[X/H] as a function of the atomic number. Also log ¹²C/¹³C is shown (shifted downwards by 4 dex for clarity). Each panel is dedicated to one observed CEMP-no star (red starry symbols). Arrows indicate upper/lower limits. If available, error bars are indicated. The correction Δ[C/Fe] of Placco et al. (2014b) applied on [C/Fe] (if any) is taken into account and indicated in the upper-left corner. In each panel we show the composition of the ejecta of the indicated models (solid, dashed and dotted lines). The masses ejected by the winds (M_W) and the supernova (M_SN) are written in the upper-right corner of each panel. The composition of the ISM is shown in the first panel. The dilution coefficient D and A(Li) value (if available) are shown in the upper-left corner. The range of observed [X/H] ratios and log (¹²C /¹³C) ratios for the stars in Table 2 are shown by the red rectangles.