ photoionisation by an accreting Direct Collapse Black Hole (DCBH) hosted by the HeII clump; we find that this scenario is less favoured, but it remains a possible alternative interpretation. We also report the detection of a Ly\alpha halo stemming out of GN-z11 and extending out to ~2 kpc, as well as resolved, funnel-shaped CIII] emission, likely tracing the ionisation cone of the AGN.