Back to the Abstract

	1 Introduction
	2 Observations and data reduction
	3 Faint galaxy counts at 12 m
	4 Modeling MIR galaxy counts per type with the code PÉGASE.3
	5 Results of galaxy count model at 12 m
	6 Galaxy count model at 24 m
	7 The cosmic star formation rate SFR(z) per type
	8 Discussion
	9 Conclusion
	References

	List of tables
	List of figures