Table 5: Informations and average quantities for the variable stars in field A.
Id   $\alpha$ $\delta$ Type     P    Epoch Np    $\langle {V_{\rm int}}\rangle$ $\langle {B_{\rm int}}\rangle$ $\langle {I_{\rm int}}\rangle$ $\langle {V_{\rm mag}}\rangle$ $\langle {B_{\rm mag}}\rangle$ $\langle {I_{\rm mag}}\rangle$ A_V A_B A_I   Notes

(2000) (2000) (days) (-2 400 000) (V,B,I) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag)

1731 5:23:38.69 -70:31:08.17 ab 0.58245 51 183.63490 6, 14, - - - - - - -   - 1.100:   - Incomplete

2525 5:23:32.39 -70:39:15.34 ab 0.61615 51 933.57692 69, 41, - 19.340 19.764 - 19.376 19.826 - 0.991 1.272   -

2767 5:23:17.70 -70:38:55.90 ab 0.53106 51 183.52271 64, 33, - 19.467 19.874 19.074 19.517 19.962 19.089 1.091 1.363   -

3061 5:23:25.13 -70:38:28.94 ab 0.47622 51 182.69038 66, 41, 11 19.631 20.037 19.220 19.679 20.121 19.239 0.809 1.093 0.765 Blazhko

3805 5:24:04.69 -70:37:18.42 ab 0.62740 51 185.78000 60, 37, 10 19.402 19.866 18.850 19.415 19.889 18.848 0.623 0.805 0.345

**Table 5:** Informations and average quantities for the variable stars in field A.
Id	$\alpha$	$\delta$	Type	P	Epoch	Np	$\langle {V_{\rm int}}\rangle$	$\langle {B_{\rm int}}\rangle$	$\langle {I_{\rm int}}\rangle$	$\langle {V_{\rm mag}}\rangle$	$\langle {B_{\rm mag}}\rangle$	$\langle {I_{\rm mag}}\rangle$	A_V	A_B	A_I	Notes
	(2000)	(2000)		(days)	(-2 400 000)	(V,B,I)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
1731	5:23:38.69	-70:31:08.17	ab	0.58245	51 183.63490	6, 14, -	-	-	-	-	-	-	-	1.100:	-	Incomplete
2525	5:23:32.39	-70:39:15.34	ab	0.61615	51 933.57692	69, 41, -	19.340	19.764	-	19.376	19.826	-	0.991	1.272	-
2767	5:23:17.70	-70:38:55.90	ab	0.53106	51 183.52271	64, 33, -	19.467	19.874	19.074	19.517	19.962	19.089	1.091	1.363	-
3061	5:23:25.13	-70:38:28.94	ab	0.47622	51 182.69038	66, 41, 11	19.631	20.037	19.220	19.679	20.121	19.239	0.809	1.093	0.765	Blazhko
3805	5:24:04.69	-70:37:18.42	ab	0.62740	51 185.78000	60, 37, 10	19.402	19.866	18.850	19.415	19.889	18.848	0.623	0.805	0.345

Table 5 is presented in its entirety in the electronic edition of the Journal. A portion is shown here for guidance regarding its form and content.

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