Correction to: The role of environment and AGN feedback in quenching local galaxies: comparing cosmological hydrodynamical simulations to the SDSS.

The article titled "Correction to: The role of environment and AGN feedback in quenching local galaxies: comparing cosmological hydrodynamical simulations to the SDSS" by Goubert et al. has been published in the Monthly Notices of the Royal Astronomical Society. The study included an error in the calculation of nearest neighbor densities, which has now been corrected. The main results and conclusions of the publication remain unchanged, except for figure 16. The corrected pre-selection criteria and an updated version of the figure are presented in this erratum. The difference in density parameters between observations and simulations can be explained by the lower completeness of the data obtained from the SDSS. The fundamental conclusions regarding which galaxies quench via intrinsic and environmental routes remain the same. [Extracted from the article]