Table 3.
Main properties of the PSZ2 cluster lenses per survey.
| Survey | Ncl | z | MSZ | (S/N)WL | nsources |
|---|---|---|---|---|---|
| [1014 M⊙] | [arcmin−2] | ||||
| HSC-SSP S16a | 5 | 0.20 ± 0.10 | 4.45 ± 1.34 | 2.45 ± 1.01 | 12.1 ± 4.9 |
| CFHTLenS | 8 | 0.16 ± 0.06 | 3.88 ± 1.28 | 2.69 ± 1.40 | 6.8 ± 2.4 |
| KiDS DR4 | 37 | 0.21 ± 0.12 | 4.36 ± 2.14 | 2.45 ± 1.47 | 2.8 ± 1.0 |
| DES SV1 | 11 | 0.37 ± 0.19 | 6.27 ± 3.87 | 0.99 ± 1.28 | 1.9 ± 1.3 |
| RCSLenS | 28 | 0.23 ± 0.17 | 4.69 ± 1.79 | 1.58 ± 2.17 | 1.9 ± 1.4 |
Notes. We list the number of clusters in the considered survey footprint and their typical redshift; mass proxy value, here the catalogue SZ mass in units of 1014 M⊙, (S/N)WL; and the source galaxy density per cluster (in units of arcmin−2). Location and scale are computed as biweight estimators of the sample distribution.
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.