We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information. This dataset contains images/SEDs for Auriga galaxies 27-30 i.e. 4/30 galaxies.

Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme, grant agreement No. 683184 (Consolidator Grant LEGA-C). AUK, MB, DBA, and AT acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. IDL acknowledges support from ERC starting grant 851622 DustOrigin. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. The radiative transfer simulations carried out for this work used the Tier-2 facilities of the Flemish Supercomputer Center (https:// www.vscentrum.be/) located at the Ghent University.