An extremely metal-poor star complex in the reionization era: Approaching Population III stars with JWST

Abstract

We present JWST/Near Infrared Spectrograph (NIRSpec) integral field spectroscopy (IFS) of a lensed Population III candidate stellar complex (dubbed Lensed And Pristine 1, LAP1), with a lensing-corrected stellar mass of ≲10 4 M ⊙ and an absolute luminosity of M UV > −11.2 ( m UV > 35.6), confirmed at redshift 6.639 ± 0.004. The system is strongly amplified ( μ ≳ 100) by straddling a critical line of the Hubble Frontier Field galaxy cluster MACS J0416. Although the stellar continuum is currently not detected in the Hubble and JWST/Near Infrared Camera (NIRCam) and Near Infrared Imager and Slitless Spectrograph (NIRISS) imaging, arclet-like shapes of Lyman and Balmer lines, Ly α , H γ , H β and H α are detected with NIRSpec IFS with signal-to-noise ratios (S/N) of approximately 5 − 13 and large equivalent widths (> 300 − 2000 Å), along with a remarkably weak [O III ] λ λ 4959, 5007 at S / N ≃ 4. LAP1 shows a large ionizing photon production efficiency, log( ξ ion [erg Hz −1 ]) > 26. From the metallicity indexes R23 = ([O III ] + [O II ])/H β ≲ 0.74 and R3 = ([O III ]/H β ) = 0.55 ± 0.14, we derive an oxygen abundance of 12 + log(O/H)≲6.3. Intriguingly, the H α emission is also measured in mirrored subcomponents where no [O III ] is detected, providing even more stringent upper limits on the metallicity if in situ star formation is ongoing in this region (12 + log(O/H) < 6). The formal stellar mass limit of the subcomponents would correspond to ∼10 3 M ⊙ or M UV fainter than −10. Alternatively, this metal-free, pure line-emitting region could be the first case of a fluorescing H I gas region induced by transverse escaping ionizing radiation from a nearby star complex. The presence of large equivalent-width hydrogen lines and the deficiency of metal lines in such a small region make LAP1 the most metal-poor star-forming region currently known in the reionization era and a promising site that may host isolated, pristine stars.