Presentation + Paper
23 August 2024 Demonstration of coronagraphs and wavefront control at the testbed EXIST
Author Affiliations +
Abstract
We have built a laboratory testbed called the Exoplanet Imaging System Testbed (EXIST) to develop future highcontrast imaging technologies. The main objective of the EXIST is the development of broadband coronagraph and wavefront control techniques. The EXIST is equipped with several fiber-coupled laser and broadband light sources to model star and planets. A spatial light modulator (SLM) is used to carry out the wavefront control in front of the coronagraph. We incorporated a variety of coronagraphic masks, including four-quadrant, eightoctant, and 12-sector phase masks. These masks exhibit second-, fourth-, and sixth-order starlight suppression properties, respectively. When combined with the wavefront control, higher-order coronagraphic masks provided better dark hole contrast. This paper reports on recent experimental results and prospects for future technological development at the EXIST.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Naoshi Murakami, Mizuki Asano, Shunya Sato, Kenta Yoneta, and Jun Nishikawa "Demonstration of coronagraphs and wavefront control at the testbed EXIST", Proc. SPIE 13092, Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave, 1309220 (23 August 2024); https://doi.org/10.1117/12.3018382
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KEYWORDS
Coronagraphy

Wavefronts

Spatial light modulators

Point spread functions

Exoplanets

Spiral phase plates

Wave plates

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