Best-fit number counts models and their integrated energy densities. Left: derived number counts models underlying distribution of sources in ELAN fields compared to blank field models (gray). To highlight the typical uncertainties in these models, we show the confidence bands for the Geach et al. model and for the Jackpot field. Right: extragalactic background light as a function of flux. In both panels, the models for ELANe are plotted in solid at the flux range of the measured counts, and dashed in flux regimes fainter than our measurements.