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Article Contents
1 Introduction
2 The galaxy sample
3 Observations
4 SN detection method, limiting magnitudes, and the SNe detections
5 Computing the infrared SN rate
6 The K-band light curve of the core-collapse SN
7 SN rate and FIR luminosity
8 The role of type Ia SNe
9 The infrared SN rate
10 Comparison between expected and detected SN rates
11 Summary and conclusions
Appendix A: The spatial dimension of the starburst activity

Copyright ESO 2003
Published by EDP Sciences