Summary
Optical searches can detect supernovae (SNe) only if they suffer of a limited amount of dust extinction. This is a severe limitation as most of the core-collapse SNe could explode inside dusty regions. We describe a few ongoing projects aimed at detecting dusty SNe at near-IR wavelengths both in ground-based and HST images and to study their properties.
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© 2005 Springer-Verlag Berlin Heidelberg
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Mannucci, F., Cresci, G., Maiolino, R., Della Valle, M. (2005). The Infrared Supernova Rate. In: Marcaide, JM., Weiler, K.W. (eds) Cosmic Explosions. Springer Proceedings in Physics, vol 99. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26633-X_49
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DOI: https://doi.org/10.1007/3-540-26633-X_49
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-23039-7
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