Ratio of previous ²⁸P(p, γ)²⁹S rates normalized to present recommended rate (the median rates in Table 5). The different line patterns correspond to the rates from Rauscher & Thielemann (2000), Cyburt et al. (2010), Wallace & Woosley (1981), and Sallaska et al. (2013), as marked in rath, ths8, wawo, and starlib, respectively. The shallow blue shaded areas correspond to 68% coverage probabilities, labeled as “Low” and “High” in Table 5. The vertical shallow gray band indicates the typical temperature range of nova nuclear burning.