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

List of tables
List of figures

Copyright ESO 2007
Published by EDP Sciences