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Table 1.

Inputs to simulation models.

Properties Simulation run UV HI shielding H2 shielding IMF εSN Extra modules
(a) (b) (c) (d) (e) (f) (g) (h)
HM HM DB96 S 0.1
HM-HISS HM R13 DB96 S 0.1
HM-HISSmed (ref) HM B.1 DB96 S 0.1
P19 P19 DB96 S 0.1
UV rate P19-HISS P19 R13 DB96 S 0.1
Modeling P19-HISSmed P19 B.1 DB96 S 0.1
FG20 FG20 DB96 S 0.1
FG20-HISS FG20 R13 DB96 S 0.1
FG20-HISSmed FG20 B.1 DB96 S 0.1

HM-std HM DB96 S 0.1 Threshold 0.1 cm−3
Star formation HM-HISSmed-std HM B.1 DB96 S 0.1 Threshold 0.1 cm−3
HM-HISSmed-H2 HM B.1 DB96 S 0.1 Non-equilibrium H2-based

HM-HISSmed-3b HM B.1 DB96 S 0.1 3-body processes
HM-HISSmed-3b-DB2 HM B.1 DB96 (Eq. (37)) S 0.1 3-body processes
HM-HISSmed-3b-WG HM B.1 WG17 S 0.1 3-body processes
HM-HISSmed- HM B.1 DB96 S 0.1 channel only
HM-HISSmed-none HM B.1 DB96 S 0.1 No H2 channels
HM-HISSmed-cat-75-Zevol HM B.1 DB96 S 0.1 Catalysis at 75 K
HM-HISSmed-cat-75-pe HM B.1 DB96 S 0.1 Catalysis at 75 K and
photoelectric heating
Gas physics HM-HISS-cat-40-Zevol HM R13 DB96 S 0.1 Catalysis at 40 K
& chemistry HM-HISS-cat-75-Zevol HM R13 DB96 S 0.1 Catalysis at 75 K
HM-HISS-cat-120-Zevol HM R13 DB96 S 0.1 Catalysis at 120 K
HM-HISS-cat-Tcmb-Zevol HM R13 DB96 S 0.1 Catalysis at TCMB(z)
HM-HISS-cat-Tbeta-Zevol HM R13 DB96 S 0.1 Catalysis at Tβ(z)
HM-HISS-cat-75-Zsun HM R13 DB96 S 0.1 Catalysis at 75 K and Z = Z
HM-HISS-cat-75-0.01Zsun HM R13 DB96 S 0.1 Catalysis at 75 K and Z = 10−2Z
HM-HISS-cat-75-Zt HM R13 DB96 S 0.1 Catalysis at 75 K and Z = Z(t)
With Z(t)-dependent cooling
HM-cat-75-Zevol HM DB96 S 0.1 Catalysis at 75 K
HM-HISSmed-cr HM B.1 DB96 S 0.1 Constant ζ , all gas
HM-HISSmed-cr-P18 HM B.1 DB96 S 0.1 ζ by P18,(*) all gas
HM-HISSmed-cr-P18sfr HM B.1 DB96 S 0.1 ζ by P18,(*) SFR-scaled

HM-1 HM DB96 S 1.0
HM-0.5 HM DB96 S 0.5
HM-0.01 HM DB96 S 0.01
HM-w700 HM DB96 S 0.1 Wind velocity of 700 km s−1
Feedback HM-wf HM DB96 S 0.1 Winds decoupled for 0.1 tH
& IMF HM-Chabrier HM DB96 Ch 0.1
HM-1-Chabrier HM DB96 Ch 1.0
P19-1 P19 DB96 S 1.0
P19-Chabrier P19 DB96 Ch 0.1
P19-1-Chabrier P19 DB96 Ch 1.0

Notes. Blocks in the first column (a) collect, from top to bottom, runs with different implementation properties. Following columns refer to: simulation name (b), cosmological UV rates (c), HI shielding (d), H2 shielding (e), IMF (f), SN energy fraction (g), and description of extra modules adopted besides basics ones (h). UV backgrounds are by Haardt & Madau (1996, HM), Puchwein et al. (2019, P19) or Faucher-Giguère (2020, FG20); HI shielding by Rahmati et al. (2013, R13) or Eq. (B.1); H2 shielding by Draine & Bertoldi (1996, DB96, their Eq. (36) if not otherwise specified) or Wolcott-Green et al. (2017, WG17); IMF by Salpeter (1955, S) or Chabrier (2003, Ch). (*) Simple fit in Appendix E to the ℒ model by Padovani et al. (2018).

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