Abstract
The spectra of Se V and Br VI were photographed in the 2000 Å-200 Å and 1200 Å-200 Å regions on a variety of spectrographs using a triggered spark light source. The new observations have lead to revision and extension of earlier analyses. The 4s2, 4s4p, 4p2, 4s4d, 4s5s and 4s5p configurations have been confirmed in both Se V and Br VI. In addition, the 4s5d and 4s6s configurations have been established in Se V. Fifty-three lines have been classified in Se V and forty-nine lines have been classified in Br VI.
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