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Table 3.

Rest-frame X-ray luminosity in the 0.5–2 keV band within R500c in erg s−1 of different components for CEN and CENhalo samples.

log10(M*/M) CENSF


min max med LX, total LX, mask LX, CGM LX, AGN + XRB + SAT
(no mask) (with mask) (with mask)
10.0 10.5 10.2 8.9 ± 7.1 × 1039 2.5 ± 2.9 × 1039 2.7 ± 0.8 × 1039
10.5 11.0 10.7 3.6 ± 0.9 × 1040 1.7 ± 0.4 × 1040 8.0 ± 5.0 × 1039 9.2 ± 2.9 × 1039
11.0 11.25 11.1 1.3 ± 0.4 × 1041 5.0 ± 1.0 × 1040 2.3 ± 1.5 × 1040 2.6 ± 1.1 × 1040
11.25 11.5 11.3 2.7 ± 0.6 × 1041 7.8 ± 1.8 × 1040 4.0 ± 2.4 × 1040 3.8 ± 1.7 × 1040

CENQU

10.0 10.5 10.3 2.9 ± 2.7 × 1039 1.5 ± 2.7 × 1039 1.4 ± 0.6 × 1039
10.5 11.0 10.8 2.6 ± 0.9 × 1040 1.6 ± 0.4 × 1040 1.1 ± 0.4 × 1040 4.4 ± 1.0 × 1039
11.0 11.25 11.1 1.2 ± 0.3 × 1041 7.3 ± 0.8 × 1040 6.2 ± 0.8 × 1040 1.1 ± 0.3 × 1040
11.25 11.5 11.35 4.4 ± 0.6 × 1041 3.2 ± 0.2 × 1041 3.0 ± 0.2 × 1041 2.1 ± 0.4 × 1040

log10(M200 m/M) CENhalo, SF


min max med LX, total LX, mask LX, CGM LX, AGN + XRB + SAT
(no mask) (with mask) (with mask)

11.5 12.0 11.75 5.3 ± 3.6 × 1039 4.5 ± 1.6 × 1039 2.3 ± 1.7 × 1039 2.2 ± 0.5 × 1039
12.0 12.5 12.2 4.1 ± 0.9 × 1040 2.1 ± 0.4 × 1040 9.6 ± 5.8 × 1039 1.2 ± 0.4 × 1040
12.5 13.0 12.6 1.9 ± 0.4 × 1041 5.9 ± 1.1 × 1040 3.1 ± 1.6 × 1040 2.8 ± 1.3 × 1040
13.0 13.5 13.1 6.5 ± 2.5 × 1041 1.9 ± 0.7 × 1041 1.7 ± 0.7 × 1041 2.4 ± 1.8 × 1040

CENhalo, QU

11.5 12.0 11.7 2.7 ± 2.1 × 1040 6.2 ± 3.3 × 1039 2.7 ± 3.6 × 1039 3.5 ± 1.5 × 1039
12.0 12.5 12.25 3.6 ± 1.2 × 1040 1.4 ± 0.6 × 1040 9.6 ± 6.0 × 1039 4.9 ± 1.5 × 1039
12.5 13.0 12.8 6.7 ± 1.9 × 1040 4.6 ± 0.8 × 1040 3.7 ± 0.8 × 1040 9.1 ± 2.2 × 1039
13.0 13.5 13.2 3.2 ± 0.5 × 1041 2.4 ± 0.2 × 1041 2.3 ± 0.2 × 1041 1.7 ± 0.3 × 1040
13.5 14.0 13.7 1.1 ± 0.1 × 1042 8.6 ± 0.6 × 1041 8.2 ± 0.6 × 1041 3.7 ± 0.7 × 1040

Notes. For the CENSF and CENQU samples (top), CENhalo, SF and CENhalo, QU samples (bottom), the X-ray luminosity of all X-ray emission (LX, total, without masking detected X-ray sources), the X-ray luminosity after excluding detected 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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