Paper
29 July 2016 The Segmented Aperture Interferometric Nulling Testbed (SAINT) I: overview and air-side system description
Brian A. Hicks, Richard G. Lyon, Peter Petrone III, Marlin Ballard III, Matthew R. Bolcar, Jeff Bolognese, Mark Clampin, Peter Dogoda, Daniel Dworzanski, Michael A. Helmbrecht, Corina Koca, Ron Shiri
Author Affiliations +
Abstract
This work presents an overview of the Segmented Aperture Interferometric Nulling Testbed (SAINT), a project that will pair an actively-controlled macro-scale segmented mirror with the Visible Nulling Coronagraph (VNC). SAINT will incorporate the VNC’s demonstrated wavefront sensing and control system to refine and quantify end-to-end high-contrast starlight suppression performance. This pathfinder testbed will be used as a tool to study and refine approaches to mitigating instabilities and complex diffraction expected from future large segmented aperture telescopes.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Brian A. Hicks, Richard G. Lyon, Peter Petrone III, Marlin Ballard III, Matthew R. Bolcar, Jeff Bolognese, Mark Clampin, Peter Dogoda, Daniel Dworzanski, Michael A. Helmbrecht, Corina Koca, and Ron Shiri "The Segmented Aperture Interferometric Nulling Testbed (SAINT) I: overview and air-side system description", Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 990420 (29 July 2016); https://doi.org/10.1117/12.2234313
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Telescopes

Space telescopes

Mirrors

Coronagraphy

Image segmentation

Point spread functions

Exoplanets

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