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Table 4.

Timescale of mass assembly of the example galaxies derived from the central 1.3 arcsec.

Redshift ID Class t 10 sim $ t_{10}^{\mathrm{sim}} $ t 50 sim $ t_{50}^{\mathrm{sim}} $ t 90 sim $ t_{90}^{\mathrm{sim}} $ t 10 obs $ t_{10}^{\mathrm{obs}} $ t 50 obs $ t_{50}^{\mathrm{obs}} $ t 90 obs $ t_{90}^{\mathrm{obs}} $
[Gyr] [Gyr] [Gyr] [Gyr] [Gyr] [Gyr]
(1) (2) (3) (4) (5) (6) (7) (8) (9)
0.7 172231 SF 2.00 3.86 6.13 1.22 ± 0.01 2.11 ± 0.01 4.8 ± 0.3
0.5 218606 SF 2.03 4.05 7.44 0.63 ± 0.02 2.1 ± 0.3 7.0 ± 0.1
0.3 251598 GV 1.94 3.63 6.56 0.29 ± 0.03 3.3 ± 0.9 6.1 ± 0.5

0.7 222130 GV 1.37 2.40 5.05 0.99 ± 0.01 1.24 ± 0.01 5.2 ± 0.4
0.5 234935 GV 1.32 2.28 4.60 0.63 ± 0.01 1.2 ± 0.1 4.4 ± 0.5
0.3 277675 SF 1.38 2.40 5.11 0.28 ± 0.01 0.30 ± 0.06 3.9 ± 0.9

0.7 212087 Q 1.15 1.60 2.83 0.99 ± 0.01 1.00 ± 0.01 2.4 ± 0.1
0.5 253460 GV 1.13 1.57 2.74 0.63 ± 0.01 0.64 ± 0.01 2.6 ± 0.4
0.3 298351 SF 1.17 1.57 2.45 0.28 ± 0.01 0.30 ± 0.01 3.4 ± 0.7

Notes. (1) Redshift. (2) Galaxy ID. (3) Class: SF = star forming, GV = green valley, Q = quiescent. (4)−(6) Time when the galaxy formed 10%, 50%, and 90% of its stellar mass, respectively, as derived from TNG50. (7)−(9) Time when the galaxy formed 10%, 50%, and 90% of its stellar mass, respectively, as derived with pPXF from noiseless spectra.

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