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Table D.1.
Details of the columns provided in the catalogue associated with this paper.
| Number | Name | Units | Description |
|---|---|---|---|
| 1 | KID | KROSS ID. (Harrison et al. 2017, hereafter Ref: H17). | |
| 2 | Name | Object name (Ref: H17). | |
| 3 | Redshift | Redshift from Hα (Ref: H17). | |
| 4 | INC | Degrees | Inclination angle (Ref: H17). |
| 5–6 | Re, Re_err | kpc | Deconvolved continuum half-light radii, R1/2, from the image and error (Ref: H17). |
| 7–8 | Ve, Ve_err | km s−1 | Rotation velocity computed at Re and error. |
| 9–10 | Vopt, Vopt_err | km s−1 | Rotation velocity computed at 1.89 Re or 3.2 RD (where RD = 0.59 Re) and error. |
| 11–12 | Vout, Vout_err | km s−1 | Rotation velocity computed at 2.95 Re or 5 RD and error. |
| 13–14 | Mstar, Mstar_err | M⊙ | Stellar mass derived from fixed mass-to-light ratio and error. |
| 15–16 | MH2, MH2_err | M⊙ | Molecular gas mass derived from derived from scaling relation and error. |
| 17–18 | MHI, MHI_err | M⊙ | Atomic gas mass (includes helium content) derived from derived from scaling relation and error. |
| 19 | Rot_Disp_ratio_int | – | Rotation to dispersion ratio derived from intrinsic velocity (inclination corrected) |
| 20–21 | Rgas, Rgas_err | log(kpc) | Gaseous disk length derived from Hα surface brightness and error |
| 22 | Rout_Flag | – | If ‘F’ then Vout cannot be extrapolated due to large difference between last point in rotation curve and Rout. |
| 23 | Mstar_flag | – | If ‘F’ then Mdyn < M*. |
| 24 | Wiggle_Flag | – | If ‘F’ then RC is badly perturbed. |
| 25 | Rgas_flag | – | If ‘F’ then Rgas is unable to determine. |
Notes. For details of other relevant physical quantities such as velocity dispersion, Hα luminosity, see the catalogue released with Sharma et al. (2021).
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