SIMBAD references

Based upon 33A/mm dispersion spectroscopic material we examine if equivalent widths of H and He lines can be used for the detection of new helium-peculiar stars. The answer is affirmative and we present some new candidates discovered this way. We have also investigated if the use of different helium lines than those of the ³D series (4026, 4471) modifies the assignments of helium peculiar stars. This is not the case, since the use of λ6678 (¹D) and λ7065 (3S) gives the same results.