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Table F.1.

Column description of the MAGIC catalogue, which contains morpho-kinematics and physical parameters for the MS sample of 447 galaxies.

No. Title Description
1 ID MUSE galaxy ID in the form X-CGRY, where X refers to the galaxy identification number within the field
targeting COSMOS group CGRY
2 z Spectroscopic systemic redshift derived from kinematics modelling
3 RA J2000 Right Ascension of morphological centre in decimal degrees
4 Dec J2000 Declination of morphological centre in decimal degrees
5 N Number of galaxies in structures with more than three members
6 Reffd Disk effective radius in kpc (Reff,d)
7 Reffb Bulge effective radius in kpc (Reff,b)
8 Reff Global effective radius in kpc (Reff)
9 logBD Logarithm of the bulge-to-disk ratio at Reff
10 q Axis ratio of the disk (q)
11 PAm Morphological position angle of the major axis in degrees
12 FWHM Median PSF FWHM, corresponding to narrow band [O II] MUSE observations in arcsecond
13 OIIflux(R22) [O II] flux derived from MUSE flux maps at R22 = 1.311 × Reff,d in 10−21 erg s−1 cm−2
14 OIIflux [O II] flux derived from MUSE flux maps at 3″ in 10−21 erg s−1 cm−2
15 SNR Total [O II] signal-to-noise ratio ((S/N)tot)
16 i Disk inclination corrected for thickness in degrees (i)
17 PAk Kinematics position angle of the major axis in degrees
18 rs NFW halo scale radius in kpc (rs)
19 Vhmax Maximum rotation velocity of the NFW rotation curve in km s−1 (Vh, max)
20 Vr22 Rotation velocity at R22 in km s−1 (V22)
21 sigma Median velocity dispersion in km s−1 (σV)
22 Vc22 Corrected rotation velocity at R22 in km s−1 (Vc, 22)
23 logM* Logarithm of the stellar mass (M / M) within an aperture of 3″
24 logM*(R22) Logarithm of the corrected stellar (M⋆,corr / M) inside R22
25 logSFR Logarithm of the SFR (SFR / [M yr−1]) at 3″ using Gilbank et al. (2010, 2011) prescription
26 logMg Logarithm of the gas mass (Mg / M) computed from the Schmidt-Kennicutt law and [O II] flux
measured at R22
27 logMdyn Logarithm of the dynamical mass (Mdyn / M) computed at R22 from the mass model

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