The quality function of the period fits in terms of the effective temperature for the PG 1159 sequences with different stellar masses (in solar units) corresponding to the case in which 4 observed periods are assumed to be associated to quadrupole (ℓ = 2) and the remainder 2 periods can be associated either to dipole (ℓ = 1) or quadrupole (ℓ = 2) modes. No clear and distinguishable seismological solution is evident for TIC 095332541 in this figure.