Table 12: Comparison with MACHO photometry for the non-variable stars with V < 18.25, from Alves subsample.
Bin $\langle \Delta V\rangle $ $\sigma$ N
Field A
15.00-17.00 0.045 0.021 64
17.00-17.25 0.055 0.031 34
17.25-17.50 0.043 0.011 31
17.50-17.75 0.037 0.027 58
17.75-18.00 0.038 0.021 81
18.00-18.25 0.045 0.025 88
Field B
15.00-17.00 0.026 0.029 61
17.00-17.25 0.022 0.037 36
17.25-17.50 0.027 0.041 29
17.50-17.75 0.011 0.031 30
17.75-18.00 0.012 0.029 57
18.00-18.25 0.010 0.022 62

Notes: $\langle \Delta V\rangle = \langle V_{\rm this~paper}-V_{\rm Alves}\rangle$.

Source LaTeX | All tables | In the text

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