**Table 17:** Metallicities, absolute magnitudes, (B-V)₀ colours, and effective temperatures from the Fourier parameters of the light curves for the subset of 29 RRab stars.
Id	Field	D_m	[Fe/H]	[Fe/H]	M_V	M_V	(B-V)₀	(B-V)₀	$\log T_{\rm eff}$
			(Fourier)	G04	(Fourier)	(this paper)	(Fourier)	(this paper)	(Fourier)
1408	B	$\leq$ 4.159	$-0.588\pm0.172$	$-1.70\pm 0.11$	0.495 $\pm$ 0.027	0.561	0.353	0.358	3.812
2249	B	$\leq$ 4.769	$-1.497\pm0.212$	$-1.56\pm 0.15$	0.520 $\pm$ 0.027	0.564	0.352	0.366	3.806
2525	A	$\leq$ 3	$-1.363\pm0.206$	$-2.06\pm 0.14$	0.513 $\pm$ 0.027	0.465	0.356	0.334	3.806
2884	B	$\leq$ 3	$-1.622\pm0.216$	$-1.90\pm 0.09$	0.507 $\pm$ 0.027	0.435	0.355	0.354	3.804
3054	B	$\leq$ 4.158	$-0.944\pm0.208$	-	0.729 $\pm$ 0.028	0.284	0.354	0.311	3.809
3400	B	$\leq$ 4.025	$-1.588\pm0.239$	$-1.45\pm 0.24$	0.624 $\pm$ 0.028	0.687	0.315	0.305	3.817
3412	B	$\leq$ 3	$-1.619\pm0.232$	-	0.572 $\pm$ 0.028	0.643	0.324	0.356	3.814
4540	B	$\leq$ 3.111	$-1.403\pm0.216$	-	0.544 $\pm$ 0.027	0.632	0.338	0.330	3.811
4974	A	$\leq$ 3	$-1.085\pm0.200$	$-1.35\pm 0.09$	0.611 $\pm$ 0.027	0.509	0.363	0.328	3.806
5167	A	$\leq$ 4.762	$-1.323\pm0.202$	-	0.553 $\pm$ 0.027	0.484	0.369	0.375	3.802
5902	B	$\leq$ 3	$-1.436\pm0.217$	$-2.12\pm 0.11$	0.531 $\pm$ 0.027	0.339	0.337	0.320	3.811
6398	A	$\leq$ 3	$-1.099\pm0.205$	$-1.40\pm 0.30$	0.587 $\pm$ 0.027	0.442	0.346	0.339	3.811
6426	A	$\leq$ 3.667	$-1.707\pm0.212$	$-1.59\pm 0.09$	0.404 $\pm$ 0.027	0.310	0.348	0.317	3.806
7247	A	$\leq$ 3	$-1.262\pm0.211$	$-1.41\pm 0.10$	0.601 $\pm$ 0.027	0.533	0.348	0.290	3.809
7325	A	$\leq$ 3	$-0.874\pm0.209$	$-1.28\pm 0.09$	0.684 $\pm$ 0.028	0.560	0.332	0.332	3.817
7468	A	$\leq$ 4.923	$-0.746\pm0.177$	-	0.626 $\pm$ 0.026	0.740	0.392	0.404	3.799
8094	A	$\leq$ 4.088	$-1.188\pm0.178$	$-1.83\pm 0.12$	0.460 $\pm$ 0.026	0.478	0.394	0.432	3.795
8220	A	$\leq$ 3.605	$-1.032\pm0.182$	-	0.496 $\pm$ 0.026	0.594	0.375	0.350	3.802
8720	A	$\leq$ 3	$-1.682\pm0.212$	$-1.76\pm 0.20$	0.365 $\pm$ 0.028	0.254	0.336	0.283	3.810
9494	A	$\leq$ 3.889	$-1.526\pm0.219$	$-1.69\pm 0.28$	0.505 $\pm$ 0.027	0.342	0.335	0.292	3.811
9660	A	$\leq$ 3.746	$-1.345\pm0.204$	-	0.580 $\pm$ 0.026	0.517	0.373	0.367	3.800
10 214	A	$\leq$ 4.261	$-0.314\pm0.165$	$-1.48\pm 0.12$	0.621 $\pm$ 0.027	0.329	0.374	0.332	3.807
12 896	A	$\leq$ 4.745	$-1.298\pm0.211$	$-1.53\pm 0.10$	0.564 $\pm$ 0.027	0.714	0.347	0.351	3.809
14 449	B	$\leq$ 4.877	$-1.483\pm0.216$	$-1.70\pm 0.13$	0.585 $\pm$ 0.027	0.732	0.357	0.370	3.805
18 314	A	$\leq$ 3	$-1.324\pm0.209$	$-1.71\pm 0.12$	0.487 $\pm$ 0.028	0.535	0.334	0.218	3.813
25 301	A	$\leq$ 3	$-1.095\pm0.204$	$-1.40\pm 0.18$	0.547 $\pm$ 0.027	0.891	0.336	0.396	3.814
25 362	A	$\leq$ 3	$-1.279\pm0.209$	$-1.49\pm 0.10$	0.509 $\pm$ 0.027	0.568	0.335	0.299	3.813
26 525	A	$\leq$ 3	$-1.887\pm0.245$	$-1.63\pm 0.12$	0.602 $\pm$ 0.028	0.598	0.329	0.368	3.811
26 821	A	$\leq$ 3	$-1.235\pm0.205$	$-1.37\pm 0.13$	0.606 $\pm$ 0.027	0.749	0.364	0.372	3.804

Note: The $\log T_{\rm eff}$ 's from the Fourier parameters are from the Fourier (B-V)₀ colours.

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