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Table 5

Stellar parameters of the two most massive young metal-poor stars.

Gaia DR3 Teff (K) [Fe/H] (dex) log(𝑔) (dex) L (L) M (M) AgeTracks (Gyr) AgeModel (Gyr)
5413575344812320640 4936100+100$4936_{ - 100}^{ + 100}$ 1.270.1+0.1$ - 1.27_{ - 0.1}^{ + 0.1}$ 1.8740.038+0.038$1.874_{ - 0.038}^{ + 0.038}$ 362.56101.13+103.13$362.56_{ - 101.13}^{ + 103.13}$ 1.8500.57+0.57$1.850_{ - 0.57}^{ + 0.57}$ 1.040.50+1.47$1.04_{ - 0.5}^{ + 1.47}$ 1.750.46+0.46$1.75_{ - 0.46}^{ + 0.46}$
6045465055252946560 4928100+100$4928_{ - 100}^{ + 100}$ 1.040.1+0.1$ - 1.04_{ - 0.1}^{ + 0.1}$ 2.4430.034+0.034$2.443_{ - 0.034}^{ + 0.034}$ 83.1610.18+10.18$83.16_{ - 10.18}^{ + 10.18}$ 1.5820.263+0.263$1.582_{ - 0.263}^{ + 0.263}$ 1.500.50+0.95$1.50_{ - 0.50}^{ + 0.95}$ 1.480.38+0.38$1.48_{ - 0.38}^{ + 0.38}$

Notes. The Teff, [Fe/H], and log(𝑔) come from APOGEE DR17. The errors on log(𝑔) originate from the predictions of the neural network reported in APOGEE DR17. The two last columns refer to the ages obtained with the BaSTI stellar tracks and the CatBoostRegressor model, respectively.

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