• Vandenbusch, J. L.
• Vela, Pablo Fosalba
• Norberg, P.
• Sevilla-Noarbe, I.
• Hoekstra, Henk
• Siudek, Malgorzata
• Casas, R.
• Miquel, R.
• Sanchez, Eusebio
• Tortorelli, Luca
• Fernandez, E.
• Garcia-Bellido, Juan
• Gaztanaga, E.
• Baugh, Carlton
• Cabayol, L.
• Wittje, A.
• Gonzalez, Elizabeth
• Padilla, C.
• Koonkor, S.
• Eriksen, M.
• Carretero, J.
• Navarro Gironés, David
• Renard, Pablo
• Tallada-Crespì, P.
• Helly, J. C.
• Castander, Francisco Javier
• Vicente-Albendea, Juan De
• Hildebrandt, H.

Abstract

<jats:title>ABSTRACT</jats:title><jats:p>We use the GALFORM semi-analytical galaxy formation model implemented in the Planck Millennium N-body simulation to build a mock galaxy catalogue on an observer’s past lightcone. The mass resolution of this N-body simulation is almost an order of magnitude better than in previous simulations used for this purpose, allowing us to probe fainter galaxies and hence build a more complete mock catalogue at low redshifts. The high time cadence of the simulation outputs allows us to make improved calculations of galaxy properties and positions in the mock. We test the predictions of the mock against the Physics of the Accelerating Universe Survey, a narrow-band imaging survey with highly accurate and precise photometric redshifts, which probes the galaxy population over a lookback time of 8 billion years. We compare the model against the observed number counts, redshift distribution, and evolution of the observed colours and find good agreement; these statistics avoid the need for model-dependent processing of the observations. The model produces red and blue populations that have similar median colours to the observations. However, the bimodality of galaxy colours in the model is stronger than in the observations. This bimodality is reduced on including a simple model for errors in the GALFORM photometry. We examine how the model predictions for the observed galaxy colours change when perturbing key model parameters. This exercise shows that the median colours and relative abundance of red and blue galaxies provide constraints on the strength of the feedback driven by supernovae used in the model.</jats:p>

Topics

• impedance spectroscopy
• simulation
• strength