The vector vortex coronagraph is an ideal choice for the future space-based mission that is proposed by Astro2020. However, it requires polarization filtering and every observing band requires a different VVC. The triple-grating vector vortex coronagraph (TGVVC) aims to mitigate these limitations. In this paper, we present the first laboratory results of a TGVVC prototype using the High Contrast Imaging Testbed facility at NASA’s Jet Propulsion Laboratory. We describe the design and manufacturing, study the coronagraphic performance, the impact of polarization filtering on the dark zone contrast, and the appearance and impact of half-orders.
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