Table 3: Limits in mmag for detecting the individual groups of objects. For example 49% of all CP1 stars can be detected with a 3 $\sigma$ limit of +5 mmag. In addition, the mean group $\overline {\Delta a}$ , the maximum values for group members $\Delta a_{\rm m}$ , and the number N of well-established members for the analysis are listed.
+5 +10 +15 +20 $\overline {\Delta a}$ $\Delta a_{\rm m}$ N

CP1 49% 17% 8% 1% +3.2 +22 78

CP2 98% 93% 90% 79% +32.5 +79 108

CP3 80% 10% - - +5.3 +11 10

CP4 94% 94% 77% 35% +18.8 +36 17

I/II 61% 28% 17% 11% +5.4 +19 18

-5 -10 -15 -20

$\lambda$ Boo 95% 65% 35% 20% -16.2 -35 20

Be 41% 12% 5% - -1.5 -19 59

**Table 3:** Limits in mmag for detecting the individual groups of objects. For example 49% of all CP1 stars can be detected with a 3 $\sigma$ limit of +5 mmag. In addition, the mean group $\overline {\Delta a}$ , the maximum values for group members $\Delta a_{\rm m}$ , and the number N of well-established members for the analysis are listed.
	+5	+10	+15	+20	$\overline {\Delta a}$	$\Delta a_{\rm m}$	N
CP1	49%	17%	8%	1%	+3.2	+22	78
CP2	98%	93%	90%	79%	+32.5	+79	108
CP3	80%	10%	-	-	+5.3	+11	10
CP4	94%	94%	77%	35%	+18.8	+36	17
I/II	61%	28%	17%	11%	+5.4	+19	18
	-5	-10	-15	-20
$\lambda$ Boo	95%	65%	35%	20%	-16.2	-35	20
Be	41%	12%	5%	-	-1.5	-19	59

Source LaTeX | All tables | In the text

	1 Introduction
	2 Selection, preparation, and homgenizationof the data
	3 Analyzing the sample
	4 Conclusions
	References
	Online Material