Although the galaxy distribution is observed to be scale invariant at
some scales, it cannot be identified to a perfect fractal which is a m
athematical idealization. In this letter we illustrate, by a simple ex
ample, the fact that discretisation and finite sampling effects modify
the expected properties of a fractal-like distribution : sampling an
ideal fractal by a finite sequence of independent observations, we obt
ain a Poisson distribution on a fractal. Analyzing its main properties
, with emphasis on number counts probabilities and mean N-points corre
lation functions, we illustrate these effects. Alhough this is not int
ended to modelize the galaxy distribution, we point out some similarit
ies which justify the interest of this distribution for tests on stati
stical methods.