Key points are not available for this paper at this time.
Context. Supernovae play an integral role in the feedback of processed material into the ISM of galaxies making them responsible for much of the chemical enrichment of the universe. The rate of supernovae can also reveal star formation histories. These rates are usually measured through the nonthermal radio continuum luminosity; however, a correlation between near-infrared FeII emission and supernova remnants has also been noted.
Rosenberg et al. (Mon,) studied this question.
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