The VIMOS VLT Deep Survey - Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairs

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Table 5:

Spectral types of pairs for the less and the most massive selected samples. Fractions are given in brackets.
	$N_{\rm pairs}$	Early-type pairs	Late-type pairs	Mixed type pairs
$\log(M/M_{{\odot}}) \geq 9.5$	106	$31\ (29.2\%)$	$53\ (50.0\%)$	$22\ (20.8\%)$
$\log(M/M_{\odot{}}) \geq 10$	77	$29\ (37.7\%)$	$29\ (37.7\%)$	$19\ (24.6\%)$
$\log(M/M_{\odot{}}) \geq 10.5$	37	$22\ (59.5\%)$	$6\ (16.2\%)$	$9\ (24.3\%)$

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