Fast-rotating massive Population III stars as possible sources of extreme N enrichment in high-redshift galaxies

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Table 3.

Observational data shown in Fig. 4, obtained from Fig. 6 of Marques-Chaves et al. (2024).

Galaxy	log(O/H) + 12	log(N/O)	log(C/O)
GN-z11 ^(†)	$7 . 84_{- 0.05}^{+ 0.06}$ $7.84^{+0.06}_{-0.05}$	$- 0 . 38_{- 0.04}^{+ 0.05}$ $-0.38^{+0.05}_{-0.04}$	–
GN-z11 ^(‡)	$7 . 82_{- 0.20}^{+ 0.18}$ $7.82^{+0.18}_{-0.20}$	> − 0.25	> − 0.78
CEERS-1019	7.7 ± 0.2	−0.13 ± 0.2	−0.80 ± 0.09
Sunburst	8.03 ± 0.1	−0.21 ± 0.1	−0.5 ± 0.1
Mrk 996	8.38 ± 0.3	−0.14 ± 0.3	−0.22 ± 0.3
Lynx arc	7.87 ± 0.2	−0.53 ± 0.2	−0.14 ± 0.2
SMACS2031	7.76 ± 0.1	−0.66 ± 0.1	−0.8 ± 0.1
Sun	8.69	–0.86	–0.23

Notes.

^(†)

Data from Senchyna et al. (2024).

^(‡)

Data from Cameron et al. (2023).

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