Table A.1
Redshifts used for the deep study of the central area of RX J1119.7+2126.
RA | Dec | z | Nature | Source |
|
||||
169.86131 | 21.43701 | 0.362 | galaxy | TNG |
169.87387 | 21.44891 | 0.261/0.261 | galaxy | TNG/TNG |
169.88421 | 21.46373 | 0.2595 | galaxy | TNG |
169.88604 | 21.38743 | 1.422 | active | TNG |
169.88833 | 21.46607 | 0.28100 | galaxy | NED |
169.89172 | 21.40683 | 0.3379 | galaxy | TNG |
169.90656 | 21.43067 | 0. | star | TNG |
169.90868 | 21.44097 | 2.97 | active | TNG |
169.90989 | 21.39666 | 0.3065 | galaxy | TNG |
169.91870 | 21.43216 | 0.2755 | galaxy | TNG |
169.92206 | 21.45909 | 0.361 | galaxy | TNG |
169.92260 | 21.46334 | 0. | star | TNG |
169.92296 | 21.42640 | 0.4345 | galaxy | TNG |
169.92513 | 21.43622 | 0.06134 * | galaxy | NED |
169.92680 | 21.45457 | 0.392 | galaxy | TNG |
169.93159 | 21.44756 | 0.06055/0.0603/0.0603 * | galaxy | NED/TNG/TNG |
169.93549 | 21.46902 | 0.306 | galaxy | TNG |
169.93623 | 21.53648 | 0.14058 | galaxy | NED |
169.93633 | 21.51504 | 0.2275 | galaxy | TNG |
169.93824 | 21.51931 | 0.22931/0.228 | galaxy | NED/TNG |
169.94032 | 21.50432 | 0.153 | galaxy | TNG |
169.94221 | 21.42251 | 0.3975 | galaxy | TNG |
169.94622 | 21.48221 | 0.21409/0.2125/0.213 | galaxy | NED/TNG/TNG |
169.96226 | 21.51082 | 0.0565 *? | galaxy | TNG |
169.96593 | 21.51904 | 0.405 | galaxy | TNG |
169.96682 | 21.50062 | 0.08247/0.082 | galaxy | NED/TNG |
169.96832 | 21.41800 | 0.1652 | galaxy | TNG |
169.98881 | 21.44085 | 0.059 * | galaxy | TNG |
169.99585 | 21.53157 | 0.05976 * | galaxy | NED |
169.99891 | 21.45859 | 0.299 | galaxy | TNG |
170.00296 | 21.44578 | 0.2095/0.2104 | galaxy | TNG/TNG |
170.00600 | 21.43058 | 0.429 | galaxy | TNG |
Notes. Columns 1 and 2: J2000.0 coordinates of the object (in decimal degrees); Col. 3: redshift (the number of significant digits depends on the spectrum quality, galaxies marked with a * are potential group members); Col. 4: nature of the object (galaxy, active object, star); Col. 5: source (TNG, NED). The typical uncertainty on non-literature redshifts is 0.001. Given the low signal-to-noise ratio of the TNG spectra, we chose to use mainly literature redshifts when available. We note that the group velocity dispersion was computed without the z = 0.0565 galaxy.
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