Table 1.
Simulation details of the feedback variations used in this work.
| Identifier | Δm* | Δfgas | AGN | Nb |
|---|---|---|---|---|
| (σ) | (σ) | |||
| L1_m9 | 0 | 0 | Thermal | 18003 |
| fgas+2σ | 0 | +2 | Thermal | 18003 |
| fgas-2σ | 0 | –2 | Thermal | 18003 |
| fgas-4σ | 0 | –4 | Thermal | 18003 |
| fgas-8σ | 0 | –8 | Thermal | 18003 |
| M*-σ | –1 | 0 | Thermal | 18003 |
| Jet | 0 | 0 | Jets | 18003 |
| Jet fgas-4σ | 0 | –4 | Jets | 18003 |
| L2p8_m9 | 0 | 0 | Thermal | 50403 |
Notes. All runs have a mean CDM particle mass of mCDM = 5.65 × 109 M⊙. The L2p8_m9 run has a box size of 2.8 Gpc while the rest have a box size of 1 Gpc. Identifier refers to the simulation run, Δm* is the number of standard deviations by which the observed stellar masses are shifted before calibration, Δfgas is the number of standard deviations the observed cluster gas fractions are shifted before calibration, AGN is the form of AGN feedback implemented, and Nb is the number of baryonic particles. All these runs assume the fiducial cosmology with h = 0.681, Ωm = 0.306, ΩΛ = 0.694, Ωb = 0.0486, Σmνc2 = 0.06eV, As = 2.099 × 10−9, ns = 0.967, σ8 = 0.807, and Ων = 1.39 × 10−3
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