Problems in the analysis of the XCOV4 data for AM CVn (HZ 29)

Articles in the same Issue

1. Titelei
2. Contents
3. List of Participants
4. Introduction
5. R.E. Nather - the founder of the WET
6. Musings on the Whole Earth Telescope
7. The WET from outside Texas
8. A third world view of, and approach to, some WET problems
9. A brief report on WET observations from India
10. Review of the 1991 WET Workshop
11. The pulsation properties of the DA white dwarf variables
12. Progress report on the analysis of the WET campaign on RXJ 2117+3412
13. Inside GD 358
14. Whole Earth Telescope data on G 117-B15A and G 226-29
15. Problems in the analysis of the XCOV4 data for AM CVn (HZ 29)
16. AM CVn - finally solved? Results of XCOV4, March 1990
17. Extending the WET technique to lower frequencies
18. Some Central Asian Observatories for the WET
19. Reduction of simultaneous photometric data or how to make a bigger telescope
20. Microsatellites for communication with remote places
21. Autoguider at Mt. Suhora Observatory
22. Improvements of the Pancake travelling photometer
23. Update on extensions to the Texas interface
24. Some components of photometric equipment for the WET project
25. The QED data reduction program
26. Whole Earth Telescope data analysis
27. A comparison of the prewhite and clean procedures to find the real frequencies
28. The several peaks deconvolution method
29. Methods of asteroseismology for white dwarf stars
30. Appendix 1: Variable white dwarf data tables (September 23, 1993 Version)
31. Appendix 2: WET Business Meeting