Speaker
Laura Bisigello
(INAF-OAPD)
Description
In this talk I’ll present the most recent update of the state-of-the-art phenomenological simulation SPRITZ to include neutral hydrogen (HI). This update has been performed using the empirical stellar mass - HI mass relation and validate against available observations. SPRITZ already correctly reproduce the stellar mass function at different redshifts and the molecular gas mass density and with the inclusion of the HI it can be now be used to fully investigate the baryon content of the Universe and perform predictions for SKA.
| Topics | Galaxy Evolution & AGN |
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Author
Laura Bisigello
(INAF-OAPD)
