dc.description.abstract | The Nancy Grace Roman Space Telescope, NASA’s next flagship observatory, will redefine deep-field galaxy survey with a field of view two orders of magnitude larger than
Hubble and an angular resolution of matching quality. These future deep-wide galaxy
surveys necessitate new simulations to forecast their scientific output and to optimise
survey strategies. In this work, we present five realizations of 2-deg2
lightcones, containing a total of & 25 million simulated galaxies with −16 & MUV & −25 spanning
z ∼ 0 to 10. This dataset enables a new set of experiments with the impacts of survey size on the derived galaxy formation and cosmological constraints. The intrinsic
and observable galaxy properties are predicted using a well-established, physics-based
semi-analytic modelling approach. We provide forecasts for number density, cosmic
SFR, field-to-field variance, and angular two-point correlation functions, and demonstrate how the future wide-field surveys will be able to improve these measurements
relative to current generation surveys. We also present a comparison between these
lightcones and others that have been constructed with empirical models. | en_US |