Table 5
Best-fit parameters of the scaling relations.
| Best fit parameters | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| Relation | Free redshift evolution | Self-similar redshift evolution | |||||||
| Y | X | A | B | C | σy |x | A | B | C = Cself | σ y|x |
| Lx | T |  |
 |
 |
 |
 |
 |
1 |  |
| Lx | Mgas |  |
 |
 |
 |
 |
 |
2 |  |
| Lx | Yx |  |
 |
 |
 |
 |
 |
 |
 |
| Lbol | T |  |
 |
 |
 |
 |
 |
1 |  |
| Lbol | Mgas |  |
 |
 |
 |
 |
 |
 |
 |
| Lbol | Yx |  |
 |
 |
 |
 |
 |
9/5 |  |
| Mgas | T |  |
 |
 |
 |
 |
 |
−1 |  |
Notes. Fitted relation is of the form 
with a log-normal intrinsic scatter σY|X (in natural log). Pivot values of the observables are provided in Table 3. Each relation is fitted twice; first leaving the redshift evolution exponent (C) free, and second with a redshift evolution exponent fixed to the corresponding self-similar value (see Table 4 for the self-similar exponents). Details of the modeling and fitting the scaling relations can be found in Sect. 3. Errors are 1c uncertainties calculated from the second half of the MCMC chains.
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