The Infrared Supernova Rate

@article{Mannucci2005TheIS,
  title={The Infrared Supernova Rate},
  author={Filippo Mannucci and Giovanni Cresci and Roberto Maiolino and Massimo Della Valle},
  journal={arXiv: Astrophysics},
  year={2005},
  pages={355-359}
}
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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