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Table 1.

General characteristics of the BETIS showcase sample, in order of morphological type.

Galaxy Morphology RA Dec D z FWHM Incl PA spx size log M log SFR
(J2000) (J2000) (kpc) (pc) (°) (°) (pc) (M) (M yr−1)
NGC863 SA(s)a 02h14m −00d46m 34 0.02639 591.98 22.40 175.6 109 12.02 0.37
NGC3393 (R′)SB(rs)a 10h48m −25d09m 69 0.01246 253.56 25.74 12.8 51 10.96 0.19
NGC6627 (R′)SB(s)b 18h22m 15d41m 28 0.01771 297.82 25.12 70.0 73 10.94 0.12
NGC692 (R′)SB(r)bc 01h48m −48d38m 96 0.02115 395.21 30.30 84.4 87 11.33 0.45
ESO584-7 Sc 16h12m −21d37m 65 0.03171 618.88 45.12 148.0 131 10.52 0.40
ESO325-43 SAB(s)c pec 13h59m −37d51m 107 0.03503 960.03 38.37 115.0 145 10.56 0.14
IC3476 IB(s)m 12h32m 14d03m 10 −0.00063 49.60 33.99 30.0 16 11.03 0.69

Notes. The columns represents, from left to right: the designation of the galaxy, the morphological Hubble-De Vaculeurs type, the RA and Dec in the J2000 epoch of the centre of the galaxies, restricted from the Paranal observatory (Dec < 25°), the physical diameter in kpc, the redshift, the PSF FWHM in pc, inclination with respect to the line of sight (in deg), the position angle (in deg) and the physical size of the spaxel, in parsec/spaxel, the log of the integrated stellar mass in solar masses, and the log of the star formation rate in solar masses per year. The RA, Dec, the diameter and the redshift are obtained from NED. The morphological type and position angle, from Hyperleda. M was obtained from López-Cobá et al. (2020), except NGC3393 and NGC6627 that was obtained from SSP fitting. The SFR was obtained as explained in Sect. 2.

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