Table 2: First entries in the electronically available table, which lists: OGLE-name, oribital period, and time used to define phase zero.
OGLE name Period (d) Ta
bul_sc01_0053 2.521648 530.819
bul_sc01_0108 1.532373 550.789
bul_sc01_0202 4.513265 535.895
bul_sc01_0257 2.378940 540.765
bul_sc01_0422 4.201144 530.836
bul_sc01_0424 1.738786 530.836
bul_sc01_0426 4.236257 530.819
bul_sc01_0487 1.782421 550.789
bul_sc01_0552 2.049995 550.789
bul_sc01_0616 1.761581 530.837
bul_sc01_0691 3.350188 535.895
bul_sc01_0696 1.329869 550.789
bul_sc01_0738 1.427248 540.765
bul_sc01_0777 1.578524 550.789
bul_sc01_0778 1.107325 540.765
bul_sc01_0851 8.904982 550.789
a T = (JD-2 450 000) used to define zero phase in Fig. 1.
First entries only. Complete table available in electronic form at the CDS.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 The data sets
3 Analysis of the lightcurve shape and selecting eclipsing binaries
4 Results
5 Summary
References
Online Material
Appendix A: The model
Appendix B: Newly discovered eclipsing binaries in the Magellanic Clouds
List of tables
List of figures