Optical tests of four TiN MKID inductor volumes at 410 GHz identify the 660 µm^3 design as optimal for the CCAT Prime-Cam module under 10-20 pW sky loading.
CCAT-Prime: science with an ultra-widefield submillimeter observatory on Cerro Cha- jnantor,
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CCAT: The 410 GHz camera module for FYST - design and testing of the MKID focal plane
Optical tests of four TiN MKID inductor volumes at 410 GHz identify the 660 µm^3 design as optimal for the CCAT Prime-Cam module under 10-20 pW sky loading.