SuperTIGER Abundances of Galactic Cosmic-Rays for the Charge Interval Z$=$41-56*

The SuperTIGER (Trans-Iron Galactic Element Recorder) instrument was launched from Williams Field, Antarctica on December 8, 2012 and flew for 55 days on a long-duration balloon at a mean altitude of 125,000 feet. SuperTIGER measured the relative abundances of Galactic cosmic-ray nuclei with high statistical precision and well resolved individual element peaks in the charge range Z$=$10-40. SuperTIGER also made exploratory measurements of the relative abundances up to Z$=$56. Although the statistics are low for charges greater than Z$=$40, we will show how the relative abundances of charges Z$=$40-56 compare to those reported by HEAO3-HNE. The charge range Z$=$40-60 is of particular interest because these elements are formed both in supernova explosions and in binary neutron star mergers. A well resolved relative abundance measurement of these elements can show us how much these astrophysical events contribute to the composition of the Galactic cosmic-rays.