Table 1: Basic data for the three new eclipsing binaries. An average I-band magnitude $\bar{m}_I$ is calculated from the OGLE-III time-series photometry of N observations over six Galactic Bulge seasons. The epoch of primary minimum E₀ is also given. The current zeropoint of $\bar{m}_I$ is roughly calibrated to an uncertainty of $\sim$ 0.1-0.2 mag.
PN G Name RA (J2000) Dec (J2000) OGLE field E₀ (HJD-2 450 000) P (days) $\bar{m}_I$ N

359.1-02.3 M 3-16 17 52 46.1 -30 49 35 BLG180.1 3850.9184 $\pm$ 0.0015 0.573648 $\pm$ 0.000020 15.93 1039

357.6-03.3 H 2-29 17 53 16.8 -32 40 38 BLG155.1 3619.5208 $\pm$ 0.0025 0.244110 $\pm$ 0.000005 18.12 609

000.2-01.9 M 2-19 17 53 45.6 -29 43 46 BLG101.3 4224.7822 $\pm$ 0.0035 0.670170 $\pm$ 0.000020 15.87 1273

**Table 1:** Basic data for the three new eclipsing binaries. An average I-band magnitude $\bar{m}_I$ is calculated from the OGLE-III time-series photometry of N observations over six Galactic Bulge seasons. The epoch of primary minimum E₀ is also given. The current zeropoint of $\bar{m}_I$ is roughly calibrated to an uncertainty of $\sim$ 0.1-0.2 mag.
PN G	Name	RA (J2000)	Dec (J2000)	OGLE field	E₀ (HJD-2 450 000)	P (days)	$\bar{m}_I$	N
359.1-02.3	M 3-16	17 52 46.1	-30 49 35	BLG180.1	3850.9184 $\pm$ 0.0015	0.573648 $\pm$ 0.000020	15.93	1039
357.6-03.3	H 2-29	17 53 16.8	-32 40 38	BLG155.1	3619.5208 $\pm$ 0.0025	0.244110 $\pm$ 0.000005	18.12	609
000.2-01.9	M 2-19	17 53 45.6	-29 43 46	BLG101.3	4224.7822 $\pm$ 0.0035	0.670170 $\pm$ 0.000020	15.87	1273

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