Photometric measurements of 352 Gisela during December 1999 were used to produce a light curve showing a sinodic rotation period of 7.49±0.01h with a brightness variation of 0.32 in magnitude.[7] This period estimate was refined to 7.4796±0.0002h in 2012.[4]
↑Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, 34 (4): 113–119, Bibcode:2007MPBu...34..113W.
↑Lazar, S.; etal. (June 2001), "Lightcurves and Rotation Periods for Minor Planets (305) Gordonia (307) Nike, (337) Devosa, and (352) Gisela", The Minor Planet Bulletin, 28: 32–34, Bibcode:2001MPBu...28...32L.{{citation}}: CS1 maint: multiple names: authors list (link)