In astronomy, the spectral index of a source is a measure of the dependence of radiative flux density on frequency. Given frequency
Note that if flux does not follow a power law in frequency, the spectral index itself is a function of frequency. Rearranging the above, we see that the spectral index is given by
Spectral index is also sometimes defined in terms of wavelength
and at a given frequency, spectral index may be calculated by taking the derivative
The opposite sign convention is sometimes employed, in which the spectral index is given by
The spectral index of a source can hint at its properties. For example, using the positive sign convention, a spectral index of 0 to 2 at radio frequencies indicates thermal emission, while a steep negative spectral index typically indicates synchrotron emission.
Spectral Index of Thermal emission
At radio frequencies (i.e. in the low-frequency, long-wavelength limit), where the Rayleigh–Jeans law is a good approximation to the spectrum of thermal radiation, intensity is given by
Taking the logarithm of each side and taking the partial derivative with respect to
Using the positive sign convention, the spectral index of thermal radiation is thus