TL;DR: A large survey of the sky has been undertaken in the near u.v. as discussed by the authors in two different steps by the Laboratoire d'Astronomie Spatiale du Centre National de la Recherche Scientifique: 1. A wide field camera 120 x 80° survey programme on rockets began in 1967 and was continued by the launch of the Janus camera in 1972.
Abstract: A large survey of the sky has been undertaken in the near u.v. in two different steps by the Laboratoire d’Astronomie Spatiale du Centre National de la Recherche Scientifique: 1. A wide field camera 120 x 80° survey programme on rockets began in 1967 and was continued by the launch of the Janus camera in 1972. 2. A medium field (6 x 8°) programme due to the S 183 French experiment on Skylab. The map shows the distribution of the S 183 fields on the celestial sphere, superposed with the two wide fields of the Janus camera (figure 1). A complementary work in visible light (H a) using similar wide field (60°) optics and very selective interference filters has been made during the same period in order to obtain an idea of the penetration in interstellar space of radiation below 912 A owing to ionization of the interstellar hydrogen considered as evidence of this radiation. The full set of these experiments in u.v. and H a gives a good synthetic figure of the extreme population I extension in the Milky Way.