Upper panel: percentage of observations per element according to the SAGA database, adding the detections of the star HD 222925. Dashed vertical lines show specific elements as indicated at the top of the plot. Lower panel: median abundances of all previous calculations of the models H (blue line), L1-90 (green line), and L1-0 (orange line) versus atomic number using the same color scheme as Fig. 2.. Shaded bands around the lines give the maximum and minimum yield or the calculations outlined in the previous section. Hereby, we include all variations with the exception of the calculations with no included neutrino reactions. Black squares indicate abundances of the r-process enhanced star HD 222 925 (Roederer et al. 2022), magenta circles the star HD 122 563 from Honda et al. (2007) with additional values of Roederer et al. (2012) indicated by magenta diamonds. Cyan stars and brown triangles indicate the stars CS22897-008 from Spite et al. (2018) and HE0109-4510 from Hansen et al. (2015), respectively. All stars are normalized to the abundance of Sr (Z = 38) of model L1-0. Upper limits are indicated with a downwards pointing arrow. The background colours indicate different percentages of observations (out of a total of ∼19 500 stars) as shown in the upper panel: green indicates more than 5 per cent, blue more than 1 per cent, orange more than one observation, red exactly one observation, and white no observation at all. This gives an estimate on how easy it is to observe a certain element. The arrows at the bottom of the lower panel indicate the regions of the first, second, and third r-process peak.