Table A.1.
Properties of the 19 X-ray clusters in the SSC.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|---|---|---|---|---|---|---|---|---|
| RA (J2000) | Dec (J2000) | z | r200 | M200 | Lx | a | b | ϕx |
| (deg) | (deg) | (Mpc) | (1014 M⊙) | (1044 erg s−1) | (arcmin) | (arcmin) | (deg) | |
| 200.866 | -31.722 | 0.048 | 1.154 | 1.685 | 0.288 | 23.077 | 13.485 | 99.297 |
| 194.167 | -30.357 | 0.055 | 1.638 | 4.904 | 1.542 | 23.071 | 10.082 | 90.257 |
| 202.038 | -31.482 | 0.048 | 1.895 | 7.530 | 2.987 | 20.378 | 10.598 | 114.657 |
| 194.537 | -28.514 | 0.066 | 1.053 | 1.301 | 0.196 | 19.932 | 9.228 | 110.027 |
| 193.639 | -29.149 | 0.054 | 1.722 | 5.468 | 1.824 | 19.823 | 11.397 | 162.367 |
| 193.102 | -31.267 | 0.054 | 1.529 | 3.899 | 1.076 | 15.827 | 9.373 | 98.757 |
| 203.439 | -31.667 | 0.049 | 1.600 | 4.342 | 1.264 | 15.789 | 12.028 | 87.947 |
| 195.959 | -31.410 | 0.055 | 0.895 | 0.770 | 0.085 | 15.678 | 10.128 | 42.037 |
| 196.513 | -34.399 | 0.063 | 1.042 | 1.251 | 0.184 | 14.735 | 10.393 | 43.477 |
| 203.108 | -33.074 | 0.049 | 1.400 | 3.003 | 0.711 | 12.645 | 11.380 | 170.867 |
| 194.259 | -31.345 | 0.056 | 1.106 | 1.459 | 0.232 | 12.240 | 7.531 | 57.987 |
| 199.884 | -33.480 | 0.046 | 1.066 | 1.298 | 0.191 | 11.428 | 7.626 | 59.357 |
| 202.439 | -29.538 | 0.049 | 0.946 | 0.943 | 0.116 | 10.168 | 6.812 | 48.587 |
| 203.655 | -35.271 | 0.052 | 0.796 | 0.541 | 0.049 | 9.386 | 6.156 | 47.727 |
| 202.022 | -34.065 | 0.049 | 0.937 | 0.907 | 0.110 | 8.209 | 7.028 | 3.427 |
| 202.374 | -28.311 | 0.034 | 0.639 | 0.279 | 0.017 | 12.788 | 9.123 | 92.087 |
| 198.556 | -33.824 | 0.050 | 0.909 | 0.820 | 0.094 | 8.507 | 6.139 | 166.757 |
| 200.405 | -35.823 | 0.050 | 0.866 | 0.706 | 0.074 | 8.491 | 7.671 | 63.977 |
| 201.756 | -27.168 | 0.036 | 1.375 | 2.794 | 0.625 | 18.500 | 14.155 | 29.658 |
Notes. Columns are: (1) and (2): right ascension and declination of the cluster center, defined by the X-ray peak from the eROSITA detections (purple circles in Fig. 1); (3): redshift of the cluster; (4) and (5): radius and corresponding mass enclosing a mean density of 200 times the critical mass density of the Universe at the cluster redshift; (6): X-ray luminosity of the cluster; (7) and (8): major and minor axes of the ellipse fitted to the X-ray emission of the cluster; (9): inclination angle of the major axis (see Sect. 4.3).
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