Table 1.
Simulation details of the runs used in this work.
| Identifier | Δm* | Δfgas | AGN | Nb | mCDM |
|---|---|---|---|---|---|
| (σ) | (σ) | (109 M⊙) | |||
| L1_m8 (m8) | 0 | 0 | Thermal | 36003 | 0.706 |
| L1_m9 (m9) | 0 | 0 | Thermal | 18003 | 5.65 |
| L1_m10 (m10) | 0 | 0 | Thermal | 9003 | 45.2 |
| L1_m8_DMO | – | – | – | 36003 | 0.84 |
| L1_m9_DMO | – | – | – | 18003 | 6.72 |
| L1_m10_DMO | – | – | – | 9003 | 53.8 |
| L2p8_m9 | 0 | 0 | Thermal | 50403 | 5.65 |
| fgas+2σ | 0 | +2 | Thermal | 18003 | 5.65 |
| fgas−2σ | 0 | −2 | Thermal | 18003 | 5.65 |
| fgas−4σ | 0 | −4 | Thermal | 18003 | 5.65 |
| fgas−8σ | 0 | −8 | Thermal | 18003 | 5.65 |
| M*−σ | −1 | 0 | Thermal | 18003 | 5.65 |
| Jet | 0 | 0 | Jets | 18003 | 5.65 |
Notes. 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, where m8, m9, and m10 indicate log10 of the mean baryonic particle mass. When absent, a feedback variation at the m9 resolution is being referred to. 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, Nb is the number of baryonic particles and mCDM the mean Cold Dark Matter (CDM) particle mass.
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