Patrick Simon Argelander-Institute for Astronomy, Bonn, Germany
Patrick Simon Argelander-Institute for Astronomy, Bonn, Germany
Patrick Simon Argelander-Institute for Astronomy, Bonn, Germany
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Quality control<br />
Frequency statistics of noise peaks<br />
noise<br />
B-mode<br />
E-mode<br />
Peaks: pixel larger than all neighbour<br />
pixels in transverse&radial direction<br />
Troughs: negative peaks<br />
Noise realisations vs. E/B-mode maps<br />
tan. shear<br />
Z-scaling of tan. shear inside<br />
apertures (≈1-2 arcmin radius)<br />
mag<br />
rad. shear<br />
γ t (θ c ,z s )=− ∑<br />
i∈M s (z s )<br />
θi ∗ − θ∗ c<br />
ɛ i<br />
θ i − θ c<br />
ε i<br />
θ i<br />
θ c<br />
targets: A901a/b/α, SW and A902
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