Table 2.
Observed rest-frame X-ray luminosity in the 0.5–2 keV band within R500c in erg s−1 of different components for CENhalo sample.
| log10(M200m) |
log10(M500c) |
Redshift |
CENhalo sample |
||||||
|---|---|---|---|---|---|---|---|---|---|
| LX, total | LX, mask | LX, CGM | LX, AGN + XRB + SAT | ||||||
| min | max | min | max | min | max | (no mask) | (with mask) | (with mask) | |
| 11.5 | 12.0 | 11.3 | 11.8 | 0.01 | 0.08 | (1.2 ± 0.5)×1040 | (5.2 ± 1.5)×1039 | (3.0 ± 1.6)×1039 | (2.2 ± 0.5)×1039 |
| 12.0 | 12.5 | 11.8 | 12.3 | 0.02 | 0.13 | (3.9 ± 0.7)×1040 | (1.9 ± 0.3)×1040 | (1.1 ± 0.4)×1040 | (8.3 ± 2.2)×1039 |
| 12.5 | 12.75 | 12.3 | 12.5 | 0.02 | 0.16 | (9.7 ± 1.6)×1040 | (5.0 ± 0.9)×1040 | (3.4 ± 1.0)×1040 | (1.6 ± 0.6)×1040 |
| 12.75 | 13.0 | 12.5 | 12.8 | 0.02 | 0.16 | (1.5 ± 0.3)×1041 | (7.0 ± 1.7)×1040 | (5.7 ± 1.7)×1040 | (1.3 ± 0.4)×1040 |
| 13.0 | 13.25 | 12.8 | 13.0 | 0.03 | 0.20 | (2.6 ± 0.8)×1041 | (1.5 ± 0.2)×1041 | (1.3 ± 0.2)×1041 | (1.6 ± 0.4)×1040 |
| 13.25 | 13.5 | 13.0 | 13.3 | 0.03 | 0.20 | (4.5 ± 0.6)×1041 | (3.7 ± 0.4)×1041 | (3.5 ± 0.4)×1041 | (2.3 ± 0.6)×1040 |
| 13.5 | 13.75 | 13.3 | 13.5 | 0.03 | 0.20 | (8.6 ± 1.0)×1041 | (6.4 ± 0.7)×1041 | (6.1 ± 0.7)×1041 | (3.2 ± 0.7)×1040 |
| 13.75 | 14.0 | 13.5 | 13.7 | 0.03 | 0.20 | (1.6 ± 0.2)×1042 | (1.4 ± 0.1)×1042 | (1.3 ± 0.1)×1042 | (4.6 ± 1.0)×1040 |
Notes. The CENhalo sample binned in M200m derived based on the group finder algorithm (Tinker 2021), the corresponding M500c derived considering the concentration model from Ishiyama et al. (2021) and the redshift bins. The luminosities are defined in Table 1.
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