Table B.1.
Results of the MISTRAL observing runs at OHP.
| X-CLASS | R.A. | DEC. | g | r | zphot | z | Conf | Comments |
|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | |||||||
| xclass0297_G1 | 68.5873 | -8.4908 | 18.27 | 16.73 | 0.247 | 0.2392 | 3 | BCG |
| xclass0297_G2 | 68.5703 | -8.5124 | 19.10 | 17.52 | 0.250 | 0.2397 | 3 | |
| xclass0297_G3 | 68.5564 | -8.5095 | 20.02 | 18.54 | 0.232 | 0.2404 | 3 | |
| xclass0297_G4 | 68.5681 | -8.5067 | 19.86 | 18.53 | 0.224 | 0.2406 | 2 | |
| xclass0473_G1 | 7.4357 | 4.8736 | 18.06 | 16.78 | 0.205 | 0.2069 | 3 | |
| xclass0473_G2 | 7.4408 | 4.8529 | 18.80 | 17.53 | 0.209 | 0.2050 | 2 | |
| ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. For each X-CLASS cluster (1), the galaxies are listed with their coordinates (2,3). The magnitudes in g and r are derived from the DESI Legacy Survey when available (4,5), as is the photometric redshift (6). The confidence level (7) ranges from 1 (tentative, no more than 2 absorption lines clearly identified) to 3 (good, based on a minimum of 3 strong absorption lines). Some comments are added, particularly the identification of the BCG when possible (8). Only part of the table is presented here. The full table is available at the CDS.
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