Table 6: Data for objects with no detected signal in the CCF. N: number of measurements, $\sigma _{\rm CCF}$ : rms of the CCF continuum, ${\it SNR}$ : signal-to-noise ratio of the spectrum, $v^{\min}_{\sin i}$ : minimum projected rotation velocity compatible with the absence of CCF signal for a single, late-type star.
Name N rms $_{\rm CCF}$ ${\it SNR}$ $v^{\min}_{\sin i}$

[%] [km s^-1]

OGLE-TR-68 1 0.9 3 19

OGLE-TR-82 1 1.2 <1 -

OGLE-TR-84 1 0.6 4 34

OGLE-TR-89 1 0.5 7 49

OGLE-TR-107 1 0.6 4 32

OGLE-TR-118 3 0.4 6 53

OGLE-TR-127 1 0.2 15 119

**Table 6:** Data for objects with no detected signal in the CCF. N: number of measurements, $\sigma _{\rm CCF}$ : rms of the CCF continuum, ${\it SNR}$ : signal-to-noise ratio of the spectrum, $v^{\min}_{\sin i}$ : minimum projected rotation velocity compatible with the absence of CCF signal for a single, late-type star.
Name	N	rms $_{\rm CCF}$	${\it SNR}$	$v^{\min}_{\sin i}$
		[%]		[km s^-1]
OGLE-TR-68	1	0.9	3	19
OGLE-TR-82	1	1.2	<1	-
OGLE-TR-84	1	0.6	4	34
OGLE-TR-89	1	0.5	7	49
OGLE-TR-107	1	0.6	4	32
OGLE-TR-118	3	0.4	6	53
OGLE-TR-127	1	0.2	15	119

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and reductions
	3 Analysis
	4 Results
	5 Discussion
	References
	Online Material