Table 8.
Photometric properties and stellar masses of the host galaxies.
| Object | RA(J2000) | Dec(J2000) | g | i | W1 | W2 | W3 | log(M⋆/M⊙) |
|---|---|---|---|---|---|---|---|---|
| A 3528 N | ||||||||
| J1254-2900 | 12 54 22.24 | −29 00 46.73 | 14.09 ± 0.01 | 12.85 ± 0.01 | 10.07 ± 0.01 | 10.09 ± 0.01 | 9.65 ± 0.05 | 11.75 ± 0.08 |
| J1254-2901a | 12 54 23.22 | −29 01 03.05 | 15.89 ± 0.01 | 14.76 ± 0.01 | 12.46 ± 0.02 | 12.45 ± 0.03 | 11.60 ± 0.19 | 10.84 ± 0.10 |
| J1254-2901b | 12 54 40.75 | −29 01 48.55 | 16.23 ± 0.01 | 15.12 ± 0.01 | 12.63 ± 0.01 | 12.66 ± 0.02 | 12.40 ± 0.30 | 10.71 ± 0.09 |
| J1254-2904 | 12 54 20.41 | −29 04 08.67 | 15.87 ± 0.01 | 14.76 ± 0.01 | 12.39 ± 0.01 | 12.35 ± 0.01 | 12.15 ± 0.20 | 10.85 ± 0.10 |
| A 3528 S | ||||||||
| J1254-2913 | 12 54 41.10 | −29 13 39.58 | 13.46 ± 0.01 | 12.33 ± 0.01 | 9.81 ± 0.01 | 9.78 ± 0.01 | 9.44 ± 0.07 | 11.89 ± 0.09 |
| J1254-2916 | 12 54 52.42 | −29 16 16.80 | 14.88 ± 0.01 | 13.72 ± 0.01 | 11.22 ± 0.01 | 11.25 ± 0.01 | 10.84 ± 0.13 | 11.20 ± 0.09 |
| A 3532 | ||||||||
| J1257-3021 | 12 57 21.94 | −30 21 49.00 | 14.34 ± 0.01 | 13.27 ± 0.01 | 10.87 ± 0.01 | 10.87 ± 0.01 | 10.54 ± 0.11 | 11.43 ± 0.10 |
| A 3556 | ||||||||
| J1324-3138 | 13 23 57.61 | −31 38 44.82 | 14.69 ± 0.01 | 13.46 ± 0.01 | 10.91 ± 0.01 | 10.90 ± 0.01 | 10.49 ± 0.09 | 11.38 ± 0.08 |
| J1324-3140 | 13 24 06.73 | −31 40 11.56 | 13.89 ± 0.01 | 12.74 ± 0.01 | 10.01 ± 0.01 | 10.00 ± 0.01 | 9.62 ± 0.06 | 11.66 ± 0.07 |
| A 3558 | ||||||||
| J1327-3129b | 13 27 56.86 | −31 29 45.32 | 13.29 ± 0.01 | 12.17 ± 0.01 | 9.39 ± 0.01 | 9.49 ± 0.01 | 9.13 ± 0.11 | 11.85 ± 0.08 |
| A 3562 | ||||||||
| J1333-3140 | 13 33 34.73 | −31 40 20.34 | 14.13 ± 0.01 | 12.97 ± 0.01 | 10.77 ± 0.01 | 10.81 ± 0.01 | 10.34 ± 0.07 | 11.46 ± 0.09 |
| J1333-3141 | 13 33 31.63 | −31 40 58.33 | 16.30 ± 0.01 | 15.09 ± 0.01 | 12.63 ± 0.02 | 12.80 ± 0.05 | 12.57 ± 0.39 | 10.70 ± 0.08 |
Notes. Columns 2 and 3: galaxy coordinates corresponding to the photometric centre in g band. Columns 4 and 5: optical (gi) magnitudes from VST given in AB photometric system (see Merluzzi et al. 2015; Mercurio et al. 2015). Columns 6–8: mid-infrared (mid-IR) magnitudes from WISE channels W1, W2 and W3 derived as explained in the text. All magnitudes are corrected for the Galactic extinction following Schlafly & Finkbeiner (2011). Column 9: logarithm of stellar mass in units of solar mass.
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