Table 4.
Summary of the median values and uncertainties at the 16th and 84th percentiles of the parameters in the HSE-to-lensing SR when considering a deviation from linearity, an offset between HSE and lensing masses or an evolution with redshift.
Cluster sample | # of clusters | No ![]() |
||||
---|---|---|---|---|---|---|
αHSE | βHSE | σHSE | σlens | γHSE | ||
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
[0] |
Reference sample (BCES) | 53 | 0.826 ± 0.886 | 0.481 ± 0.415 | 0.326( * ) | − | [0] |
Reference sample | 53 |
![]() |
[1] |
![]() |
![]() |
![]() |
Ref. no CL J1226.9+3332 | 52 |
![]() |
[1] |
![]() |
![]() |
![]() |
AHSE [1014 M⊙] | BHSE | σHSE [1014 M⊙] | σlens [1014 M⊙] | γHSE [1014 M⊙] | ||
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
[0] |
Reference sample (BCES) | 53 | 4.467 ± 1.85 | 0.246 ± 0.19 | 2.109( * ) | – | [0] |
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
![]() |
With ![]() |
||||||
αHSE | βHSE | σHSE | σlens | γHSE | ||
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
[0] |
Reference sample (BCES) | 53 | 1.000 ± 0.692 | 0.397 ± 0.324 | 0.191( * ) | – | [0] |
Reference sample | 53 |
![]() |
[1] |
![]() |
![]() |
![]() |
Ref. no CL J1226.9+3332 | 52 |
![]() |
[1] |
![]() |
![]() |
![]() |
AHSE [1014 M⊙] | BHSE | σHSE [1014 M⊙] | σlens [1014 M⊙] | γHSE [1014 M⊙] | ||
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
[0] |
Reference sample (BCES) | 53 | 4.644 ± 1.727 | 0.226 ± 0.176 | 1.340( * ) | − | [0] |
Reference sample | 53 |
![]() |
![]() |
![]() |
![]() |
![]() |
Notes. We present the results for the reference sample, accounting or not for the systematic scatter in the error bars of the masses. For the BCES fit we report the best-fit values and 1σ uncertainties. ( * )We also calculate the scatter with respect to the best BCES scaling relations following Eq. (4).
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