Table A.1.
Basic parameters of the three nearby objects selected as models for the host galaxies of AGN at redshifts around the cosmic noon (see Sect. 3.1).
| Name | D | V | AB | mB | Type | Structure | Reff | log Mass | log SFR | PA | incl. | Vsys | σ |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
| NGC 809 | 79.2 | 5340 | 0.10 | 14.59 | S0 | Ring | 3.5 | 10.6 | 0.41 | -4 | 41 | 5369 | 145 |
| PGC 055442 | 105.5 | 7026 | 0.25 | 14.76 | E/SABb ( * ) | Bar + ring | 3.8 | 10.9 | -0.1 | 15 | 46 | 7036 | 149 |
| NGC 7119A | 142.3 | 9875 | 0.08 | 13.44 | SBbc | Companion | 9.9 | 11.6 | 1.4 | -45 | 57 | 9874 | 138 |
Notes. Columns correspond to: (1) galaxy name, (2) galactocentric distance in Mpc, computed assuming a Hubble flow with a Hubble constant H0 = 67.8 km s−1 Mpc−1, (3) mean heliocentric radial velocity (cz) in km s−1, (4) galactic extinction in B band, (5) total B magnitude, (6) morphological type, (7) morphological particularities reported, (8) effective radius in kpc, (9) integrated stellar mass in log M⊙, (10) star formation rate in log M⊙/yr, (11) photometric position angle in degrees, (12) inclination in degrees, (13) systemic velocity in km s−1, and (14) stellar velocity dispersion in km s−1. Data for columns (3) to (7) are as provided by HyperLeda12. Data for columns (8) to (12) are from Sánchez-Menguiano et al. (2018). Data for columns (13) and (14) are estimates of this work (see text), with rms errors always ≤10 km s−1 in both parameters. ( * )Classified by HyperLeda as elliptical, the MUSE data shows the presence of a clear spiral structure (Sánchez-Menguiano et al. 2018).
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