Abstract
Following the largely positive results of the table-top LG mode experiments, we were afforded a fortuitous opportunity to work in collaboration with members of the Glasgow interferometry group towards testing the LG mode technology on the 10 m suspended cavity in Glasgow. Progression from table-top experiments to a prototype experiment with suspended mirrors is a standard feature of the development of new technologies for gravitational wave detectors, in order to ensure compatibility with realistic interferometer subsystems and requirements.
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