SMOG is a rough statistical model of some galaxy properties (such as number counts, morphological classification, angular sizes, surface brightness profiles...) I developed in collaboration with Erik Høg as part of my Master Thesis. As such, it is therefore heavily based on its Chapter 4 and Appendix D. Self-contained descriptions of SMOG are also available as technical reports SAG-CUO-61 (older version) and GAIA-CUO-104 (current version). This page is however still...
In the meantime, you can browse the html version of the GAIA-CUO-104 technical report.
Please contact Mattia Vaccari for further information