Table 1.
Coefficients, probabilities and likelihoods of the observations fitting the different models and rest frames.
| Model | Frame | kobs |
 |
σk, mock | Δk[σ] | P |
|---|---|---|---|---|---|---|
| Λ-CDM (full) | LG | −0.06 | −0.05 | 0.25 | 0.34 | 0.734 |
| Λ-CDM (full) | CMB | −0.03 | −0.05 | 0.25 | 0.74 | 0.459 |
| Λ-CDM (selected) | LG | −0.19 | −0.25 | 0.23 | 2.24 | 0.025 |
| Λ-CDM (selected) | CMB | −0.16 | −0.25 | 0.23 | 3.75 | 0.0002 |
| Differential expansion (full) | LG | −0.06 | −0.19 | 0.23 | 5.69 | < 0.0001 |
| Differential expansion (full) | CMB | −0.03 | −0.19 | 0.23 | 6.86 | < 0.0001 |
| Differential expansion (selected) | LG | −0.19 | −0.39 | 0.20 | 9.50 | < 0.0001 |
| Differential expansion (selected) | CMB | −0.16 | −0.39 | 0.20 | 11.22 | < 0.0001 |
Notes. LG stands for local group and CMB for cosmic microwave background. kobs: slope of the weight least square fitted linear regression on the observational data; 
: mean expected slope for a specific model; σk, mock: standard deviation of the slope for a specific model (derived using the different combined mock catalogues); Δk: deviation of the observations from the mean value of the model, given in standard deviations; P: probability for the observations to be represented by the model.
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