Evaluated spectroscopic data and level schemes from radioactive decay and nuclear reaction studies are presented for ²³N, ²³O, ²³F, ²³Ne, ²³Na, ²³Mg, ²³Al, and ²³Si. This evaluation for A=23 supersedes the earlier one by R. B. Firestone (2007Fi02).

Highlights of this evaluation are the following:

The recommended absolute γ-ray emission probability (%Pγ) in the ²³Ne β-decay was reported with 3.0% systematic uncertainty in 1986BrZQ. In 2007Fi02, the Pγ for the most intense γ ray was recommended with 4% uncertainty. These uncertainties are comparable with the total excited state β feeding uncertainty of 33 l, resulting from 100–67 l (g.s. β feeding) in ²³Na (1963Ca06). In this evaluation, notes are added for relative and absolute γ-ray emission probabilities.

From new measurements 2020Kw01 constrain the spin of the 7788 keV level, the dominant resonance state for the ²²Na(p,γ)²²Mg reaction rate at stellar temperature, in ²³Mg to (3/2⁺,5/2⁺). Earlier assignment was 7/2⁺.

The ²³Al ε decay scheme appears to be incomplete. Some of the latest reported data on the ²³Al ε decay study in the literature need verification.

提出了由放射性衰变和核反应研究得出的评估光谱数据和能级方案，涉及的是²³ N，²³ O，²³ F，²³ Ne，²³ Na，²³ Mg，²³ Al和²³ Si。对于A = 23的此评估取代了RB Firestone（2007Fi02）的较早评估。

该评估的重点如下：

推荐的绝对γ射线发射概率（％P γ中）²³氖β衰变报道与1986BrZQ 3.0％，系统性不确定性。在2007Fi02，在P γ为最强烈的γ建议用4％的不确定性射线。这些不确定性都与总激发态可比β 33升的馈送的不确定性，从100-67升（GS所得β在喂养）²³的Na（1963Ca06）。在此评估中，添加了有关相对和绝对γ射线发射概率的注释。

从新的测量值2020Kw01可以限制7788 keV水平的自旋，这是恒星温度下²² Na（p，γ）²² Mg反应速率的主要共振态，在²³ Mg至（3/2 ⁺，5/2 ⁺）之间。较早的任务是7/2 ⁺。

在²³的Al ε衰变方案似乎是不完整的。一些在最新的报告数据的²³铝ε文献需要验证衰变研究。