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Table A.1

The sample of spatially resolved galaxies in the MUSE-HDFS.

ID z i PAmor R d PAkin V max σ Int. log (Mstar) log (SFR)
(°) (°) (/kpc) (°) (km s-1) (km s-1) (M) (M yr-1)
[1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11]

1 0.1723 75 31.3 ± 0.1 0.46 / 1.34 ± 0.01 33 ± 2 74 ± 4 30 ± 3 0 8.78 ± 0.42 − 1.01 ± 0.67
3 0.5637 16 − 18.8 ± 3.0 0.66 / 4.28 ± 0.04 64 ± 2 103 ± 20 34 ± 1 0 9.66 ± 0.14 0.24 ± 0.37
4 0.5638 75 35.8 ± 0.1 0.62 / 4.01 ± 0.03 34 ± 1 204 ± 20 48 ± 3 0 9.86 ± 0.17 0.54 ± 0.35
5 0.5798 68 6.9 ± 0.2 0.25 / 1.67 ± 0.02 37 ± 6 47 ± 16 54 ± 3 0 9.82 ± 0.17 0.59 ± 0.38
6 0.4230 29 45.0 ± 2.0 0.46 / 2.54 ± 0.03 9 ± 7 80 ± 4 29 ± 3 1 9.23 ± 0.10 − 0.61 ± 0.50
7 0.4637 41 43.0 ± 0.7 0.44 / 2.55 ± 0.03 50 ± 3 76 ± 2 27 ± 15 1 9.31 ± 0.12 − 0.51 ± 0.54
8 0.5772 61 − 29.4 ± 0.4 0.18 / 1.20 ± 0.01 − 20 ± 2 124 ± 20 84 ± 12 1 9.88 ± 0.23 1.39 ± 0.58
9 0.5638 61 − 34.8 ± 0.4 0.25 / 1.60 ± 0.02 − 37 ± 2 125 ± 3 54 ± 3 0 9.31 ± 0.20 0.80 ± 0.41
10 1.2840 26 39.9 ± 4.1 0.24 / 2.05 ± 0.06 107 ± 15 98 ± 14 116 ± 3 2 10.77 ± 0.11 0.30 ± 0.89
11 0.5779 62 27.3 ± 0.5 0.10 / 0.67 ± 0.01 29 ± 3 61 ± 12 49 ± 1 0 9.22 ± 0.18 0.08 ± 0.49
12 0.6701 37 − 144.0 ± 4.9 0.04 / 0.29 ± 0.01 − 145 ± 30 48 ± 12 59 ± 1 2 9.02 ± 0.27 0.82 ± 0.67
13 1.2900 33 − 45.9 ± 1.9 0.15 / 1.25 ± 0.02 − 13 ± 2 24 ± 4 48 ± 1 0 9.89 ± 0.11 1.89 ± 0.18
16 0.4647 20 − 40.0 ± 7.6 0.40 / 2.35 ± 0.06 − 53 ± 10 91 ± 3 34 ± 3 0 8.74 ± 0.21 − 0.65 ± 0.55
17 0.5810 45 77.3 ± 1.2 0.26 / 1.73 ± 0.04 95 ± 15 87 ± 30 41 ± 6 0 9.06 ± 0.17 − 0.13 ± 0.84
20 0.4275 73 − 38.8 ± 0.5 0.49 / 2.77 ± 0.10 − 121 ± 4 41 ± 15 21 ± 3 0 8.71 ± 0.06 − 1.16 ± 0.50
23 0.5641 24 78.3 ± 4.9 0.51 / 3.38 ± 0.09 14 ± 8 32 ± 6 31 ± 3 0 8.72 ± 0.27 − 0.19 ± 0.70
24 0.9723 14 − 1.2 ± 13.8 0.18 / 1.44 ± 0.05 − 68 ± 3 164 ± 21 45 ± 3 0 9.61 ± 0.24 0.77 ± 0.73
26 0.2249 70 15.0 ± 0.4 0.46 / 1.66 ± 0.05 14 ± 4 75 ± 9 16 ± 3 0 7.95 ± 0.35 − 1.87 ± 0.63
27 1.2853 71 − 9.4 ± 0.5 0.48 / 4.00 ± 0.05 5 ± 2 168 ± 15 99 ± 6 1,2 10.32 ± 0.19 1.06 ± 0.95
28 0.3179 32 84.9 ± 3.0 0.21 / 0.99 ± 0.04 75 ± 22 47 ± 10 29 ± 3 0 7.99 ± 0.14 − 1.24 ± 0.38
32 0.5644 68 122.0 ± 0.5 0.28 / 1.83 ± 0.06 112 ± 8 70 ± 7 50 ± 3 0 8.57 ± 0.17 − 1.07 ± 0.39
35 1.2806 41 44.3 ± 2.5 0.17 / 1.40 ± 0.06 34 ± 7 214 ± 30 87 ± 12 0 10.12 ± 0.26 1.37 ± 0.96
37 1.0978 72 6.1 ± 0.7 0.12 / 0.98 ± 0.02 46 ± 20 21 ± 7 66 ± 3 0 9.12 ± 0.17 0.89 ± 0.43
38 1.0217 57 − 29.0 ± 1.2 0.23 / 1.82 ± 0.08 − 23 ± 6 98 ± 10 45 ± 6 0 8.86 ± 0.14 0.17 ± 0.42
49 0.9991 68 − 68.8 ± 1.0 0.19 / 1.52 ± 0.08 − 69 ± 6 86 ± 20 51 ± 6 1 8.83 ± 0.21 − 0.02 ± 0.72
68 0.9715 78 26.3 ± 0.9 0.16 / 1.29 ± 0.06 9 ± 7 70 ± 13 39 ± 6 0 8.29 ± 0.24 − 0.51 ± 0.53
72 0.8391 74 − 90.0 ± 1.0 0.16 / 1.22 ± 0.07 − 87 ± 8 135 ± 9 24 ± 21 0 8.68 ± 0.25 − 0.62 ± 0.42
88 1.3600 77 8.8 ± 2.0 0.21 / 1.76 ± 0.22 − 64 ± 12 51 ± 9 34 ± 12 2 8.71 ± 0.14 − 0.45 ± 0.37

Notes. Column (1): identification number according to Bacon et al. (2015); Col. (2): spectroscopic redshift from MUSE according to Bacon et al. (2015); Cols. (3), (4), (5): disk inclination (with typical uncertainties of ±5°), position angle of the disk major axis, and disk scale length (both in arcsec and kpc, but uncertainties are given in kpc only) derived from Galfit modeling on HST F814W images (see Sect. 3); Cols. (6), (7), (8): position angle of the disk major axis, maximum rotation velocity, and velocity dispersion derived from kinematic modeling of MUSE data cubes (see Sect. 4); Col. (9): flag indicating the level of gravitational interactions: 0 = isolated, 1 = minor pair/interaction, 2 = major pair/interaction or clear merger remnant (see Sect. 5.1.3); Cols. (10, 11): stellar mass and star formation rate derived from SED fitting on visible+NIR photometry (see Sect. 2.2.2).

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