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The spectral index of a source, $\alpha$, is a measure of how the intensity changes with frequency as given by the power law distribution $S_\nu \propto \nu^{\alpha}$. A steep spectrum means that the intensity of the emission decreases rapidly with increasing frequency.
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1 erg = 10-7 Joules
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Flux density, $S_\nu$ is the incident flux received at a detector per unit area per unit frequency, at a frequency $\nu$. It has units of Janskys, where 1 Jy = $10^{-26} \mbox{ Wm}^{-2} \mbox{Hz}^{-1}$
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Tara Murphy
1999-10-31