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

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Table 3:

The completeness in stellar mass of mass-selected mock subsamples reproducing the properties and selection criteria of our 10K data samples.
Sample	Redshift	Stellar mass ( $\log(M/M_\odot)$ )	Completeness
	range	range
M1.1	0.2-0.5	$\ge$ 9.0	0.783
M1.2	0.2-0.5	$\ge$ 9.5	0.972
M1.3	0.2-0.5	$\ge$ 10.0	1.000
M1.4	0.2-0.5	$\ge$ 10.5	1.000
M2.1	0.5-0.8	$\ge$ 9.0	0.349
M2.2	0.5-0.8	$\ge$ 9.5	0.652
M2.3	0.5-0.8	$\ge$ 10.0	0.919
M2.4	0.5-0.8	$\ge$ 10.5	0.996
M3.1	0.8-1.0	$\ge$ 10.0	0.571
M3.2	0.8-1.0	$\ge$ 10.5	0.882

Source LaTeX | All tables | In the text

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