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Table E.1

Best fit parameters and uncertainties of optical-only fits. Rows with gray text indicate parameter values that are likely not representative of the stellar properties.

Source Teff [K] log g v sin i [km s−1] log M˙$\[\dot{M}\]$ yHe εC εN εO εSi
AV 80 43250−250+500$\[43250_{-250}^{+500}\]$ 3.84−0.06+0.12$\[3.84_{-0.06}^{+0.12}\]$ 305−20+25$\[305_{-20}^{+25}\]$ −6.14−0.05+0.08$\[-6.14_{-0.05}^{+0.08}\]$ 0.08−0.01+0.02$\[0.08_{-0.01}^{+0.02}\]$ 8.2−0.8+0.1$\[8.2_{-0.8}^{+0.1}\]$ 7.5−0.4+0.4$\[7.5_{-0.4}^{+0.4}\]$ 7.0−0.8+0.7$\[7.0_{-0.8}^{+0.7}\]$ 6.4−0.4+0.7$\[6.4_{-0.4}^{+0.7}\]$
AV 15 40500−750+750$\[40500_{-750}^{+750}\]$ 3.64−0.06+0.08$\[3.64_{-0.06}^{+0.08}\]$ 110−10+10$\[110_{-10}^{+10}\]$ −6.07−0.05+0.08$\[-6.07_{-0.05}^{+0.08}\]$ 0.10−0.01+0.01$\[0.10_{-0.01}^{+0.01}\]$ 7.5−0.6+0.3$\[7.5_{-0.6}^{+0.3}\]$ 7.8−0.2+0.2$\[7.8_{-0.2}^{+0.2}\]$ 6.1−0.1+1.1$\[6.1_{-0.1}^{+1.1}\]$ 6.3−0.3+0.5$\[6.3_{-0.3}^{+0.5}\]$
AV 95 37750−250+1000$\[37750_{-250}^{+1000}\]$ 3.60−0.04+0.08$\[3.60_{-0.04}^{+0.08}\]$ 75−10+10$\[75_{-10}^{+10}\]$ −6.50−0.08+0.03$\[-6.50_{-0.08}^{+0.03}\]$ 0.14−0.02+0.01$\[0.14_{-0.02}^{+0.01}\]$ 7.4−0.5+0.1$\[7.4_{-0.5}^{+0.1}\]$ 7.8−0.1+0.1$\[7.8_{-0.1}^{+0.1}\]$ 8.2−0.8+0.2$\[8.2_{-0.8}^{+0.2}\]$ 6.7−0.7+0.2$\[6.7_{-0.7}^{+0.2}\]$
AV 207 38250−750+750$\[38250_{-750}^{+750}\]$ 3.86−0.06+0.06$\[3.86_{-0.06}^{+0.06}\]$ 110−15+10$\[110_{-15}^{+10}\]$ −7.02−0.10+0.13$\[-7.02_{-0.10}^{+0.13}\]$ 0.12−0.03+0.01$\[0.12_{-0.03}^{+0.01}\]$ 7.5−0.8+0.2$\[7.5_{-0.8}^{+0.2}\]$ 7.9−0.3+0.1$\[7.9_{-0.3}^{+0.1}\]$ 8.4−0.6+0.4$\[8.4_{-0.6}^{+0.4}\]$ 6.5−0.5+0.4$\[6.5_{-0.5}^{+0.4}\]$
AV 69 36750−250+1500$\[36750_{-250}^{+1500}\]$ 3.48−0.06+0.12$\[3.48_{-0.06}^{+0.12}\]$ 100−15+10$\[100_{-15}^{+10}\]$ −6.47−0.05+0.08$\[-6.47_{-0.05}^{+0.08}\]$ 0.09−0.01+0.03$\[0.09_{-0.01}^{+0.03}\]$ 7.5−0.5+0.4$\[7.5_{-0.5}^{+0.4}\]$ 6.7−0.7+0.2$\[6.7_{-0.7}^{+0.2}\]$ 6.2−0.3+1.1$\[6.2_{-0.3}^{+1.1}\]$ 6.8−0.8+0.3$\[6.8_{-0.8}^{+0.3}\]$
AV 469 33750−1000+1000$\[33750_{-1000}^{+1000}\]$ 3.24−0.08+0.12$\[3.24_{-0.08}^{+0.12}\]$ 85−10+10$\[85_{-10}^{+10}\]$ −6.00−0.08+0.05$\[-6.00_{-0.08}^{+0.05}\]$ 0.20−0.04+0.03$\[0.20_{-0.04}^{+0.03}\]$ 7.3−0.4+0.4$\[7.3_{-0.4}^{+0.4}\]$ 8.3−0.3+0.1$\[8.3_{-0.3}^{+0.1}\]$ 8.0−0.2+0.7$\[8.0_{-0.2}^{+0.7}\]$ 7.2−0.3+0.4$\[7.2_{-0.3}^{+0.4}\]$
AV 479 33750−750+250$\[33750_{-750}^{+250}\]$ 3.34−0.10+0.04$\[3.34_{-0.10}^{+0.04}\]$ 90−5+15$\[90_{-5}^{+15}\]$ −6.04−0.08+0.05$\[-6.04_{-0.08}^{+0.05}\]$ 0.13−0.01+0.04$\[0.13_{-0.01}^{+0.04}\]$ 7.5−0.2+0.2$\[7.5_{-0.2}^{+0.2}\]$ 7.5−0.2+0.4$\[7.5_{-0.2}^{+0.4}\]$ 7.8−1.0+0.5$\[7.8_{-1.0}^{+0.5}\]$ 6.9−0.2+0.4$\[6.9_{-0.2}^{+0.4}\]$
AV 307 29250−1750+250$\[29250_{-1750}^{+250}\]$ 3.42−0.18+0.06$\[3.42_{-0.18}^{+0.06}\]$ 55−10+15$\[55_{-10}^{+15}\]$ −6.88−0.28+0.08$\[-6.88_{-0.28}^{+0.08}\]$ 0.11−0.03+0.01$\[0.11_{-0.03}^{+0.01}\]$ 7.5−0.3+0.4$\[7.5_{-0.3}^{+0.4}\]$ 7.8−0.3+0.5$\[7.8_{-0.3}^{+0.5}\]$ 8.0−0.5+0.2$\[8.0_{-0.5}^{+0.2}\]$ 6.7−0.3+0.5$\[6.7_{-0.3}^{+0.5}\]$
AV 372 29750−500+1250$\[29750_{-500}^{+1250}\]$ 2.88−0.06+0.14$\[2.88_{-0.06}^{+0.14}\]$ 155−5+15$\[155_{-5}^{+15}\]$ −5.91−0.05+0.05$\[-5.91_{-0.05}^{+0.05}\]$ 0.17−0.03+0.03$\[0.17_{-0.03}^{+0.03}\]$ 7.7−0.3+0.3$\[7.7_{-0.3}^{+0.3}\]$ 7.6−0.2+0.3$\[7.6_{-0.2}^{+0.3}\]$ 8.3−2.2+0.7$\[8.3_{-2.2}^{+0.7}\]$ 7.3−0.5+0.2$\[7.3_{-0.5}^{+0.2}\]$
AV 327 31750−1000+750$\[31750_{-1000}^{+750}\]$ 3.26−0.08+0.10$\[3.26_{-0.08}^{+0.10}\]$ 80−15+10$\[80_{-15}^{+10}\]$ −6.47−0.18+0.10$\[-6.47_{-0.18}^{+0.10}\]$ 0.15−0.04+0.01$\[0.15_{-0.04}^{+0.01}\]$ 7.2−0.3+0.2$\[7.2_{-0.3}^{+0.2}\]$ 7.8−0.4+0.2$\[7.8_{-0.4}^{+0.2}\]$ 7.8−1.7+0.5$\[7.8_{-1.7}^{+0.5}\]$ 6.8−0.2+0.3$\[6.8_{-0.2}^{+0.3}\]$
AV 83 37000−1750+1750$\[37000_{-1750}^{+1750}\]$ 3.24−0.12+0.24$\[3.24_{-0.12}^{+0.24}\]$ 80−20+45$\[80_{-20}^{+45}\]$ −5.87−0.05+0.05$\[-5.87_{-0.05}^{+0.05}\]$ 0.18−0.05+0.06$\[0.18_{-0.05}^{+0.06}\]$ 7.4−1.4+0.3$\[7.4_{-1.4}^{+0.3}\]$ 8.6−0.3+0.4$\[8.6_{-0.3}^{+0.4}\]$ 7.0−1.1+1.8$\[7.0_{-1.1}^{+1.8}\]$ 6.5−0.6+1.4$\[6.5_{-0.6}^{+1.4}\]$
2dFS 163 33500−750+750$\[33500_{-750}^{+750}\]$ 3.54−0.18+0.24$\[3.54_{-0.18}^{+0.24}\]$ 90−35+35$\[90_{-35}^{+35}\]$ −6.20−0.05+0.08$\[-6.20_{-0.05}^{+0.08}\]$ 0.08−0.01+0.05$\[0.08_{-0.01}^{+0.05}\]$ 7.2−1.2+0.5$\[7.2_{-1.2}^{+0.5}\]$ 7.8−1.3+0.6$\[7.8_{-1.3}^{+0.6}\]$ 6.2−0.3+2.0$\[6.2_{-0.3}^{+2.0}\]$ 6.2−0.2+0.7$\[6.2_{-0.2}^{+0.7}\]$
AV 70 30750−1000+750$\[30750_{-1000}^{+750}\]$ 3.02−0.08+0.06$\[3.02_{-0.08}^{+0.06}\]$ 120−15+15$\[120_{-15}^{+15}\]$ −5.75−0.05+0.08$\[-5.75_{-0.05}^{+0.08}\]$ 0.15−0.01+0.04$\[0.15_{-0.01}^{+0.04}\]$ 7.3−0.2+0.3$\[7.3_{-0.2}^{+0.3}\]$ 7.7−0.2+0.2$\[7.7_{-0.2}^{+0.2}\]$ 7.0−1.0+1.6$\[7.0_{-1.0}^{+1.6}\]$ 6.6−0.2+0.4$\[6.6_{-0.2}^{+0.4}\]$

Notes. The bottom rows with gray text indicate parameter values that are likely not representative of the stellar properties due to poor fits.

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