Table A.1
Parameters for the Y500–M500 relation, expressed as 
.
| Sample | N c | MB | Mass | A | α | [ σlog Y | M ] int | [ σlog Y | M ] raw | Section |
|
|
||||||||
| XMM-ESZ PEPXI | 62 | N |
|
− 0.19 ∗ ± 0.01 ∗ | 1.74 ± 0.08 | 0.10 ∗ ± 0.01 ∗ | ... | A.2.1 |
| Cosmo sample | 71 | N |
|
− 0.175 ± 0.011 | 1.77 ± 0.06 | 0.065 ± 0.010 | 0.080 ± 0.009 | A.2.1 |
| Cosmo sample | 71 | Y |
|
− 0.186 ± 0.011 | 1.79 ± 0.06 | 0.063 ± 0.011 | 0.079 ± 0.009 | A.2.2 |
| XMM-ESZ | 62 | Y |
|
− 0.19 ∗ ± 0.01 ∗ | 1.75 ± 0.07 | 0.065 ± 0.011 | 0.079 ± 0.009 | A.2.3 |
| S/N > 7 | 78 | Y |
|
− 0.18 ∗ ± 0.01 ∗ | 1.72 ± 0.06 | 0.063 ± 0.010 | 0.078 ± 0.008 | A.2.3 |
| Cosmo sub-sample A | 10 | Y |
|
− 0.15 ∗ ± 0.04 ∗ | 1.6 ∗ ± 0.3 ∗ | ... | 0.08 ∗ ± 0.02 ∗ | A.3.2 |
| Cosmo sub-sample B | 58 | Y |
|
− 0.19 ∗ ± 0.03 ∗ | 1.7 ∗ ± 0.2 ∗ | 0.25 ∗ ± 0.06 ∗ | 0.27 ∗ ± 0.06 ∗ | A.3.2 |
Notes. Column 1, considered sample; Col. 2, number of clusters in the sample; Col. 3, Malmquist bias correction; if this column contains Y, a mean correction for Malmquist bias has been applied to each point before fitting; Col. 4, mass definition; Cols. 5 and 6, slope and normalization of the relation; Cols. 7 and 8, intrinsic and raw orthogonal scatter around the best-fit relation at a given mass; Col. 9, Section in which sub-sample is discussed. The Cosmo sample highlighted in bold represents the baseline relation (see text for details).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.