THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 96:605-626, 1995 February FAR-ULTRAVIOLET STELLAR PHOTOMETRY: FIELDS IN SAGITTARIUS AND SCORPIUS EDWARD G. SCHMIDT Division of Astronomical Sciences, National Science Foundation, 4201 Wilson Boulevard, Arlington, VA 22230; eschmidt@unlinfo.unl.edu AND GEORGE R. CARRUTHERS E.O. Hulburt Center for Space Research, Code 7609, Naval Research Laboratory, Washington, DC 20375-5320 ABSTRACT Far-ultraviolet photometry for 741 objects in a field in Sagittarius centered near M8 and 541 objects in a field centered near zeta Scorpii is presented. These data were extracted from electrographic images obtained with two cameras during a shuttle flight in 1991 April/May. The cameras provided band passes with lambda_eff = 1375 A and lambda_eff = 1781 A. Synthetic colors show that these bands are sensitive to effective temperature for hot stars. Our measurements were placed on a quantitative far-ultraviolet magnitude scale by convolving the spectra of stars observed by IUE with our cameras' spectral response functions. Fifty-eight percent of the ultraviolet objects were identified with visible stars using the SIMBAD database while another 40% of the objects are blends of early type stars too close together to separate with our resolution. Our photometry is compared with that from the TD-1, OAO 2, and ANS satellites and the S201 (Apollo 16) far-ultraviolet camera and found to agree at the level of a few tenths of a magnitude. Unlike previous studies, almost half of the identified visual counterparts to the ultraviolet objects are early B stars. A plot of distance modulus against ultraviolet color excess reveals a significant population of stars with strong ultraviolet excesses. Subject headings: stars: early-type -- surveys -- techniques: photometric -- ultraviolet: stars