First Sentence:
The radio emission from supernovae (SNe) serves as an excellent, and often the only, probe of the final stages of the evolution of the massive progenitor star.
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Key Phrases - Statistically Improbable Phrases (SIPs):
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late light curves, positron escape, neutrino sphere, radio light curves, radio supernovae, circumstellar ring, radio afterglows, relativistic blast waves, young supernovae, early spectroscopy, accretion torus, supernova debris, shocked ejecta, explosion models, neutrino transport, optical afterglows, nebular phase, reverse shock, bolometric light curves, central absorption, early spectra, spherical explosion, progenitor star, progenitor models, early type galaxies
Key Phrases - Capitalized Phrases (CAPs):
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Della Valle, Space Sci, New York, Hubble Space Telescope, Monte Carlo, University of California, Very Large Array, Garden Street, National Facility, National Science Foundation, Oak Ridge, Osservatorio Astronomico, Space Telescope Science Institute, Australia Telescope Compact Array, Cambridge Univ, Enrico Cappellaro, Mark Sullivan, Office of Naval Research, Afterglow Era, Black-Hole-Forming Supernovae, Deep Radio Imaging, Edo Berger, Firenze Italy, Introduction Type, Italy Summary
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