Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
Maria Emilia De Rossi, Volker Bromm

TL;DR
This paper models the detectability of the first galaxies in far-infrared surveys, showing that upcoming space telescopes could observe galaxies at redshifts above 7, depending on dust properties and survey sensitivity.
Contribution
It introduces an analytical model of primordial dust emission to predict the redshift horizon for detecting early galaxies with future FIR telescopes.
Findings
Detection horizon extends above z~7 for sensitivities below 0.5 μJy.
Higher metallicity and dust-to-metal ratios improve detection prospects.
Survey area and dust properties significantly influence detection capabilities.
Abstract
We explore the possibility of detecting the first galaxies with the next generation of space-based far infrared (FIR) telescopes by applying an analytical model of primordial dust emission. Our results indicate that FIR/sub-mm sources at will experience a strong negative K-correction. Systems of a given virial mass would exhibit larger dust luminosities at higher , as a consequence of the increase in dust temperature driven by the higher temperature floor set by the cosmic microwave background. In addition, high- systems are more concentrated, which enhances the heating efficiency associated with stellar radiation. By analysing source densities as a function of , and considering survey areas of 0.1 and 10 , we find that the redshift horizon for detecting at least one source would be above for instrument sensitivities $\lesssim…
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