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Table 1

Primary characteristics of the simulations analysed in this work.

Galaxy IMF c ϵSNe SR T max n th M

MUGS-g1536 Kroupa 0.05 40% 0% 15 000 0.1 7.0
MUGS-g15784 Kroupa 0.05 40% 0% 15 000 0.1 14.0
MaGICC-g1536 Chabrier 0.1 100% 10% 10 000 9.3 6.8
MaGICC-g15784 Chabrier 0.1 100% 10% 10 000 9.3 14.3
109-CH Kroupa01 0.01 100% 0.3 7.1

Notes. Information for each column: 1) simulation label; 2) initial mass function (KroupaKroupa et al. 1993; Kroupa01Kroupa 2001; ChabrierChabrier 2003); 3) star formation efficiency; 4) thermalised SNe energy fraction coupled to the interstellar medium (ISM); 5) thermalised massive star radiation energy fraction coupled to the ISM; 6) maximum allowable gas temperature for star formation (K); 7) minimum gas density needed for star formation (cm-3); 8) total mass of the galaxy (1011M).

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