Forecasts indicate [Ne V] LIM cross-correlations can constrain mean AGN intensity and bias at cosmic noon with sensitivity to sources fainter than 5 sigma thresholds.
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AGN Line-Intensity Mapping: A Probe of Faint Black Holes at Cosmic Noon
Forecasts indicate [Ne V] LIM cross-correlations can constrain mean AGN intensity and bias at cosmic noon with sensitivity to sources fainter than 5 sigma thresholds.