Wavelengths, energy levels, ionization energies, line classifications, intensities and transition probabilities for Kr Vthrough Kr XXXVI, ;with the exception of Kr XIthrough Kr XVII, are tabulated. No data have been published for Kr XIthrough Kr XVII. These data are based on the energy levels compilation of Sugar and Musgrove [13]. Transition probabilities for selected M1 lines have been reported and are quoted here. A short review of the line identifications and wavelength measurements is given for each stage of ionization. The literature has been surveyed through February 1995.