The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at z=0.2–1

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Table 4:

The five main eigenvalules of the correlation matrix derived with the bootstrap resampling of galaxies (first column) and subvolumes (Col. 2), and from the ensemble variance of the 24 mocks (Col. 3).
Eigenvalue	Bootstrap		Mocks
	Galaxies	Volumes	catalogues
$\lambda_1$	3.87784	8.28193	11.82062
$\lambda_2$	1.95834	2.17866	0.15708
$\lambda_3$	1.36841	0.71635	0.01794
$\lambda_4$	1.11316	0.38252	0.00436
$\lambda_5$	0.91683	0.20340	0.00000

For the two latest cases, each mock sample is used in turn as ``data'' and the reported
eigenvalues are the obtained as the average over the 24 mocks.

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