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Table 4

Solar abundances from STELLA+SES and VATT+PEPSI Sun-as-a-star spectra.

Element STELLA+SES VATT+PEPSI Asplund et al. (2021)
C (atomic) 8.42±0.01 8.45±0.02 8.46±0.04
CH 8.31±0.05
N (CN) 7.93±0.05 7.83±0.07
O (NIR-NLTE) 8.63±0.01 8.65±0.01 8.69±0.04
O(6300Å) 8.64±0.10
Na 6.26±0.05 6.13±0.06 6.22±0.03
Mg 7.47±0.05 7.58±0.05 7.55±0.03
Al 6.41±0.01 6.39±0.03 6.43±0.03
Si 7.47±0.02 7.55±0.02 7.51±0.03
S 7.12±0.01 7.19±0.01 7.12±0.03
K 5.16±0.02 5.11±0.06 5.07±0.03
Ca 6.27±0.03 6.29±0.03 6.30±0.03
Sc(a) 3.11±0.07 3.08±0.06 3.14±0.04
Ti 4.88±0.04 4.94±0.01 4.97±0.05
V (a) 3.90±0.02 3.94±0.04 3.90±0.08
Cr 5.50±0.02 5.64±0.03 5.62±0.04
Mn(a) 5.29±0.03 5.56±0.08 5.42±0.06
Fe 7.40±0.02 7.46±0.01 7.46±0.04
Co(a) 4.85±0.02 4.95±0.04 4.94±0.05
Ni 6.21±0.03 6.22±0.03 6.20±0.04
Cu(a) 4.04±0.10 4.14±0.05 4.18±0.05
Zn 4.49±0.04 4.56±0.06 4.56±0.05
Y 2.14±0.06 2.29±0.08 2.21±0.05
Zr 2.66±0.01(b) 2.62±0.03 2.59±0.04
Ba 2.15±0.05 2.08±0.01 2.27±0.05
La(a) 1.45±0.01 1.22±0.09 1.11±0.04
Ce 1.65±0.04 1.57±0.07 1.58±0.04
Eu(a) 0.62±0.01 0.52±0.04

Notes. Mean values and standard deviations between neutral and ionized atoms are given for Sc, Ti, Fe, and Zr. (a)HFS included in the analysis.(b) Abundance is from Zr II only.

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