Table 16: Fourier parameters of the light curves and corresponding estimate of the star metallicity, absolute magnitude, intrinsic (B-V)0 colour, and effective temperature.
Star P $\langle B-V\rangle_{\rm int}$ A1 A2 A3 A4 A5 A6 A7 A8
7325 0.48677 0.410 0.34815 0.18973 0.13552 0.09432 0.05650 0.04252 0.01980 0.01321
      $\Phi_{21}$ $\Phi_{31}$ $\Phi_{41}$ $\Phi_{51}$ $\Phi_{61}$ $\Phi_{71}$ $\Phi_{81}$  
      3.94169 1.90815 6.15817 4.23861 2.16828 0.40072 4.83247  
                     
      df1 df2 df3 df4 df5      
      1.414 0.909 0.352 1.388 2.824      
                     
      df21 df31 df41 df51        
      0.661 0.757 0.894 0.501        
                     
[Fe/H] MV (B-V)0 $ \log T_{\rm eff}(B-V)$              
                     
-0.874 0.684 0.332 3.817              
Table 16 is presented in its entirety in the electronic edition of the Journal.
A portion is shown here for guidance regarding its form and content.

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Article Contents
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
List of tables
List of figures