Table 3.
Age and mass estimates for the Sculptor stars observed with Giraffe.
| Method tracks |
Method isochrones |
|||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Solution0 |
Solution1 |
Solution2 |
Solution1 |
Solution2 |
||||||||||||
| Name | Age | Mass | Phase | Age | Mass | Phase | Age | Mass | Phase | Age | Mass | Phase | Age | Mass | Phase | |
| (Myr) | (M⊙) | (Myr) | (M⊙) | (Myr) | (M⊙) | (Myr) | (M⊙) | (Myr) | (M⊙) | |||||||
| Scl2 | 629 | 2.0 | CHeB | 629 | 2.0 | CHeB | 473 | 2.4 | RGB | 499 | 2.5 | CHeB | 389 | 2.7 | SG | |
| Scl3 | 494 | 2.4 | CHeB | 494 | 2.4 | CHeB | 494 | 2.4 | CHeB | 722 | 2.2 | CHeB | 331 | 2.8 | SG | |
| Scl8 | 544 | 2.2 | CHeB | 1206 | 1.8 | AGB | 512 | 2.4 | CHeB | 731 | 2.2 | CHeB | 358 | 2.8 | SG | |
| Scl9 | 467 | 2.4 | CHeB | 790 | 2.0 | CHeB | 467 | 2.4 | CHeB | 703 | 2.3 | CHeB | 317 | 2.8 | SG | |
| Scl12 | 912 | 1.9 | CHeB | 912 | 1.9 | CHeB | 848 | 1.9 | AGB | 757 | 2.1 | SG | 339 | 2.8 | SG | |
| Scl19 | 781 | 2.1 | CHeB | 4715 | 1.1 | RGB | 468 | 2.4 | RGB | 399 | 2.8 | SG | ||||
| Scl29 | 436 | 2.4 | CHeB | 962 | 1.9 | AGB | 436 | 2.4 | CHeB | 795 | 2.0 | AGB | 752 | 2.1 | CHeB | |
| Scl31 | 980 | 1.9 | CHeB | 1301 | 1.7 | CHeB | 581 | 2.3 | CHeB | 1356 | 1.7 | CHeB | 482 | 2.3 | SG | |
| Scl38 | 1016 | 1.9 | CHeB | 1171 | 1.6 | CHeB | 537 | 2.4 | CHeB | 1393 | 1.7 | CHeB | 521 | 2.3 | RGB | |
| Scl47 | 608 | 2.1 | CHeB | 1403 | 1.6 | RGB | 521 | 2.3 | RGB | 608 | 2.1 | CHeB | 555 | 2.2 | RGB | |
| Scl61 | 782 | 2.1 | CHeB | 852 | 2.0 | CHeB | 613 | 2.2 | CHeB | 2168 | 1.4 | CHeB | 658 | 2.0 | CHeB | |
| Scl68 | 655 | 2.2 | CHeB | 1062 | 1.8 | CHeB | 523 | 2.4 | CHeB | 962 | 1.9 | CHeB | 394 | 2.6 | SG | |
| Scl70 | 723 | 2.2 | CHeB | 957 | 1.9 | CHeB | 488 | 2.3 | CHeB | 904 | 2.0 | CHeB | 364 | 2.6 | SG | |
| Scl75 | 740 | 2.1 | CHeB | 1309 | 1.7 | CHeB | 630 | 2.2 | CHeB | 1144 | 1.8 | CHeB | 449 | 2.4 | SG | |
Notes. Two types of solutions from “method tracks” and “method isochrones” are provided. The solutions “1” and “2” correspond to the lowest and highest possible mass in different methods, respectively. The solution “0” of the “method tracks” is the most probable solution based on the elapsed-time argument.
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