Table 1.
General information on MAGNUM galaxies.
| Name | AGN type | Dl [Mpc]1 | BH mass [M⊙]2 | Morphology/type | Interaction3 | 1″ [pc] |
|---|---|---|---|---|---|---|
| Centaurus A | Seyfert 2 | 3.82 | 6.5 × 107a | Lenticular/early type | yes j | 18.5 |
| Circinus | Seyfert 2 | 4.2 | ≈106.23b | spiral | no | 20.4 |
| IC 5063 | Seyfert 2 | 45.3 | 5.5 × 107c | early type | yes l | 219.6 |
| NGC 1068 | Seyfert 2 | 12.5 | ≈107.23d | spiral | yes m | 69 |
| NGC 1365 | Seyfert 1.8 | 18.6 | 2 × 106e | spiral | no | 90.2 |
| NGC 1386 | Seyfert 2 | 15.6 | ≈107.24f | Sb/c spiral | − | 76 |
| NGC 2992 | Seyfert 1.9 | 31.5 | ≈107.72g | spiral | yes o | 150 |
| NGC 4945 | Seyfert 2 | 3.7 | ≈106.5h | spiral | no | 18 |
| NGC 5643 | Seyfert 2 | 17.3 | ≈106.4i | spiral | no | 84 |
Notes. 1) Luminosity distance. 2) Black Hole(BH) mass. 3) To determine if a galaxy reveals interactions with its surroundings. a) Marconi et al. (2006). b) Koss et al. (2017). c,d,e,f,g) Woo & Urry (2002). h) Davis et al. (2017). i) Goulding et al. (2010). j) Wang et al. (2020). l) Colina et al. (1991). m) Tanaka et al. (2017). o) Guolo-Pereira et al. (2021).
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