  It is suggested that the chemical abundance trend with the condensation
temperature, Tc , can be a signature of rocky planet formation or accretion.
Recently, a strong Tc trend was reported in the Zetta Reticuli binary system
(Saffe et al., 2016), where ${\zeta}$2 Ret Ret shows a deficit of refractory
elements relative to its companion (${\zeta}$1 Ret). This depletion was
explained by the presence of a debris disk around ${\zeta}$2 Ret. Later,
Adibekyan et al. (2016b) confirmed the significance of the trend, however,
casted doubts on the interpretation proposed. Using three individual highest
quality spectra for each star, they found that the Tc trends depend on the
individual spectra (three spectra of each star were used) used in the
analaysis. In the current work we re-evaluated the presence and variability of
the Tc trend in this system using a larger number of individual spectra. In
total, 62 spectra of ${\zeta}$2 Ret and 31 spectra of ${\zeta}$1 Ret was used.
Our results confirm the word of caution issued by Adibekyan et al. (2016b) that
nonphysical factors can be at the root of the T c trends for the cases of
individual spectra.
