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Table 3.
Priors of our numerical fits.
| Parameters | Redshift z | Function y2 | Padé P2, 1 |
|---|---|---|---|
| h0 | [0.4, 1.0] | [0.4,1.0] | [0.4,1.0] |
| q0 | [−1.0, 0.0] | [−1.5, 0.5] | [−2.0, 1.0] |
| j0 | [−2.0, 2.0] | [−2.0, 3.0] | [−2.0, 3.0] |
| s0 | [−2.0, 2.0] | [−6.0, 6.0] | [−6.0, 6.0] |
Notes. The large intervals for y2 and P2, 1 are due to the computational complexity that increases as alternative versions of expansions are involved into computation. In our results, no poles and/or divergences occur for P2, 1 in the range of explored redshifts.
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