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Table 2.
Contribution of emitting sources in halos per halo mass bin.
| ΔLogM200 | All | no eSASS PT | ||||
|---|---|---|---|---|---|---|
| no eSASS PT | ||||||
| XRB | AGN | IGrM | XRB | AGN | IGrM | |
| 12.2 − 12.5 | 0.15 | 0.63 | 0.22 | 0.12 | 0.65 | 0.23 |
| 12.5 − 12.8 | 0.11 | 0.64 | 0.25 | 0.09 | 0.64 | 0.26 |
| 12.8 − 13.1 | 0.05 | 0.66 | 0.30 | 0.04 | 0.67 | 0.29 |
| 13.1 − 13.4 | 0.03 | 0.39 | 0.58 | 0.02 | 0.37 | 0.61 |
| 13.4 − 13.7 | 0.01 | 0.25 | 0.74 | 0.01 | 0.21 | 0.78 |
| 13.7 − 14.0 | 0.01 | 0.26 | 0.73 | 0.01 | 0.21 | 0.78 |
Notes. The table shows the average contributions in all halos and in halos not containing eSASS detected point sources (PT).
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