Ultraviolet stellar fluxes have been presented for 140 bright stars in the spectral region from 1200 A to 3600 Å in a graphical and tabular form (A. D. Code and M. R. Meade, 1976). The spectra represent a subset of 0A0-2 spectrometer data on file at the National Space Science Data Center. The monochromatic flux is given in units of ergs cm−2 sec−1 Å−1 with a spectral resolution of about 22 Angstroms in the region from 3600 Å to 1850 Å and approximately 12 Angstroms from 1850 Å to 1160 Å.The monochromatic flux, Fλ, is based upon the absolute calibration described by Bless, Code and Fairchild (1976).
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