Table 3: Coordinates and magnitudes of the comparison stars.
Id $\alpha_{2000}$ $\delta_{2000}$ V n_V B n_B I n_I

Field A

1253 5 22 57.93 -70 31 31.96 $16.889\pm0.026$ 14 $17.575\pm0.045$ 14 $16.102\pm0.025$ 14

Field B

128 5 16 29.75 -71 01 46.62 $16.194\pm0.023$ 15 $16.888\pm0.037$ 14 $15.410\pm0.035$ 14

**Table 3:** Coordinates and magnitudes of the comparison stars.
Id	$\alpha_{2000}$	$\delta_{2000}$	V	n_V	B	n_B	I	n_I
Field A
1253	5 22 57.93	-70 31 31.96	$16.889\pm0.026$	14	$17.575\pm0.045$	14	$16.102\pm0.025$	14
Field B
128	5 16 29.75	-71 01 46.62	$16.194\pm0.023$	15	$16.888\pm0.037$	14	$15.410\pm0.035$	14

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