Euclid on Sky
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Fig. 36

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Expected number densities for photometric and spectroscopic emission line flux selected samples as a function of redshift in the Euclid Wide Survey. Different colours show various selection cuts for the EWS (in IE , HE , and in the 2 model calibrations for the line fluxes of fHα+[N II] > 2 × 10−16 erg s−1 cm−2). The empirical model of Pozzetti et al. (2016) and the data based on slitless HST spectroscopy (Bagley et al. 2020) are also shown.

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