Table A.1.
Galaxy parameters of all galaxies in our sample.
| N° | Morphological | α | δ | i | PA | D | Rmax | log10M★ | log10j★ |
|---|---|---|---|---|---|---|---|---|---|
| UGC | type | [J2000] | [J2000] | [°] | [°] | [Mpc] | [kpc] | [M⊙] | [kpc km s−1] |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| 1913 | SAB(s)d | 02h27m16s.7 | 33°34′44″ | 48 ± 9 | 108 ± 3 | 9.30 | 23.91* | 10.48 | 2.93 ![]() |
| 2800 | Im | 03h40m02s.4 | 71° 24′22″ | 52 ± 13 | 11 ± 4 | 20.60 | 12.05 | 9.91 | 2.82 ![]() |
| 2855 | SABc | 03h48m20s.6 | 70° 07′58″ | 68 ± 2 | 100 ± 2 | 17.50 | 15.33* | 10.58 | 3.18 ![]() |
| 3574 | SA(s)cd | 06h53m10s.3 | 57° 10′41″ | 19 ± 10 | 99 ± 3 | 21.80 | 20.11* | 10.06 | 3.18 ![]() |
| 3734 | SA(rs)c | 07h12m28s.7 | 47° 10′02″ | 43 ± 7 | 139 ± 2 | 15.90 | 11.23 | 10.05 | 2.63 ![]() |
| 4284 | SA(s)cd | 08h14m40s.1 | 49° 03′43″ | 59 ± 9 | 176 ± 3 | 9.80 | 15.06* | 10.05 | 2.69 ![]() |
| 4325 | SA(s)m | 08h19m20s.5 | 50° 00′36″ | 63 ± 14 | 57 ± 3 | 10.90 | 8.49* | 9.17 | 2.28 ![]() |
| 4499 | SABdm | 08h37m41s.3 | 51° 39′12″ | 50 ± 14 | 141 ± 4 | 12.20 | 6.83 | 8.93 | 2.20 ![]() |
| 5251 | SBbc | 09h48m35s.8 | 33° 25′18″ | 73 ± 6 | 80 ± 3 | 21.50 | 35.88* | 10.57 | 3.02 ![]() |
| 5253 | (R′)SA(rs)ab | 09h50m21s.9 | 72° 16′46″ | 40 ± 4 | 176 ± 2 | 21.10 | 23.59 | 10.92 | 3.12 ![]() |
| 5414 | IAB(s)m | 10h03m57s.3 | 40° 45′26″ | 71 ± 13 | 39 ± 4 | 10.00 | 7.30* | 9.28 | 2.30 ![]() |
| 6537 | SAB(r)c | 11h33m21s.2 | 47° 01′47″ | 47 ± 5 | 20 ± 2 | 14.30 | 18.07 | 10.51 | 2.97 ![]() |
| 6778 | SAB(rs)c | 11h48m38s.0 | 48° 42′39″ | 49 ± 4 | 163 ± 2 | 15.50 | 18.08* | 10.19 | 2.90 ![]() |
| 7323 | SAB(s)dm | 12h17m30s.2 | 45° 37′11″ | 51 ± 11 | 19 ± 21Mor | 8.10 | 16.77* | 9.92 | 2.61 ![]() |
| 7766 | SAB(rs)cd | 12h35m57s.7 | 27° 57′35″ | 69 ± 3 | 143 ± 2 | 13.00 | 37.12* | 10.72 | 3.01 ![]() |
| 8334 | SA(rs)bc | 13h15m49s.3 | 42° 01′45″ | 66 ± 1 | 100 ± 1 | 9.80 | 28.78 | 11.33 | 3.11 ![]() |
| 8490 | SA(s)m | 13h29m36s.6 | 58° 25′13″ | 40 ± 15 | 167 ± 3 | 4.70 | 5.66 | 9.09 | 2.17 ![]() |
| 9179 | SAB(s)d | 14h19m48s.2 | 56° 43′46″ | 36 ± 14 | 49 ± 4 | 5.70 | 8.57 | 9.42 | 2.49 ![]() |
| 9649 | SB(rs)b | 14h57m45s.4 | 71° 40′55″ | 54 ± 6 | 55 ± 3 | 7.70 | 5.44 | 9.30 | 2.20 ![]() |
| 9858 | SABbc | 15h26m41s.6 | 40° 33′53″ | 75 ± 2 | 70 ± 2 | 38.20 | 37.14* | 10.75 | 2.22 ![]() |
| 9969 | SAB(r)b | 15h39m36s.9 | 59° 19′55″ | 61 ± 1 | 16 ± 1 | 36.00 | 32.40* | 11.21 | 3.50 ![]() |
| 10075 | SA(s)cd | 15h51m25s.3 | 62° 18′36″ | 62 ± 2 | 30 ± 1 | 14.70 | 19.66 | 10.56 | 2.87 ![]() |
| 10359 | SB(s)cd pec | 16h20m57s.9 | 65° 23′26″ | 44 ± 12 | 104 ± 3 | 16.00 | 17.11 | 9.63 | 2.79 ![]() |
| 10470 | (R)SB(rs)bc | 16h32m39s.3 | 78° 11′53″ | 34 ± 9 | 155 ± 26Mor | 21.20 | 17.54 | 10.04 | 2.82 ![]() |
| 11012 | SA(s)cd | 17h49m26s.3 | 70° 08′40″ | 72 ± 2 | 123 ± 7Mor | 5.30 | 7.97 | 10.22 | 2.29 ![]() |
| 11597 | SAB(rs)cd | 20h34m52s.4 | 60° 09′14″ | 40 ± 10 | 61 ± 3 | 5.90 | 20.08 | 10.48 | 3.04 ![]() |
| 11670 | SA(r)0/a | 21h03m33s.5 | 29° 53′52″ | 65 ± 2 | 153 ± 2 | 12.80 | 18.65* | 10.65 | 2.93 ![]() |
| 11852 | SBa | 21h55m59s.3 | 27° 53′55″ | 47 ± 7 | 9 ± 3 | 80.10 | 21.59 | 10.49 | 3.10 ![]() |
| 11914 | (R)SA(r)ab | 22h07m52s.4 | 31° 21′34″ | 33 ± 4 | 86 ± 2 | 15.00 | 33.06* | 10.76 | 3.35 ![]() |
| 12754 | SB(s)cd | 23h43m54s.2 | 26° 04′35″ | 53 ± 5 | 162 ± 2 | 8.90 | 10.80* | 9.37 | 2.61 ![]() |
Notes. (1) Name of the galaxy in the UGC catalogue, (2) morphological type extracted from NASA/IPAC Extragalactic Database (NED), (3) and (4) right ascension and declination of the photometric centre determined as the brightest pixel of the WISE W1 band image, (5) and (6) kinematic inclination and PA taken from the velocity field analysis carried out in Epinat et al. (2008a). The Mor superindex indicates that the photometric PA taken from HyperLeda replaces the kinematic PA to compute the stellar sAMSD. (7) distance to the galaxy taken from Epinat et al. (2008a). (8) maximum radius determined by the criterion presented in Eq. (9). The * superindex flags the galaxies for which the RC was extrapolated to reach Rmax, (9) stellar mass calculated following Eq. (8), and (10) total stellar sAM computed using Eq. (6).
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