The result of the Photometric observations of UAI campaign, was published in Minor Planet Bulletin 46-3.

The result of the UAI campaign was published in Minor Planet Bulletin 46-3. Photometric observations of four main-belt asteroids were made in order to acquire lightcurves for shape/spin axis models. The synodic period and lightcurve amplitude were found for: 224 Oceana: 9.404 ± 0.001 h, 0.10 mag; 359 Georgia: 5.5329 ± 0.0001 h, 0.14 mag.; 1453 Fennia: 4.4120 ± 0.0002 h, 0.14 mag; and 1717 Arlon: 5.1448 ± 0.0004 h, 0.10 mag. We also confirmed previous discoveries of a satellite for 1453 Fennia and 1717 Arlon. 

MPC 46-3, pages 350-352