Table 3: Parameters from the transit light curve fit: $\overline {r}$ ratio of the radii of the primary and secondary bodies, V_T/R transit velocity in units of the radius of the primary, b impact parameter, P revised period according to the radial velocity measurements. We deliberately do not provide the results for the 4 unsolved cases suspected to be false positives, OGLE-TR-19, 48, 49 and 58. For the two cases of SB2, stellar parameters were deduced from the spectroscopic orbits and the rotational velocities.
Name $\overline {r}$ V_T/R b $[b_{\rm down}-b_{\rm up}]$ P

[days^-1] [days]

5 0.189 $\pm$ 0.008 22.70 $\pm$ 1.9 0.56 [0.47-0.65] 0.80827

6 0.198 $\pm$ 0.006 9.76 $\pm$ 0.44 0.20 [0.00-0.21] 4.54881

7 0.172 $\pm$ 0.006 13.58 $\pm$ 0.50 0.02 [0.00-0.09] 2.71782

8 - - 1.65 [1.62-1.68] 5.43284

10 0.129 $\pm$ 0.007 16.80 $\pm$ 1.22 0.45 [0.00-0.46] 3.10140

12 0.299 [0.26-0.74] 8.44 $\pm$ 0.83 1.02 [0.89-1.32] 8.65725

17 0.245 [0.22-0.63] 8.27 $\pm$ 0.56 0.90 [0.72-1.28] 13.87370

18 0.200 $\pm$ 0.020 11.78 $\pm$ 0.83 0.77 [0.73-0.87] 2.22803

19 - - - - -

33 0.160 $\pm$ 0.015 12.20 $\pm$ 1.25 0.68 [0.59-0.77] 1.95326

34 0.188 $\pm$ 0.002 6.83 $\pm$ 0.40 0.00 [0.00-0.02] 8.57633

35 - - 1.68 [1.65-1.73] 2.51957

48 - - - - -

49 - - - - -

55 0.109 [0.107-0.150] 16.45 [9.21-18.72] 0.60 [0.00-0.85] 3.18454

56 0.114 $\pm$ 0.004 22.84 [22.43-27.27] 0.69 [0.50-0.69] 1.21192

58 - - - - -

59 0.257 $\pm$ 0.089 10.238 $\pm$ 0.632 0.99 [0.82-1.31] 2.99432

**Table 3:** Parameters from the transit light curve fit: $\overline {r}$ ratio of the radii of the primary and secondary bodies, V_T/R transit velocity in units of the radius of the primary, b impact parameter, P revised period according to the radial velocity measurements. We deliberately do not provide the results for the 4 unsolved cases suspected to be false positives, OGLE-TR-19, 48, 49 and 58. For the two cases of SB2, stellar parameters were deduced from the spectroscopic orbits and the rotational velocities.
Name	$\overline {r}$	V_T/R	b	$[b_{\rm down}-b_{\rm up}]$	P
		[days^-1]			[days]
5	0.189 $\pm$ 0.008	22.70 $\pm$ 1.9	0.56	[0.47-0.65]	0.80827
6	0.198 $\pm$ 0.006	9.76 $\pm$ 0.44	0.20	[0.00-0.21]	4.54881
7	0.172 $\pm$ 0.006	13.58 $\pm$ 0.50	0.02	[0.00-0.09]	2.71782
8	-	-	1.65	[1.62-1.68]	5.43284
10	0.129 $\pm$ 0.007	16.80 $\pm$ 1.22	0.45	[0.00-0.46]	3.10140
12	0.299 [0.26-0.74]	8.44 $\pm$ 0.83	1.02	[0.89-1.32]	8.65725
17	0.245 [0.22-0.63]	8.27 $\pm$ 0.56	0.90	[0.72-1.28]	13.87370
18	0.200 $\pm$ 0.020	11.78 $\pm$ 0.83	0.77	[0.73-0.87]	2.22803
19	-	-	-	-	-
33	0.160 $\pm$ 0.015	12.20 $\pm$ 1.25	0.68	[0.59-0.77]	1.95326
34	0.188 $\pm$ 0.002	6.83 $\pm$ 0.40	0.00	[0.00-0.02]	8.57633
35	-	-	1.68	[1.65-1.73]	2.51957
48	-	-	-	-	-
49	-	-	-	-	-
55	0.109 [0.107-0.150]	16.45 [9.21-18.72]	0.60	[0.00-0.85]	3.18454
56	0.114 $\pm$ 0.004	22.84 [22.43-27.27]	0.69	[0.50-0.69]	1.21192
58	-	-	-	-	-
59	0.257 $\pm$ 0.089	10.238 $\pm$ 0.632	0.99	[0.82-1.31]	2.99432

Source LaTeX | All tables | In the text

	1 Introduction
	2 Target selection and observations
	3 Spectroscopic analysis
	4 Light curve analysis
	5 Results
	6 Discussion and conclusion
	References