Slides of 5 lectures at XV Brazilian School on Cosmology and ...

McClure-Dyer Gaussian window averageActually for COMPOSITE sample better to fitH −1α =∑ Ni=1 W i α r i (cz i ) −1∑ Nj=1 W j α,W i α =σ 2 H −1i1( −θ2√ exp i2πσθ2σ 2 θ), σ H−1i= σ icz iCanonical value <strong>of</strong> σ θ= 25 ◦ used, but varied15 ◦ < σ θ< 40 ◦ with no significant change. However, 2σ θmust be gre<strong>at</strong>er than Zone <strong>of</strong> Avoidance diameter.15th <strong>Brazilian</strong> <strong>School</strong> on Cosmology and Gravit<strong>at</strong>ion, August 2012 – p.122/143