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Table 1

Physical properties of the three simulations representative of various galaxy types in this work.

Model M f gas Redshift sSFR

spiral 6.5 × 1010M 9% z = 0 0.04 Gyr-1
SB merger 6.5 × 1010M (×2) 9% z = 0 0.63 Gyr-1
high-z disk 3.5 × 1010M 60% z = 2 0.97 Gyr-1

Notes. The specific star formation rate (sSFR) indicated here is averaged over the snapshots analyzed for each galaxy type: random for the spiral and high-z disk model, picked only in starbursting phases for the SB merger model. The stellar mass and gas fraction are the initial parameters of the models. A representative redshift is indicated for each model and is also used as an input parameter for the CMB temperature in the LVG grids.

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