Energy distribution data on 238 secondary standard stars in the range 3200-7600{AA} with a 50{AA} step are presented. These stars are common to the Catalogue of the Sternbergh State Astronomical Institute and to the Fessenkov Astrophysical Institute (Alma-Ata). For these stars, the differences between the two catalogues do not exceed 5%, and the mean internal accuracy of both catalogue data in this wavelength range are about 3.5%. For 99 stars, the energy distribution in the near infra-red (6000-10800{AA}) are also presented.