We present simulated results for the Phase Induced Amplitude Apodization (PIAA)-Vortex coronagraph for on-axis telescope architectures. In previous studies, we demonstrated that the PIAA-Vortex coronagraph has the potential to overcome limitations on coronagraph performance for on-axis telescopes, and can maintain insensitivity to stellar angular diameters on the order of 0.1 λ/D at a contrast of 10−10. Here, we present designs for the PIAA-Vortex coronagraph optimized for a segmented, on-axis telescope aperture that creates a 10−10 - contrast, broadband dark zone with a 20% bandwidth and an inner working angle of 2.5 λ/D. These designs are part of ongoing modelling work. We show that the Earthlike exoplanet yield of the design presented here reduces the performance gap between on-axis and off-axis coronagraphy, and describe preliminary results which increase the throughput, aberration sensitivity, and overall yield of the coronagraph further. The PIAA-Vortex coronagraph will contribute to enabling consideration of obstructed telescope pupils for the Habitable Worlds Observatory, thereby taking advantage of previous NASA optical observatory heritage and potentially allowing for greater flexibility in observatory design.
|