This is a exercise question from Quantum Mechanic textbook by Bransden:
Using Wien's Law to show that if the spectral distribution function of black body radiation, $\rho(\lambda,T)$ is known at one temperature then it can be obtained at any temperature (so that a single curve can be used to represent black body radiation at all temperatures.
Wien's law being: $\rho(\lambda, T)=\lambda^{-5}f(\lambda T)$
I understand this question as that temperature $T$ only acts as a scalar to the $\lambda$ variable, so that the differentiation of Wien's Law with respect to $T$ will give a constant multiple to the whole function, but in fact it is not clear that this is true by examining only on the Wien's Law.
Any help would be appreciated.