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Cosmic Voids As Standard Rulers for Cosmology - iap.fr · Statistical estimation of the shape χ2(A,R V,RE,V,σ0,σ1)=∑ p Sp [ (np−n(rp,zp))2 σ2(r p,zp,n(rp,zp)) +logσ(rp,zp,n(rp,zp))]Pixel
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