Table 1
Studied clusters from the CLASH sample.
| Cluster | RA | Dec | z | ϵ F814W | ϵ F606W | ϵIc/ϵIp | ϵ V | r max | r 200 | M 200 |
| ″ | ″ | ″/″ | ″ |
|
|
|
||||
|
|
||||||||||
| Abell 209 | 01:31:52.57 | –13:36:38.8 | 0.206 | 0.06 | 0.17 | –/0.66 | 0.73 | 382 | 2268 | 15.40 ± 3.42 |
| Abell 383 | 02:48:03.36 | –03:31:44.7 | 0.187 | 0.09 | 0.06 | 0.86/0.57 | 0.63 | 379 | 1829 | 7.98 ± 2.66 |
| MACSJ0329-02 | 03:29:41.68 | –02:11:47.7 | 0.450 | 0.25 | 0.15 | 0.90/– | 0.55 | 643 | 1742 | 8.65 ± 1.97 |
| MACSJ0429-02 | 04:29:36.10 | –02:53:08.0 | 0.399 | 0.14 | 0.09 | 1.28/– | 1.14 | 610 | 1840 | 9.76 ± 3.50 |
| MACSJ0717+37 | 07:17:31.65 | +37:45:18.5 | 0.548 | 0.14 | 0.15 | –/0.96 | 0.69 | 807 | 2358 | 26.77 ± 5.36 |
| MACSJ0744+39 | 07:44:52.80 | +39:27:24.4 | 0.686 | 0.08 | 0.06 | 0.82/0.87 | 0.71 | 859 | 2030 | 18.03 ± 4.96 |
| Abell 611 | 08:00:56.83 | +36:03:24.1 | 0.288 | 0.10 | 0.08 | 0.76/0.81 | 0.85 | 389 | 2223 | 15.76 ± 4.49 |
| MACSJ1115+01 | 11:15:52.05 | +01:29:56.6 | 0.352 | 0.09 | 0.06 | 0.96/– | 0.95 | 562 | 2250 | 16.66 ± 3.85 |
| MACSJ1206-08 | 12:06:12.28 | –08:48:02.4 | 0.440 | 0.05 | 0.16 | 0.71/– | 0.95 | 643 | 2220 | 18.17 ± 4.23 |
| RXJ1347-1145 | 13:47:30.59 | –11:45:10.1 | 0.451 | 0.11 | 0.09 | 1.14/– | 0.75 | 677 | 2720 | 34.25 ± 8.78 |
| MACSJ1423+24 | 14:23:47.76 | +24:04:40.5 | 0.545 | 0.08 | 0.13 | 0.86/– | 0.96 | 751 | – | – |
| RXJ1532.9+3021 | 15:32:53.78 | +30:20:58.7 | 0.345 | 0.08 | 0.14 | 1.11/– | 0.71 | 553 | 1508 | 5.98 ± 2.32 |
| MACSJ1720+35 | 17:20:16.95 | +35:36:23.6 | 0.391 | 0.09 | 0.12 | 1.04/– | 0.82 | 559 | 2091 | 14.50 ± 4.30 |
| MACSJ2129-07 | 21:29:26.06 | –07:41:28.8 | 0.570 | 0.05 | 0.09 | 0.55/– | 0.72 | 800 | – | – |
| RXJ2129+0005 | 21:29:39.94 | +00:05:18.8 | 0.234 | 0.11 | 0.06 | –/1.00 | 0.71 | 421 | 1680 | 6.14 ± 1.79 |
| MS 2137.3-2353 | 21:40:15.18 | –23:39:40.7 | 0.313 | 0.12 | 0.09 | 1.20/– | 1.15 | 516 | 2160 | 13.56 ± 5.27 |
Notes. The different columns are: #1: cluster ID, #2: right ascension, #3: declination, #4: redshift, #5: FWHM of the HST/ACS F814W image PSF in arcseconds, #6: FWHM of the HST/ACS F606W image PSF in arcseconds, #7: FWHM of the Subaru/Suprime-Cam Ic and Ip image PSFs in arcseconds, #8: FWHM of the Subaru/Suprime-Cam V image PSF in arcseconds, #9: maximum cluster radius that fits in the HST field-of-view, #10: radius at which the cluster mass density is 200 times the critical mass density, as computed from lensing (Umetsu et al. 2016), #11: cluster total mass, as computed from lensing (Umetsu et al. 2016).
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.