Fig. 2.
Percentage of detected objects in the simulation depending on the EW of the input Hα Gaussian line. Light green: p ≥ 0.50 probability threshold. Dark green: p ≥ 0.95 probability threshold. Typical values of Hα EWs for multiple astrophysical objects are also indicated. Black squares: median values of EW as in Gavazzi et al. (2006). Black circles: mean values as in Gallego et al. (1997). Black triangles: maximum values from Stern & Laor (2012) and Gil de Paz et al. (2003).
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