Table 2: Probabilities $\eta _{\rm F}$ and $\eta _{\rm C}$ for the stars to have respectively a background object with a magnitude in K-band similar to the one of their CC in the SHARPII camera field of view ( $12.7''\times 12.7''$ ) and within a circle with a radius as large as the CC separation.
Source l. b $\eta _{\rm F}$ $\eta _{\rm C}$

( $^{\circ}$ ) ( $^{\circ}$ ) (%) (%)

HIP 108422 322.86 -41.56 <1 <0.1

HIP 1910 308.43 -54.65 <1 <0.1

GSC 8047-0232 282.73 -62.35 $\sim$ 2 $\sim$ 0.4

HIP 6856 290.37 -63.58 $\sim$ 5 $\sim$ 2

**Table 2:** Probabilities $\eta _{\rm F}$ and $\eta _{\rm C}$ for the stars to have respectively a background object with a magnitude in K-band similar to the one of their CC in the SHARPII camera field of view ( $12.7''\times 12.7''$ ) and within a circle with a radius as large as the CC separation.
Source	l.	b	$\eta _{\rm F}$	$\eta _{\rm C}$
	( $^{\circ}$ )	( $^{\circ}$ )	(%)	(%)
HIP 108422	322.86	-41.56	<1	<0.1
HIP 1910	308.43	-54.65	<1	<0.1
GSC 8047-0232	282.73	-62.35	$\sim$ 2	$\sim$ 0.4
HIP 6856	290.37	-63.58	$\sim$ 5	$\sim$ 2

Source LaTeX | All tables | In the text