This paper introduces the use of pseudofilters that optimize the detection/
extraction of sources on a background. We assume as a first approach that s
uch sources are described by a spherical (central) profile and that the bac
kground is represented by a homogeneous and isotropic random field. We make
an n-dimensional treatment, placing emphasis on astrophysical applications
for spectra, images, and volumes, for the cases of exponential and Gaussia
n source profiles and scale-free power spectra to represent the background.