footnote_lum.tex

\paragraph{$^{$FOOTNOTE_NUMBER$}$Luminosities are given in the GAMA bands}\label{footnote:$FOOTNOTE_NUMBER$} and always using the same order 
as in the snapshots: u, g, r, i, z, Y, J, H, K. These are rest-frame dust-free
AB-luminosities of the star particles. These were computed using the \href{https://ui.adsabs.harvard.edu/abs/2003MNRAS.344.1000B}{Bruzual \& Charlot 2003}
(GALAXEV) models convolved with different filter bands and interpolated in
log-log (f(log(Z), log(age)) = log(flux)) as used in the dust-free modelling
of Trayford et al. (2015). The luminosities are given in dimensionless
units. They have been divided by 3631 Jy already, i.e. they can be turned
into absolute AB-magnitudes (rest-frame absolute maggies) directly by
applying -2.5 log10(L) without additional corrections.