Back to the Abstract

	1 Introduction
	2 The data
	3 The spectral energy distributions
	4 The IR luminosities and Star Formation Rates
	5 Cluster sources
	6 Field sources
	7 The Butcher-Oemler effect
	8 Discussion
	9 Summary and conclusions
	References
	Online Material
	Appendix A: The SED fitting procedure
	Appendix B: Notes on individual sources

	List of tables
	List of figures