Fig. 4.
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Hα pseudo-EWs as a function of spectral type obtained from the VIMOS spectra. The dashed and the dotted orange lines represent the accretion thresholds defined by Barrado y Navascués & Martín (2003) and Fang et al. (2009), respectively. The sources with the SpT K7 and M0 have been randomly displaced within (SpT-0.5, SpT+0.5), for clarity. The error bars are shown only when they are larger than the plotting symbols.
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