The DESI DR1 peculiar velocity survey: Growth rate measurements from the galaxy power spectrum

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Table F.1.

MCMC-fit cosmological parameter estimates.

fσ₈	$0 . 427_{- 0.048}^{+ 0.056}$ $Mathematical equation: $ 0.427^{+0.056}_{-0.048} $$	σ_δ, vT²	$34_{- 18}^{+ 14}$ $Mathematical equation: $ 34^{+14}_{-18} $$

b₁^δσ₈	$0 . 836_{- 0.021}^{+ 0.027}$ $Mathematical equation: $ 0.836^{+0.027}_{-0.021} $$	σ_vS²	$124_{- 22}^{+ 42}$ $Mathematical equation: $ 124^{+42}_{-22} $$

b₂σ₈	$1 . 040_{- 0.120}^{+ 0.120}$ $Mathematical equation: $ 1.040^{+0.120}_{-0.120} $$	σ_p, vT²	$34_{- 34}^{+ 23}$ $Mathematical equation: $ 34^{+23}_{-34} $$

b₁^pσ₈	$0 . 670_{- 0.150}^{+ 0.710}$ $Mathematical equation: $ 0.670^{+0.710}_{-0.150} $$	χ²/d.o.f	10.445/(125 − 7)

Notes. Corresponding to Fig.F.2, the MCMC-fit cosmological parameter estimates are presented here.

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