Table 1.
Basic information for the galaxies used in this work.
| Galaxy | Type | Distance | Redshift | Morph. type | Jet | Prop. ID | Reference | Sample |
|---|---|---|---|---|---|---|---|---|
| (Mpc) | ||||||||
| NGC 1052 | LINER-1.9 | 19 | 0.0050 | E4 | Y | 2016 | [1] | Train |
| NGC 3081* | Sy-2 | 34 | 0.0082 | (R)SAB0/a(r) | Y | 1670 | [2] | Train |
| NGC 3227* | Sy-1.5 | 15 | 0.0038 | SAB(s)a pec | Y | 3535 | – | Test |
| NGC 3256-N | Starburst | 40 | 0.0094 | Merger pec | N | 1328 | [3,4,5] | Train |
| NGC 4051* | NLS1 | 16.6 | 0.0023 | SAB(rs)bc | N | 3535 | – | Test |
| NGC 4594 | LINER-2 | 10 | 0.0034 | SA(s)a | Y | 2016 | [1] | Train |
| NGC 5506* | Sy-2 | 26 | 0.0061 | Sa pec | Y | 1670 | [2] | Train |
| NGC 5728* | Sy-2 | 39 | 0.0092 | SAB(r)a? | Y | 1670 | [6,7] | Train |
| NGC 7172* | Sy-2 | 37 | 0.0087 | Sa pec | N | 1670 | [7,8] | Train |
| NGC 7319 | Sy-2 | 98 | 0.0225 | SB(s)bc pec | Y | 2732 | [9] | Train |
| NGC 7469 | Sy-1.5 | 71 | 0.0163 | (R’)SAB(rs)a | N | 1328 | [10,11] | Train |
| NGC 7582* | Sy-2 | 22.7 | 0.0053 | (R’)SB(s)ab | - | 3535 | [12] | Test |
| IC 5063 | Sy-2 | 48.6 | 0.0114 | SA0+(s)? | Y | 2004 | [13] | Train |
| M 83 | Starburst | 4.6 | 0.0017 | SAB(s)c | N | 2219 | [14,15] | Train |
| Centaurus A | Sy-2 | 3.5 | 0.0018 | S0 pec | Y | 1269 | [16] | Train |
Notes. * indicates the galaxies observed within the GATOS collaboration (see Sect. 2). In Type: ‘Sy’ stands for Seyfert, and ‘NLS1’ for Narrow Line Seyfert-1. The redshift and morphological types have been obtained from NASA/IPAC Extragalactic Database (NED). In Jet: ‘Y’ stands for Yes, and ‘N’ stands for No; for NGC 7582 it is unclear (Veenema et al. 2025). The cited works refer exclusively to analyses using JWST data, used to label the clusters (see Sect. 2.3): [1] Goold et al. (2024), [2] Delaney et al. (2025), [3] Bohn et al. (2024), [4] Rigopoulou et al. (2024), [5] García-Bernete et al. (2025), [6] Davies et al. (2024), [7] García-Bernete et al. (2024c), [8] Hermosa Muñoz et al. (2024a), [9] Pereira-Santaella et al. (2022), [10] Armus et al. (2023), [11] Feuillet et al. (2025), [12] Veenema et al. (2025), [13] Dasyra et al. (2024), [14] Hernandez et al. (2023), [15] Hernandez et al. (2025), [16] Alonso Herrero et al. (2025). The last column indicates if the target has been used for the training or testing samples within the analysis.
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