Table A.1
Main disc properties from the light distribution in the g, r, and i SDSS bands for the RaDES galaxies.
Galaxy | SB type | hin (kpc) | hout (kpc) | Rbreak (kpc) | ||||||
g | r | i | g | r | i | g | r | i | ||
|
||||||||||
Apollo | II | 2.68 | 2.34 | 2.19 | 1.24 | 1.39 | 1.44 | 5.14 | 4.96 | 4.94 |
Artemis | III | 0.60 | 0.79 | 0.78 | 5.56 | 5.87 | 5.97 | 4.27 | 5.30 | 5.30 |
Atlas | II | 5.08 | 4.39 | 3.43 | 2.31 | 2.47 | 2.53 | 7.63 | 7.43 | 7.91 |
Ben | II | 5.88 | 5.28 | 5.03 | 3.15 | 3.36 | 3.36 | 12.33 | 12.18 | 12.42 |
Castor | II | 10.06 | 5.70 | 5.32 | 0.95 | 0.96 | 0.96 | 5.37 | 5.35 | 5.32 |
Daphne | III | 1.23 | 1.26 | 1.27 | 3.76 | 3.84 | 3.81 | 10.05 | 10.08 | 10.08 |
Eos | III | 2.96 | 2.95 | 2.91 | 8.38 | 8.55 | 8.37 | 19.32 | 18.32 | 17.84 |
Helios | III | 1.92 | 1.93 | 2.01 | 7.73 | 7.76 | 7.82 | 11.54 | 11.49 | 11.74 |
Hyperion | II | 4.54 | 4.31 | 4.24 | 2.51 | 2.77 | 2.78 | 14.94 | 14.97 | 15.15 |
Krios | III | 2.63 | 2.62 | 2.63 | 8.51 | 8.45 | 8.33 | 16.82 | 16.11 | 15.85 |
Leia | III | 3.65 | 3.81 | 3.90 | 7.37 | 7.48 | 7.58 | 20.95 | 21.21 | 21.62 |
Leto | III | 0.95 | 0.99 | 1.00 | 4.11 | 4.07 | 3.99 | 6.65 | 6.59 | 6.51 |
Luke | I | 5.84 | 5.78 | 5.77 | − | − | − | − | − | − |
Oceanus | II | 8.19 | 8.08 | 7.93 | 5.17 | 4.18 | 4.39 | 21.19 | 23.17 | 23.21 |
Pollux | III | 1.20 | 1.25 | 1.22 | 4.33 | 4.03 | 3.93 | 8.80 | 8.61 | 8.41 |
Selene | II | 5.74 | 5.68 | 5.36 | 1.73 | 2.01 | 1.98 | 12.75 | 11.98 | 12.13 |
Tethys | II | 5.23 | 4.43 | 4.20 | 1.97 | 2.12 | 2.16 | 9.92 | 9.82 | 9.85 |
Tyndareus | III | 1.34 | 1.33 | 1.33 | 3.67 | 3.39 | 3.22 | 7.69 | 7.12 | 6.89 |
Zeus | I | 0.90 | 0.92 | 0.92 | − | − | − | − | − | − |
Notes. First column: Galaxy name. Second column: surface brightness type according to the Pohlen & Trujillo (2006) classification. Third to fifth columns: inner disc scale length in kpc (g, r, and i SDSS bands). Sixth to eighth columns: outer disc scale length in kpc (g, r and i SDSS bands). Ninth to eleventh columns: break radius in kpc (g, r and i SDSS bands).
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