Spatial correlation of the LSBGs (red dots) together with galaxies with spectroscopic measurements (blue stars) in the interval 0.003 < z < 0.008 to which the NGC 1052 environment belongs. Galaxies with spectroscopy are separated into two groups according to whether they have a magnitude greater or less than r = 12 mag. The shaded region marks the limit where an identification of LSBGs has not been carried out but galaxies with spectroscopy are included, for better characterization of the large-scale structure. A white background traces the density of galaxies with spectroscopy for ease of visualization.