One of the most profound scientific questions is whether there are other Earth-like worlds. To image such exoplanets directly, the Astro2020 Decadal Survey highly recommends technology development for a future 6- meter, space-based observatory equipped with a coronagraph. The vector vortex coronagraph (VVC) is a top candidate for providing the necessary 10−10 planet-to-star contrast ratio needed at small angular separations to image and characterize Earth-like exoplanets. The VVC is best suited for an unobscured aperture, but for a 6-meter, space-based observatory the primary mirror may need to be segmented. In this paper, we describe our laboratory experiments testing a charge four VVC with a segmented, off-axis entrance pupil. The extra diffraction from the pupil segmentation was suppressed with the single Boston Micromachines deformable mirror in the optical system. We achieved a mean normalized intensity of 4.7 × 10−9 from 3 − 10 λ/D in a 10% spectral bandwidth in the Decadal Survey Testbed at the Jet Propulsion Laboratory. To determine our current limitations and to enable 10−10 contrast in future tests, we compare to other testbed results with a monolithic aperture.
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