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Table 1 The exact form of functions used to define models 1–9.

From: Supernova Ia observations in the Lemaître-Tolman model

Model Pair of functions
model 1 t B = 0; ρ/ρ b = 0.5 + 0.2 cos(10-5πrMpc-1) + 0.5 cos2(10-5πrMpc-1)
model 2 t B = 0; ρ/ρ b = 0.4 + 0.6 cos(2 × 10-5πrMpc-1) + 1.8 cos2(2 × 10-5πrMpc-1)
model 3 t B = 0; ρ/ρ b = 1 + 0.4 cos(10-5πrMpc-1)
model 4 t B = 0; ρ/ρ b = 1 + (8 × 10-6rMpc-1)0.55
model 5 ρ/ρ b = 1;
  H/H0 – not an analytic functions, see Fig. 4.1.2
model 6 t B = 0; H/H0 = 1
model 7 as in model 1
model 8 as in model 2
model 9 as in model 3