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Table 1.

Summary of the radiation energy bins adopted in our simulations.

Bin Range (eV) Metallicity bins (Z) Function Reference
IR 0.1 − 1 N/A IR radiation pressure (RP) Kannan et al. (2020a)
Opt. 1 − 5.8 {10−8, 10−6, 10−5, 10−4, 0.01, 1} RP T20 (EXT)
FUV 5.8 − 11.2 {10−8, 10−6, 10−5, 10−4, 0.01, 1} Photoelectric heating (PE), RP T20 (EXT)
LW 11.2 − 13.6 {10−8, 10−4, 0.007} H2 dissociation T20 (EXT), E19, GJ22
C I ionization, PE, RP
EUV1 13.6 − 24.6 {10−8, 0.001, 0.0282, 1} H I, H2 ionization, RP T20 (EXT), E19, LH03, S02
EUV2 24.6 − 54.4 {10−8, 0.001, 0.0282, 1} He I, H I, H2 ionization, RP T20 (EXT), E19, LH03, S02
EUV3 54.4 − ∞ {10−8, 10−6, 10−5, 10−4, 0.01, 1} He II, He I, H I, H2 ionization, RP T20 (EXT)

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