Table 2: Log of the observations of $\delta$ Vel with NACO in the NB2.17 filter. MJD^* is the average modified Julian date minus 54 000, HJD^* the heliocentric Julian date minus 2 454 000 and $\phi$ is the phase of the eclipsing binary (see text). N is the number of frames. As in Table 1, $\theta$ is the seeing in the visible and AM is the airmass. The listed figures are median values over the observations.
# MJD^* HJD^* $\phi$ (Min I) N exp. $\theta$ ( $\hbox{$^{\prime\prime}$ }$ ) AM

1 557.0224 557.5245 0.9582 51 0.80 1.157

2 560.9976 561.4996 0.0463 46 0.91 1.164

3 562.0121 562.5141 0.0687 51 0.67 1.156

4 563.0048 563.5067 0.0907 51 0.89 1.158

5 576.9715 577.4732 0.4000 51 0.66 1.156

6 579.0231 579.5247 0.4455 50 1.06 1.191

7 580.9917 581.4932 0.4891 51 1.24 1.164

8 591.9748 592.4761 0.7323 51 0.59 1.175

9 593.9732 594.4744 0.7766 50 0.77 1.180

10 604.0442 604.5450 0.9996 49 0.76 1.479

**Table 2:** Log of the observations of $\delta$ Vel with NACO in the NB2.17 filter. MJD^* is the average modified Julian date minus 54 000, HJD^* the heliocentric Julian date minus 2 454 000 and $\phi$ is the phase of the eclipsing binary (see text). N is the number of frames. As in Table 1, $\theta$ is the seeing in the visible and AM is the airmass. The listed figures are median values over the observations.
#	MJD^*	HJD^*	$\phi$ (Min I)	N exp.	$\theta$ ( $\hbox{$^{\prime\prime}$ }$ )	AM
1	557.0224	557.5245	0.9582	51	0.80	1.157
2	560.9976	561.4996	0.0463	46	0.91	1.164
3	562.0121	562.5141	0.0687	51	0.67	1.156
4	563.0048	563.5067	0.0907	51	0.89	1.158
5	576.9715	577.4732	0.4000	51	0.66	1.156
6	579.0231	579.5247	0.4455	50	1.06	1.191
7	580.9917	581.4932	0.4891	51	1.24	1.164
8	591.9748	592.4761	0.7323	51	0.59	1.175
9	593.9732	594.4744	0.7766	50	0.77	1.180
10	604.0442	604.5450	0.9996	49	0.76	1.479

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