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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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