M_ej: ejected mass in the line-forming region.

M_{ej, s}: mass of a species in the line-forming region.

L_bol: total bolometric luminosity.

M_{bol, s}: bolometric luminosity from the species' line interaction.

Temperature: temperature of the photosphere and its line-forming region

Caveat 1: all results are based on the solar r-process abundance (Prantzos et al., 2020).

Caveat 2: the bolometric luminosity is computed from 3000A to 25000A.

Caveat 3: Other setup can be found in the Simulation Setup page.