The paper presents a survey of profiles of reasonably strong diffuse inters
tellar bands (DIBs) based on the extensive set of high-resolution spectra a
cquired with the aid of echelle spectrographs installed at the 2-m Terskol,
2-m Pic du Midi and 1-m SAO telescopes. The surveyed diffuse interstellar
bands cover the spectral ranges of blue and near-infrared, i.e the DIBs not
surveyed by Krelowski & Schmidt. The possible modifications caused by stel
lar and telluric lines are discussed. The very broad features such as 4430
are not discussed because the shapes of their profiles, extracted from eche
lle spectra, are very uncertain. The signal-to-noise (S/N) ratios of the sp
ectra are not high enough to enable discussion of the profiles of numerous
weak interstellar features discovered recently.