The unexpectedly high abundance of galaxies at z > 11 revealed by JWST has sparked a debate on the nature of early galaxies and the physical mechanisms regulating their formation. The Atacama Large Millimeter/submillimeter Array (ALMA) has begun to provide vital insights on their gas and dust content, but so far only for extreme ‘blue monsters’. Here we present new, deep ALMA observations of JADES-GS-z11-0, a more typical (sub- L * ) z > 11 galaxy that bridges the discovery space of JWST and the Hubble Space Telescope. These data confirm the presence of the O III 88 μ m line at 4.5 σ significance, precisely at the redshift of several faint emission lines previously seen with JWST/NIRSpec, while the underlying dust continuum remains undetected ( F ν 9.0 μ J y ), implying an obscured star formation rate (SFR) of SFR IR ≲ 6 M ⊙ y r − 1 and dust mass of M dust ≲ 1.0 × 10 6 M ⊙ (all 3 σ ). The accurate ALMA redshift of z O III = 11.1221 ± 0.0006 ( ≳ 5 × refined over NIRSpec) helps confirm that redshifts measured purely from the Lyman- α break, even spectroscopically, should properly take into account the effects of potential damped Lyman- α absorption (DLA) systems to avoid systematic overestimates of up to Δ z ≈ 0.5 . The O III 88 μ m luminosity of L O III = ( 1.1 ± 0.3 ) × 10 8 L ⊙ , meanwhile, agrees well with the scaling relation for local metal-poor dwarfs given the SFR measured by NIRCam, NIRSpec, and MIRI. The spatially resolved MIRI and ALMA emission also underscores that JADES-GS-z11-0 is likely to consist of two low-mass components that are undergoing strong bursts of star formation yet are already pre-enriched in oxygen ( ∼ 30 % solar), only 400 Myr after the Big Bang.
Zhu et al. (Mon,) studied this question.
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