Table 1.
Observed rest-frame X-ray luminosity in the 0.5–2 keV band within R500c in erg s−1 of different components for CEN and isolated samples.
| log10(M*/M⊙)
|
Redshift |
Isolated sample |
|||||
|---|---|---|---|---|---|---|---|
| min | max | min | max | LX, total | LX, mask | ||
| (no mask) | (with mask) | ||||||
| 9.5 | 10.0 | 0.01 | 0.09 | 4.3 ± 2.4 × 1039 | 4.2 ± 1.2 × 1039 | ||
| 10.0 | 10.5 | 0.01 | 0.12 | 1.1 ± 0.4 × 1040 | 6.0 ± 1.5 × 1039 | ||
| 10.5 | 11.0 | 0.02 | 0.17 | 2.4 ± 0.7 × 1040 | 2.0 ± 0.2 × 1040 | ||
| 11.0 | 11.25 | 0.02 | 0.33 | 1.1 ± 0.2 × 1041 | 7.8 ± 0.9 × 1040 | ||
| 11.25 | 11.5 | 0.03 | 0.40 | 4.1 ± 0.8 × 1041 | 2.8 ± 0.3 × 1041 | ||
| log10(M*/M⊙)
|
Redshift |
CEN sample |
|||||
| min | max | min | max | LX, total | LX, mask | LX, CGM | LX, AGN + XRB + SAT |
| (no mask) | (with mask) | (with mask) | |||||
| 10.0 | 10.5 | 0.01 | 0.06 | (8.6 ± 5.6)×1039 | (3.8 ± 2.0)×1039 | (1.6 ± 2.1)×1039 | (2.2 ± 0.6)×1039 |
| 10.5 | 10.75 | 0.02 | 0.10 | (2.2 ± 0.8)×1040 | (1.2 ± 0.3)×1040 | (6.9 ± 3.0)×1039 | (5.2 ± 1.5)×1039 |
| 10.75 | 11.0 | 0.02 | 0.10 | (4.2 ± 1.0)×1040 | (2.1 ± 0.4)×1040 | (1.3 ± 0.4)×1040 | (8.2 ± 2.4)×1039 |
| 11.0 | 11.125 | 0.02 | 0.15 | (7.7 ± 2.1)×1040 | (4.3 ± 0.6)×1040 | (2.8 ± 0.8)×1040 | (1.5 ± 0.5)×1040 |
| 11.125 | 11.25 | 0.02 | 0.15 | (1.5 ± 0.3)×1041 | (8.7 ± 0.9)×1040 | (6.7 ± 1.0)×1040 | (2.0 ± 0.6)×1040 |
| 11.25 | 11.375 | 0.03 | 0.19 | (2.9 ± 0.5)×1041 | (1.8 ± 0.2)×1041 | (1.6 ± 0.2)×1041 | (2.5 ± 0.7)×1040 |
| 11.375 | 11.5 | 0.03 | 0.19 | (4.8 ± 0.4)×1041 | (3.7 ± 0.3)×1041 | (3.4 ± 0.3)×1041 | (3.4 ± 0.9)×1040 |
Notes. At different stellar mass bins (first two columns) within each redshift bin (the third and fourth columns), the X-ray luminosity of all X-ray emission (LX, total, without masking detected X-ray sources), the X-ray luminosity after excluding detected X-ray point sources (LX, mask, with masking X-ray point sources), the X-ray luminosity of hot CGM (LX, CGM), and modeled X-ray luminosity from unresolved AGN, XRB sources (LX, AGN + XRB + SAT).
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