Fig. 1.

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Diagnostic plots for selecting radio-AGN using LoTSS data. Red points mark the sources classified as radio-AGN after combining all four diagnostics, and grey points show the star-forming/radio-quiet AGN: (a) Dn(4000) vs L1.4 GHz/M⋆ plot. The solid and dashed curves mark the radio-AGN, intermediate and SF/RQAGN division from Best & Heckman (2012) and Sabater et al. (2019); (b) LHα versus L1.4 GHz plot, with the separation lines from Sabater et al. (2019); (c) BPT diagram where the solid curve shows the semi-empirical relation from Kauffmann et al. (2003), and the dashed curve shows the maximum starburst curve from Kewley et al. (2006); (d) WISE colour-colour plot for sources with the division line from Sabater et al. (2019).
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