1206.6923 (R. Overzier et al.)

The Millennium Run Observatory: First Light    [PDF]

R. Overzier, G. Lemson, R. E. Angulo, E. Bertin, J. Blaizot, B. M. B. Henriques, G. -D. Marleau, S. D. M. White

Simulations of galaxy evolution aim to capture our current understanding as well as to make predictions for testing by future experiments. Simulations and observations are often compared in an indirect fashion: physical quantities are estimated from the data and compared to models. However, many applications can benefit from a more direct approach, where the observing process is also simulated and the models are seen fully from the observer's perspective. To facilitate this, we have developed the Millennium Run Observatory (MRObs), a theoretical virtual observatory which uses virtual telescopes to `observe' semi-analytic galaxy formation models based on the suite of Millennium Run dark matter simulations. The MRObs produces data that can be processed and analyzed using the standard software packages developed for real observations. At present, we produce images in forty filters from the rest-frame UV to IR for two stellar population synthesis models, three different models of IGM absorption, and two cosmologies (WMAP1/7). Galaxy distributions for a large number of mock lightcones can be `observed' using models of major ground- and space-based telescopes. The data include lightcone catalogues linked to structural properties of galaxies, pre-observation model images, mock telescope images, and Source Extractor products that can all be traced back to the higher level dark matter, semi-analytic galaxy, and lightcone catalogues available in the Millennium database. Here, we describe our methods and announce a first public release of simulated observations for SDSS, CFHT-LS Wide/Deep, GOODS, ERS, CANDELS, and HUDF, and an online MRObs browser that facilitates exploration of these simulated data. We demonstrate the benefits of a direct approach through a number of example applications (deep galaxy counts, clusters, galaxy structures, and high-z dropouts).

View original: http://arxiv.org/abs/1206.6923