Constraining cosmological parameters using void statistics from the SDSS survey

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Table G.1.

Difference in the cosmological constraints and their uncertainties using different amounts of Uchuu-SDSS lightcones.

	1 Uchuu-SDSS voids	5 Uchuu-SDSS voids	10 Uchuu-SDSS voids	32 Uchuu-SDSS voids	n
σ₈	0.997 $_{- 0.298}^{+ 0.277}$ $^{+0.277}_{-0.298}$	0.886 $_{- 0.245}^{+ 0.219}$ $^{+0.219}_{-0.245}$	0.880 $_{- 0.219}^{+ 0.199}$ $^{+0.199}_{-0.219}$	0.793 $_{- 0.187}^{+ 0.167}$ $^{+0.167}_{-0.187}$	-7
Γ	0.2725 $_{- 0.0816}^{+ 0.0924}$ $^{+0.0924}_{-0.0816}$	0.2576 $_{- 0.0579}^{+ 0.0605}$ $^{+0.0605}_{-0.0579}$	0.2203 $_{- 0.0393}^{+ 0.0413}$ $^{+0.0413}_{-0.0393}$	0.1787 $_{- 0.0217}^{+ 0.0237}$ $^{+0.0237}_{-0.0217}$	-2.5

Notes. Constraints of σ₈ and Γ = Ω_ch for voids from 1 Uchuu-SDSS lightcone (second column), 5 Uchuu-SDSS lightcones (third column) 10 Uchuu-SDSS lightcones (fourth column), 32 Uchuu-SDSS lightcones (fifth column) and the index n of the scaling of errors with the volume ( $V_{2} / V_{1}^{1 / n}$ $V_{2}/V_{1}^{1/n}$ , with V₁ < V₂) obtained using non-linear least squares (last column).

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