The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation
(2024)
Journal Article
Manzoni, G., Baugh, C. M., Norberg, P., Cabayol, L., van den Busch, J. L., Wittje, A., Navarro-Gironés, D., Eriksen, M., Fosalba, P., Carretero, J., Castander, F. J., Casas, R., De Vicente, J., Fernandez, E., García-Bellido, J., Gaztanaga, E., Helly, J. C., Hoekstra, H., Hildebrandt, H., Gonzalez, E. J., …Tortorelli, L. (2024). The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation. Monthly Notices of the Royal Astronomical Society, 530(2), 1394-1413. https://doi.org/10.1093/mnras/stae659
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 mag... Read More about The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation.