Table 1.
TNG50 galaxy sample at z = 0.
| Galaxy ID | log10(Mcrit200) | log10(M*) | D/T ((D/T)pso) | B/T ((B/T)pso) | Reff, bulge | hdisc |  |
rbar | |
|---|---|---|---|---|---|---|---|---|---|
| log10(M⊙) | log10(M⊙) | kpc | kpc | kpc | |||||
| 560751 | 11.90 | 10.62 | 0.53 (0.69) | 0.25 (0.29) | 0.92 | 4.52 | 0.57 | 6.48 | |
| 563732 | 11.91 | 10.56 | 0.58 (0.75) | 0.26 (0.12) | 0.81 | 5.51 | 0.55 | 2.64 | |
| 569251 | 11.84 | 10.60 | 0.85 (0.84) | 0.07 (0.11) | 0.91 | 3.58 | 0.61 | 3.52 | |
| 574286 | 11.71 | 10.34 | 0.68 (0.74) | 0.11 (0.20) | 0.42 | 2.56 | 0.53 | 2.40 | |
| 547293 | 11.96 | 10.73 | 0.81 (0.71) | 0.05 (0.24) | 1.10 | 2.72 | 0.48 | 5.28 | |
| 543376 | 11.97 | 10.79 | 0.67 (0.85) | 0.12 (0.13) | 0.90 | 5.78 | 0.38 | 2.16 | |
| Median | 11.91 | 10.61 | 0.67 (0.73) | 0.12 (0.17) | 0.91 | 4.05 | 0.54 | 3.08 |
Notes. From left to right: Galaxy ID from TNG50 simulation, the logarithm of halo mass, disc (thin and thick components) to total mass fraction from kinematic decomposition (from fitting surface density stellar profiles as described in Appendix A), bulge (classical component) to total mass fraction from kinematic decomposition (from fitting surface density stellar profiles), the effective radius from the bulge calculated from a Sersic profile, the disc scale length (fitting face-on stellar surface density profiles of the kinematic component), bar strength and bar length (using Fourier decomposing face-on stellar surface density as described in Appendix A.1).
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