Table 4.
Percentage stellar mass formed within the last 5 Gyr, m*, < 5 Gyr, from the PNLF predicted with the pick-one-out test.
| Region | m*, < 5 Gyr |
|
|---|---|---|
| HST CMD | PNLF prediction | |
| LMC | 50.1 ± 3.3 | 49.94 ± 11.98 |
| Disc (10–20 kpc) | 27.1 ± 3.7 | 20.02 ± 6.55 |
| Disc (20–30 kpc) | 14.7 ± 5.1 | 9.15 ± 11.02 |
| Giant Stream | 10.2 ± 8.4 | 18.04 ± 9.22 |
| NE Shelf | 11.1 ± 5.7 | 13.49 ± 5.78 |
| G1 Clump | 29.3 ± 4.2 | 32.23 ± 2.77 |
| W Shelf | N.A. | ≤42.19 |
| Stream D | N.A. | 27.14 ± 9.46 |
Notes. The m*, < 5 Gyr in the HST fields corresponding to the LMC, Disc (10–20 kpc), and all other regions are from Weisz et al. (2013), Williams et al. (2017), and Bernard et al. (2015) respectively. The m*, < 5 Gyr values are predicted for each region from its cf2 value by fitting the relation between cf2 and m*, < 5 Gyr for all the other regions except the selected region.
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