Fig. A.1

Recovered cosmic variance over input cosmic variance (top panel)
and median σσv
over the dispersion of the recovered cosmic variance (bottom
panel) as a function of Δσ. In both panels, triangles, circles, and
squares are the results from synthetic catalogues with n =
50,250, and 1000, respectively. White symbols
show the results from the BLS fit to the data (σv,BLS), while
those coloured show the ones from the MLE (σv,ML). The
n =
50 and 1000 points are shifted to avoid overlap. The dashed
lines mark identity, and the solid line in the top panel shows
the expectation from a convolution of two Gaussians in log-space,
.
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