Table 15: Comparison of our and OGLE II photometry for the non variable stars in common. $\langle \Delta V\rangle$ , $\langle \Delta B\rangle$ , $\langle \Delta I\rangle$ are: this paper - OGLE II.
Bin $\langle \Delta V\rangle$ $\sigma_{V}$ N Bin $\langle \Delta B\rangle$ $\sigma_{B}$ N Bin $\langle \Delta I\rangle$ $\sigma_{I}$ N

15.00-17.00 0.045 0.017 64 16.00-17.00 0.014 0.036 16 14.00-15.00 0.063 0.053 35

17.00-17.25 0.044 0.027 60 17.00-17.50 -0.006 0.091 22 15.00-16.00 0.070 0.044 129

17.25-17.50 0.044 0.021 76 17.50-18.00 0.009 0.027 24 16.00-17.00 0.056 0.040 300

17.50-17.75 0.044 0.023 96 18.00-18.25 0.025 0.036 28 17.00-17.50 0.052 0.042 273

17.75-18.00 0.043 0.025 107 18.25-18.50 0.011 0.036 51 17.50-18.00 0.042 0.033 368

18.00-18.25 0.048 0.028 122 18.50-18.75 0.017 0.032 88 18.00-18.25 0.040 0.037 626

18.25-18.50 0.048 0.026 174 18.75-19.00 0.022 0.030 149 18.25-18.50 0.055 0.045 1040

18.50-18.75 0.043 0.021 194 19.90-19.25 0.026 0.034 161 18.50-18.75 0.052 0.049 479

18.75-19.00 0.049 0.026 250 19.25-19.50 0.031 0.038 218 18.75-19.00 0.043 0.054 344

19.00-19.25 0.049 0.030 628 19.50-19.75 0.034 0.030 330 19.00-19.50 0.045 0.062 966

19.25-19.50 0.062 0.032 1105 19.75-20.00 0.032 0.042 524 19.50-19.75 0.027 0.080 723

19.50-19.75 0.069 0.036 579 20.00-20.25 0.026 0.049 1115 19.75-20.00 0.031 0.091 1008

19.75-20.00 0.068 0.044 510 20.25-20.50 0.044 0.047 1125 20.00-20.25 0.035 0.113 1340

20.00-20.25 0.067 0.051 611 20.50-20.75 0.035 0.063 864

20.25-20.50 0.073 0.063 838 20.75-21.00 0.039 0.066 944

21.00-21.25 0.038 0.082 1046

**Table 15:** Comparison of our and OGLE II photometry for the non variable stars in common. $\langle \Delta V\rangle$ , $\langle \Delta B\rangle$ , $\langle \Delta I\rangle$ are: this paper - OGLE II.
Bin	$\langle \Delta V\rangle$	$\sigma_{V}$	N	Bin	$\langle \Delta B\rangle$	$\sigma_{B}$	N	Bin	$\langle \Delta I\rangle$	$\sigma_{I}$	N
15.00-17.00	0.045	0.017	64	16.00-17.00	0.014	0.036	16	14.00-15.00	0.063	0.053	35
17.00-17.25	0.044	0.027	60	17.00-17.50	-0.006	0.091	22	15.00-16.00	0.070	0.044	129
17.25-17.50	0.044	0.021	76	17.50-18.00	0.009	0.027	24	16.00-17.00	0.056	0.040	300
17.50-17.75	0.044	0.023	96	18.00-18.25	0.025	0.036	28	17.00-17.50	0.052	0.042	273
17.75-18.00	0.043	0.025	107	18.25-18.50	0.011	0.036	51	17.50-18.00	0.042	0.033	368
18.00-18.25	0.048	0.028	122	18.50-18.75	0.017	0.032	88	18.00-18.25	0.040	0.037	626
18.25-18.50	0.048	0.026	174	18.75-19.00	0.022	0.030	149	18.25-18.50	0.055	0.045	1040
18.50-18.75	0.043	0.021	194	19.90-19.25	0.026	0.034	161	18.50-18.75	0.052	0.049	479
18.75-19.00	0.049	0.026	250	19.25-19.50	0.031	0.038	218	18.75-19.00	0.043	0.054	344
19.00-19.25	0.049	0.030	628	19.50-19.75	0.034	0.030	330	19.00-19.50	0.045	0.062	966
19.25-19.50	0.062	0.032	1105	19.75-20.00	0.032	0.042	524	19.50-19.75	0.027	0.080	723
19.50-19.75	0.069	0.036	579	20.00-20.25	0.026	0.049	1115	19.75-20.00	0.031	0.091	1008
19.75-20.00	0.068	0.044	510	20.25-20.50	0.044	0.047	1125	20.00-20.25	0.035	0.113	1340
20.00-20.25	0.067	0.051	611	20.50-20.75	0.035	0.063	864
20.25-20.50	0.073	0.063	838	20.75-21.00	0.039	0.066	944
				21.00-21.25	0.038	0.082	1046

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and reductions
	3 Identification of the variable stars
	4 A star by star comparison with MACHO and OGLE II photometries
	5 The pulsation characteristics of the RR Lyrae stars
	6 Fourier decomposition of the light curves
	Appendix A: Atlas of the light curves
	References
	Online Material