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Table 1.

Marginalised 1σ errors for the cosmological parameters and the nuisance parameter (b).

rmin (h−1 Mpc)
20 25 30 35 40 45 50 55 60
w12|r12p 0.08145 0.08375 0.08579 0.08580 0.09763 0.10089 0.10434 0.10440 0.11504
Ωm 0.00915 0.00963 0.01022 0.01087 0.01176 0.01277 0.01409 0.01568 0.01753
F.I. 8.90561 8.70010 8.39213 7.89261 8.30407 7.90352 7.40415 6.65691 6.56149

w12|r12p 0.02831 0.02997 0.03111 0.03119 0.03121 0.03132 0.03253 0.03259 0.03318
Ωb 0.00240 0.00249 0.00263 0.00278 0.00296 0.00323 0.00353 0.00393 0.00444
F.I. 11.81117 12.06080 11.81358 11.21327 10.53949 9.68702 9.20470 8.29658 7.47404

w12|r12p 0.34911 0.36354 0.38179 0.38180 0.38186 0.39210 0.42847 0.43300 0.43385
h 0.02259 0.02377 0.02513 0.02648 0.02836 0.03079 0.03328 0.03644 0.04095
F.I. 15.45669 15.29114 15.19120 14.42058 13.46272 12.73427 12.87531 11.88329 10.59576

w12|r12p 0.46385 0.47031 0.49449 0.49669 0.50729 0.55604 0.57261 0.57731 0.57766
ns 0.02212 0.02341 0.02492 0.02665 0.02875 0.03078 0.03397 0.03770 0.04278
F.I. 20.96929 20.08857 19.83974 18.63610 17.64347 18.06515 16.85804 15.31241 13.50433

w12|r12p 0.17063 0.17985 0.18694 0.18736 0.26644 0.31528 0.36319 0.36372 0.37668
σ8 0.01561 0.01657 0.01737 0.01841 0.01974 0.02176 0.02374 0.02625 0.02934
F.I. 10.93136 10.85548 10.76487 10.17951 13.49618 14.48853 15.29761 13.85747 12.83753

w12|r12p 0.87743 0.92138 0.97446 0.99740 1.04269 1.06858 1.22466 1.22523 1.33489
Mν 0.06547 0.06828 0.07146 0.07585 0.08156 0.08845 0.09809 0.10836 0.12265
F.I. 13.40268 13.49481 13.63547 13.15010 12.78485 12.08153 12.48528 11.30666 10.88373

w12|r12p 0.20413 0.20429 0.20610 0.21088 0.22348 0.22854 0.30910 0.32395 0.34865
b 0.01945 0.02333 0.02809 0.03340 0.04042 0.04755 0.05586 0.06514 0.07683
F.I. 10.49718 8.75640 7.33811 6.31302 5.52863 4.80646 5.53373 4.97336 4.53813

Notes. Different columns show the constraints obtained by changing the minimum separation length considered, while fixing the maximum separation to 120 h−1 Mpc. The various rows display the results for different parameters, and each of these rows is further divided into three rows to focus on the constraint coming from ⟨w12|r12p, , and the factor of improvement of the constraints from over ⟨w12|r12p denoted by F.I., respectively.

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