Out of oxygen: Extremely metal-poor galaxy candidates identified at with deep JADES medium-band imaging
arXiv:2603.15761 · doi:10.1093/mnras/stag1360
Abstract
JWST is beginning to uncover a population of extremely metal-poor galaxies (EMPGs, ) at , mostly through serendipitous NIRSpec discoveries and blind slitless spectroscopy. To accelerate our understanding of pristine star formation, we further develop a methodology to identify EMPG candidates from photometry, using the extensive deep medium-band imaging from JADES. Our EMPG candidates at exhibit strong photometric boosts by H, yet correspondingly weak boosts by [O III] + H, likely indicating extremely low metallicity to explain their lack of [O III] emission. We further demand our EMPG candidates to have strong Balmer jumps, as revealed by medium-band imaging, to ensure that they are young starbursts, as opposed to broad-line AGN/LRDs, though contamination by dusty/dense-gas starbursts and highly-obscured AGN remains a concern. SED-fitting with near-pristine models (-) indicates that our 22 EMPG candidates are low-mass (median ), faint dwarf galaxies (), with high ionizing photon production efficiencies (). Hence these are plausible sites of near-pristine star formation, comprising - of galaxies at . We discuss this extremely metal-poor extension to the mass-metallicity relation. We forecast that deep ( h) NIRCam slitless spectroscopy can identify bright EMPGs through strong H but lack of [O III] emission, or secure the redshifts of fainter systems through H detections. Highly-multiplexed NIRSpec spectroscopy offers an alternate route to discovering the faintest pristine galaxies out to , without requiring deep medium-band/MIRI imaging to identify secure candidates.
26 pages, 14 figures, 2 tables. Updated author list
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