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Fig. 14

image

Distribution of L(Hα) for the WINGS sources (w1 sample), for Hii, TOs, Seyferts, and LINERs (black line), and for the sources analyzed by Sabater et al. (2012, blue). Gray lines trace the distribution of upper limits for the w0 sample.Objects classified with censored emission line ratios are included in the histogram.

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