Table E.1.
Parameters from the literature for UPP.
| Name | Reference | P0 | c500 | α | β | γ | δ |
|---|---|---|---|---|---|---|---|
| N07 | Nagai et al. (2007) | 3.3 | 1.8 | 1.3 | 4.3 | 0.7 | 2/3 |
| A10 | Arnaud et al. (2010) | 8.403 | 1.177 | 1.0510 | 5.4905 | 0.3081 | 2/3 + 0.12 |
| P13 | Planck Collaboration X (2013) | 6.41 | 1.81 | 1.33 | 4.13 | 0.31 | 2/3 + 0.12 |
| B17 | Bourdin et al. (2017), z < 0.5 sample | 5.25 | 1.18 | 1.27 | 5.41 | 0.31 | 2/3 |
| G19 | Ghirardini et al. (2019) | 5.68 | 1.49 | 1.33 | 4.40 | 0.43 | 2/3 |
| PACT | Pointecouteau et al. (2021) | 3.36 | 1.18 | 1.08 | 4.30 | 0.31 | 2/3 + 0.12 |
| MP23 | Melin & Pratt (2023) | 1.70 | 0.61 | 1.05 | 6.32 | 0.71 | 2/3 + 0.12 |
| S23( * ) | Sayers et al. (2023) | 100.74 | 1.4 | 100.12 | 100.74 | 0.3 | 2/3 |
Notes. We give the values for the gNFW parameters and δ obtained and considered in each work. ( * )For Sayers et al. (2023), we take δ = 2/3 despite deviations to this value being measured at low significance in their work. In addition, we consider the measured mass and redshift evolutions of the gNFW parameters to be not significant and take az = 0 and am = 0 for Eq. 6 in Sayers et al. (2023).
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