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Springer Verlag, Springer Proceedings in Physics, p. 355-359

DOI: 10.1007/3-540-26633-x_49

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The Infrared Supernova Rate

Journal article published in 2003 by F. Mannucci, G. Cresci ORCID, R. Maiolino, M. Della Valle
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

Optical searches can only detect supernovae with 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.