Table 3.
SED and morphological properties of the different substructures of CEERS-1019.
| ID | RA | Dec | reff | Age | SFR10 Myr | log(M⋆) | log(ΣM) | log(ΣSFR) |
|---|---|---|---|---|---|---|---|---|
| [J2000] | [J2000] | [pc] | [Myr] | [M⊙ yr−1] | [M⊙] | [M⊙ pc−2] | [M⊙ yr−1 kpc−2] | |
| (1) | (2) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| A | 14:20:08.50 | +52:53:26.37 | 112 ± 12 | 4.0 ± 0.3 | 148 ± 25 | 8.76 ± 0.04 | 3.86 ± 0.11 | 3.27 ± 0.11 |
| B | 14:20:08.51 | +52:53:26.51 | 145 ± 35 | 5.7 ± 0.7 | 83 ± 18 | 8.66 ± 0.15 | 3.55 ± 0.53 | 2.81 ± 0.21 |
| C | 14:20:08.48 | +52:53:26.36 | 101 ± 9 | 15.0 ± 3.0 | 2 ± 10 | 8.94 ± 0.12 | 4.14 ± 0.14 | < 2.27 |
| Total | – | – | – | 14.4 ± 7.2 | 161 ± 23 | 9.31 ± 0.15 | – | – |
Notes. (1) different components of CEERS-1019, (2) J2000 coordinates, (3) the effective radius, (4) burst age for components A, B, and C, and age assuming CSF for “total”, (5) 10 Myr-weighted SFR (6) and (7) stellar mass and mass surface density, defined as 
, and (8) SFR surface density.
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