Table 12: Differential LTPV photometry of HD 168112. The quoted magnitudes and 1- $\sigma$ dispersions correspond to the difference A 5020 - B 5020 (where A 5020 is the magnitude of HD 168112 and B 5020 that of HD 168135). The first column yields the code of the telescope + instrument configuration (see Manfroid et al. 1991) and the second column indicates the number of data points for each set-up.
Telescope N u v b y

5 26 $0.780 \pm 0.011$ $1.205 \pm 0.005$ $0.976 \pm 0.004$ $0.570 \pm 0.005$

6 39 $0.747 \pm 0.053$ $1.192 \pm 0.012$ $0.962 \pm 0.008$ $0.568 \pm 0.010$

7 30 $0.873 \pm 0.010$ $1.252 \pm 0.010$ $0.966 \pm 0.010$ $0.580 \pm 0.009$

**Table 12:** Differential LTPV photometry of HD 168112. The quoted magnitudes and 1- $\sigma$ dispersions correspond to the difference A 5020 - B 5020 (where A 5020 is the magnitude of HD 168112 and B 5020 that of HD 168135). The first column yields the code of the telescope + instrument configuration (see Manfroid et al. 1991) and the second column indicates the number of data points for each set-up.
Telescope	N	u	v	b	y
5	26	$0.780 \pm 0.011$	$1.205 \pm 0.005$	$0.976 \pm 0.004$	$0.570 \pm 0.005$
6	39	$0.747 \pm 0.053$	$1.192 \pm 0.012$	$0.962 \pm 0.008$	$0.568 \pm 0.010$
7	30	$0.873 \pm 0.010$	$1.252 \pm 0.010$	$0.966 \pm 0.010$	$0.580 \pm 0.009$

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