SMOG - a Statistical Model of Galaxies

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...

!!! Under Construction !!!

In the meantime, you can browse the html version of the GAIA-CUO-104 technical report.


Please contact Mattia Vaccari for further information


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