Demonstration of high contrast with an obscured aperture with the WFIRST-AFTA shaped pupil coronagraph
arXiv:1511.01882 · doi:10.1117/1.JATIS.2.1.011004
Abstract
The coronagraph instrument on the WFIRST-AFTA mission study has two coronagraphic architectures, shaped pupil and hybrid Lyot, which may be interchanged for use in different observing scenarios. Each architecture relies on newly-developed mask components to function in the presence of the AFTA aperture, and so both must be matured to a high technology readiness level (TRL) in advance of the mission. A series of milestones were set to track the development of the technologies required for the instrument; in this paper, we report on completion of WFIRST-AFTA Coronagraph Milestone 2---a narrowband contrast test with static aberrations for the shaped pupil---and the plans for the upcoming broadband Coronagraph Milestone 5.
arXiv comment35 pages, 15 figures
References in corpus (5)
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- Fast computation of Lyot-style coronagraph propagation
- High Performance Lyot and PIAA Coronagraphy for Arbitrarily shaped Telescope Apertures
- Circularly Symmetric Apodization via Starshaped Masks
- Rectangular-Mask Coronagraphs for High-Contrast Imaging
Cited by in corpus (12)
- Characterizing Earth Analogs in Reflected Light: Atmospheric Retrieval Studies for Future Space Telescopes
- Shaped Pupil Lyot Coronagraphs: High-Contrast Solutions for Restricted Focal Planes
- Color Classification of Extrasolar Giant Planets: Prospects and Cautions
- Characterization of Exoplanet Atmospheres with the Optical Coronagraph on WFIRST
- Techniques for High-Contrast Imaging in Multi-Star Systems II: Multi-Star Wavefront Control
- Flight mask designs of the Roman Space Telescope Coronagraph Instrument
- Laboratory and On-Sky Validation of the Shaped Pupil Coronagraph's Sensitivity to Low-Order Aberrations With Active Wavefront Control
- High-contrast imager for complex aperture telescopes (HiCAT): 5. first results with segmented-aperture coronagraph and wavefront control
- Laboratory Demonstration of Spatial Linear Dark Field Control For Imaging Extrasolar Planets in Reflected Light
- High-order wavefront sensing and control for the Roman Coronagraph Instrument (CGI): architecture and measured performance
- Demonstration of broadband contrast at 1.2 /D and greater for the EXCEDE Starlight Suppression System
- Flight masks of the Roman Space Telescope Coronagraph Instrument