  Heisenberg's uncertainty principle tells us that it is impossible to
determine simultaneously the position of a photon crossing a telescope's
aperture and its momentum. Super-resolution imaging techniques rely on
modification of the observed sample, or on entangling photons. In astronomy we
have no access to the object, but resolution may be improved by optical
amplification. Unfortunately, spontaneous emission contributes noise and
negates the possible gain from stimulated emissions. We show that it is
possible to increase the weight of the stimulated photons by considering photon
statistics, and observe an improvement in resolution. Most importantly, we
demonstrate a method which can apply for all imaging purposes.
