Table A.3.
Positions, redshifts, magnitudes, cluster properties, and references for G-DDRGs hosted by BCGs.
| SrNo | RA | Dec | Cluster Name | z | rmag | r500 | RL∗500 | N500 | M500 | Reference |
|---|---|---|---|---|---|---|---|---|---|---|
| (HMS) | (DMS) | (Mpc) | (1014 M⊙) | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| 1 | 00 03 45.91 | +31 39 24.24 | J000345.9+313924 | 0.5548 | 19.9 | 0.66 | 30.91 | 6 | 1.74 | (Wen & Han 2015) |
| 2 | 08 15 38.42 | +49 56 00.30 | J081538.4+495601 | 0.5993 | 19.5 | 0.76 | 39.82 | 11 | 2.28 | " |
| 3 | 08 31 10.57 | +44 31 54.22 | J083110.6+443154 | 0.3705 | 18.8 | 0.65 | 20.91 | 10 | 1.14 | " |
| 4 | 08 32 01.85 | +39 55 45.99 | J083201.8+395546 | 0.3216 | 18.9 | 0.73 | 25.56 | 11 | 1.41 | " |
| 5 | 12 19 00.76 | +50 52 54.41 | J121900.8+505255 | 0.3851 | 18.3 | 0.69 | 26.54 | 12 | 1.47 | " |
| 6 | 13 14 58.77 | +38 27 08.7 | J131458.8+382709 | 0.6430 | 21.0 | 0.53 | 20.95 | 7 | 1.14 | " |
| 7 | 13 16 06.72 | +27 19 27.9 | J131606.7+271928 | 0.2497 | 17.5 | 0.73 | 23.63 | 15 | 1.30 | " |
| 8 | 13 21 10.07 | +36 26 27.43 | J132110.1+362627 | 0.2665 | 17.4 | 0.85 | 41.68 | 22 | 2.40 | " |
| 9 | 14 20 14.04 | +37 34 06.52 | J142014.0+373407 | 0.5813 | 20.6 | 0.59 | 19.84 | 7 | 1.07 | " |
| 10 | 14 53 02.86 | +33 08 42.40 | J145302.9+330842 | 0.2481 | 17.7 | 0.71 | 18.68 | 10 | 1.01 | " |
| 11 | 16 08 10.80 | +32 54 18.9 | J160810.9+325419 | 0.3038 | 17.6 | 0.72 | 30.14 | 12 | 1.69 | " |
| 12 | 23 14 19.63 | +19 23 25.93 | J231419.6+192326 | 0.0924 | 15.2 | 0.65 | 16.4 | 8 | 0.88 | " |
| 13 | 01 41 49.60 | +27 40 45.7 | J014149.6+274046 | 0.2702† | 17.1 | - | - | - | 1.38* | (Wen et al. 2018) |
| 14 | 15 37 23.92 | +42 59 56.8 | J153723.8+425959 | 1.4015† | 25.1 | 0.52 | - | 14 | 1.36 | (Wen & Han 2021) |
| 15 | 16 34 15.05 | +49 28 42.8 | 061323 | 0.517 | 9.7 | - | - | - | - | (Szabo et al. 2011) |
Notes. The Right Ascension (RA) and Declination (Dec) of G-DDRGs hosted by the brightest cluster galaxies (BCGs) are listed in columns (2) and (3), respectively. Column (4) provides the cluster names. Column (5) lists redshifts, which are predominantly spectroscopic, except those marked with †, which are photometric. Column (6) lists the r-band magnitude (rmag) of the BCG-DDRGs. The radius r500 (column 7) is the radius within which the mean density is 500 times the critical density of the Universe, and M500 (column 10) is the mass within this radius. Column (8) shows RL∗500, the cluster richness parameter, and column (9) lists N500, the number of galaxies within r500. References for the data are listed in column (11). For galaxy clusters from Wen & Han (2015), M500 is computed using Eq. 17 from their paper. For the cluster J014149.6+274046 (marked with ), M500 is from Gao et al. (2020).
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