Back to the Abstract


Article Contents
1 Introduction
2 Importance of the SN rate per unit mass
3 SN catalog
4 The near-infrared magnitudes
5 Galaxy mass
6 The SN rate as a function of the morphology of the host galaxy
7 The SN rate as a function of the galaxy colors
8 Discussion
References

List of tables
List of figures

Copyright ESO 2005
Published by EDP Sciences