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