The OTELO survey - New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38 < z < 1.43

Open Access

Fig. 4.

sSFRF of the Hα (black dots), Hβ (red dots), and [O II] (blue dots) from the OTELO survey. The solid lines represent the log-normal fitting functions for each line (black for Hα, red for Hβ, and blue for [O II]), following Ilbert et al. (2015)’s recipe. The shaded areas represent the propagation of 1σ uncertainties of the tabulated fits after 10⁵ Monte Carlo simulations.

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