Distribution of the [Ne V] sources on the SFR–L_bol plane. The color code indicates the age of the oldest stars in the host galaxy, as provided by sed3fit. Colored contours illustrate the number density of galaxies plus AGN at z ∼ 1 as predicted by the in situ co-evolution model (Mancuso et al. 2016a); orange, yellow, green, cyan, light blue, blue, and dark blue contours refer to number density of 10⁻⁴, 10⁻⁵, 10⁻⁶, 10⁻⁷, 10⁻⁸, 10⁻⁹ Mpc⁻¹, respectively. The black dashed lines show two evolutionary tracks (forward time direction indicated by the arrows) for AGNs with peak bolometric luminosity of 10^45.5 and 10^46.5 erg s⁻¹. The blue continuous line indicates where the SF luminosity is equal to the AGN luminosity. The average uncertainty on the t_age is ∼0.1 dex.