Back to the Abstract

	1 Introduction
	2 Early dark energy cosmologies
	3 The thermal SZ effect
	4 Creation of full-sky SZ maps
	5 Simulating SZ observations by Planck
	6 The filtering
	7 Results
	8 Summary and conclusions
	Appendix A: Impact of noise levels to the filter performance
	References

	List of tables
	List of figures