Galaxies simulated with GALFORM

The galaxies in this dataset were simulated with the semi-analytical galaxy formation code GALFORM for the study of Jahns et al. 2023, titled “How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys”. The galaxies are used as the host galaxies of simulated fast radio bursts to do forecasts of their applications. The data comprises the galaxies star formation rate, stellar mass, and the photometric magnitudes in the observer frame, including extinction, in all passbands of the Sloan Digital Sky Survey, the Euclid satellite, the Vera Rubin Observatory, and the DECam.