Cloudy with a chance of starshine: Possible photometric signatures of nebular-dominated emission in JADES galaxies
arXiv:2510.12622 · doi:10.1093/mnras/stag788
Abstract
The discovery of high-redshift galaxies exhibiting a steep spectral UV downturn potentially indicative of two-photon continuum emission marks a turning point in our search for signatures of top-heavy star formation in the early Universe. We develop a photometric search method for identifying further nebular-dominated galaxy candidates, whose nebular continuum dominates over the starlight, due to the high ionising photon production efficiencies associated with massive star formation. We utilise the extensive medium-band imaging from JADES, which enables the identification of Balmer jumps across a wide range of redshifts (), through the deficit in rest-frame optical continuum level. As Balmer jumps are a general recombination feature of young starbursts (~Myr), we further demand a high observed to power the strong nebular continuum, together with a relatively non-blue UV slope indicating a lack of stellar continuum emission. Our nebular-dominated candidates, constituting 10% of galaxies at (decreasing to 3% at , not completeness-corrected) are faint in the rest-frame optical (median ) with extreme line emission (median Å, Å). However, hot H II region temperatures, collisionally-enhanced two-photon continuum emission, and strong UV lines are expected to accompany top-heavy star formation. Thus nebular-dominated galaxies do not necessarily exhibit the biggest Balmer jumps, nor the largest or reddest UV slopes. Hence continuum spectroscopy is ultimately required to establish the presence of a two-photon downturn in our candidates, thus advancing our understanding of primordial star formation and AGN.
26 pages, 17 figures, 1 table
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