Relation between newly produced ejecta (E_j) on the y-axis of the elements C¹², O¹⁶, S, and Fe vs. the initial mass (M_i) on the x-axis from Z = 0.0001 rotational models of Goswami et al. (2022) in green (solid and dotted lines for two rotation rate values), based on Heger & Woosley (2002) pure He non-rotating models. The CCSN yields are shown in blue. The yields of rotating (solid) and non-rotating (dotted) models by Takahashi et al. (2018) for zero metallicity stars are shown in red. Since the actual S and Fe CCSN yields are low, they are shown multiplied by a factor of 15 for clarity.