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Home All issues Volume 707 (March 2026) A&A, 707 (2026) C4 Full HTML
Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202449758]

Table 1.

Updated spin parameters for the galaxy sample.

N ID λR N ID λR
1 17979 • 0.593 ± 0.004 56 23102 • 0.360 ± 0.003
2 18117 • 0.594 ± 0.004 57 20254 • 0.987 ± 0.001
3 16844 • 0.434 ± 0.007 58 20671 • 0.680 ± 0.024
4 11752 • 0.814 ± 0.003 59 29048 • 0.871 ± 0.012
5 7336 • 0.384 ± 0.019 60 21890 • 0.708 ± 0.021
6 20094 • 0.281 ± 0.010 61 25172 • 0.875 ± 0.005
7 14733 • 0.687 ± 0.010 62 30133 • 0.968 ± 0.007
8 17138 • 0.719 ± 0.010 63 30082 • 0.702 ± 0.011
9 17034 • 0.684 ± 0.007 64 26377 • 0.631 ± 0.008
10 15773 • 0.318 ± 0.004 65 25909 • 0.265 ± 0.024
11 17928 • 0.457 ± 0.012 66 22942 • 0.224 ± 0.006
12 16635 • 0.553 ± 0.011 67 28995 • 0.295 ± 0.027
13 19745 ↑ 0.314 ± 0.018 68 27438 • 0.775 ± 0.012
14 27563 • 0.517 ± 0.016 69 29238 ↑ 0.688 ± 0.014
15 28410 • 0.422 ± 0.011 70 29794 • 0.541 ± 0.004
16 19146 • 0.895 ± 0.003 71 27965 • 0.109 ± 0.013
17 28888 • 0.938 ± 0.005 72 28445 • 0.166 ± 0.017
18 32156 • 0.305 ± 0.007 73 29861 • 0.087 ± 0.023
19 33471 • 0.972 ± 0.018 74 2957 • 0.280 ± 0.009
20 26491 • 0.566 ± 0.020 75 3487 • 0.615 ± 0.023
21 29723 • 0.660 ± 0.020 76 4148 • 0.391 ± 0.005
22 31246 • 0.303 ± 0.019 77 1996 • 0.215 ± 0.005
23 24878 • 0.230 ± 0.004 78 902 • 0.640 ± 0.004
24 17223 • 0.752 ± 0.005 79 4596 • 0.449 ± 0.006
25 10176 • 0.395 ± 0.008 80 4638 • 0.872 ± 0.027
26 8813 • 0.363 ± 0.006 81 4077 • 0.640 ± 0.008
27 31463 • 0.546 ± 0.022 82 5116 • 0.551 ± 0.021
28 32648 ↑ 0.730 ± 0.005 83 901 • 0.398 ± 0.009
29 27247 • 0.655 ± 0.009 84 3165 • 0.802 ± 0.006
30 26402 • 0.548 ± 0.005 85 3637 • 0.745 ± 0.010
31 26138 • 0.345 ± 0.004 86 3880 • 0.851 ± 0.006
32 30082 • 0.838 ± 0.015 87 14034 • 0.737 ± 0.003
33 17361 • 0.201 ± 0.019 88 27564 • 0.852 ± 0.031
34 20356 • 0.829 ± 0.009 89 29169 • 0.746 ± 0.034
35 20898 • 0.568 ± 0.017 90 27535 • 0.419 ± 0.040
36 36482 • 0.498 ± 0.014 91 25053 • 0.201 ± 0.013
37 30918 • 0.632 ± 0.010 92 28356 • 0.625 ± 0.028
38 31801 • 0.639 ± 0.015 93 25487 • 0.267 ± 0.025
39 32778 • 0.572 ± 0.032 94 26233 ↑ 0.446 ± 0.044
40 32762 • 0.871 ± 0.016 95 25652 ↑ 0.291 ± 0.045
41 21978 • 0.450 ± 0.012 96 25884 • 0.366 ± 0.019
42 25622 • 0.739 ± 0.016 97 9612 • 0.724 ± 0.010
43 28098 • 0.870 ± 0.003 98 12252 • 0.102 ± 0.014
44 21832 • 0.318 ± 0.005 99 36313 • 0.182 ± 0.024
45 16742 • 0.990 ± 0.008 100 10195 • 0.457 ± 0.021
46 32855 • 0.675 ± 0.015 101 20331 • 0.653 ± 0.036
47 46386 • 0.824 ± 0.004 102 9754 • 0.466 ± 0.032
48 6203 • 0.516 ± 0.004 103 17534 • 0.418 ± 0.015
49 11536 • 0.778 ± 0.031 104 26322 • 0.623 ± 0.030
50 23802 • 0.826 ± 0.003 105 35579 • 0.867 ± 0.030
51 24622 • 0.061 ± 0.009 106 3181 • 0.660 ± 0.015
52 26322 • 0.712 ± 0.020
53 29845 • 0.710 ± 0.006
54 25592 • 0.230 ± 0.031
55 26639 • 0.730 ± 0.021

Notes.

Column N: galaxy index; column ID: 3D-HST galaxy unique identifier within a given field; column λR: updated galaxy stellar angular momentum measured for the selected aperture. The arrows (↑) correspond to galaxies where the seeing correction was not applied and thus indicate measured values. The filled dots (•) indicate galaxies with corrected values. Column (3) is an updated version of column (15) from Table B.1 in Muñoz López et al. (2024).

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