Moffat distribution

Source: Wikipedia, the free encyclopedia.

The Moffat distribution, named after the

continuous probability distribution based upon the Lorentzian distribution. Its particular importance in astrophysics is due to its ability to accurately reconstruct point spread functions, whose wings cannot be accurately portrayed by either a Gaussian or Lorentzian
function.

Characterisation

Probability density function

The Moffat distribution can be described in two ways. Firstly as the distribution of a bivariate random variable (X,Y) centred at zero, and secondly as the distribution of the corresponding radii

In terms of the random vector (X,Y), the distribution has the
probability density function (pdf)
where and are
bivariate Student distribution
with zero correlation.

In terms of the random variable R, the distribution has density

Relation to other distributions

References