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Hybrid Lyot Coronagraph for WFIRST: High Contrast Testbed Demonstration in Flight-like Low Flux Environment

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dc.contributor.author Seo, Byoung-Joon
dc.contributor.author Shi, Fang
dc.contributor.author Balasubramaian, Bala
dc.contributor.author Cady, Eric
dc.contributor.author Gordon, Brian
dc.contributor.author Kern, Brian
dc.contributor.author Lam, Raymond
dc.contributor.author Marx, David
dc.contributor.author Moody, Dwight
dc.contributor.author Muller, Richard
dc.contributor.author Patterson, Keith
dc.contributor.author Poberezhskiy, Ilya
dc.contributor.author Prada, Camilo Mejia
dc.contributor.author Riggs, A.J. Eldorado
dc.contributor.author Trauger, John
dc.contributor.author Wilson, Daniel
dc.date.accessioned 2020-05-18T22:24:48Z
dc.date.available 2020-05-18T22:24:48Z
dc.date.issued 2018-06-12
dc.identifier.citation SPIE Astronomical Telescopes + Instrumentation, Austin, Texas, June 12 - 14, 2018 en_US
dc.identifier.clearanceno 18-3558
dc.identifier.uri http://hdl.handle.net/2014/48509
dc.description.abstract In order to validate required operation of the proposed Wide-Field InfraRed Survey Telescope (WFIRST) coronagraph instrument, we have built a testbed in Jet Propulsion Laboratory (JPL), which is analogous to the baseline WFIRST coronagraph instrument architecture. Since its birth in 2016, this testbed, named as Occulting Mask Coronagraph (OMC) testbed, has demonstrated several crucial technological milestones: Broadband high contrast demonstration in both Hybrid Lyot Coronagraph (HLC) and Shape Pupil Coronagraph (SPC) modes while the Low Order Wavefront Sensing and Control (LOWFS/C) subsystem senses and corrects the dynamic flight-like wavefront disturbances. In this paper, we present up-to-date progress of HLC mode demonstration in the OMC testbed. While injecting the flight-like low photon flux starlight with expected Line of Sight (LoS) and Wavefront Error (WFE) perturbation to the OMC testbed, we demonstrate generating high contrast dark hole images. We first study the expected photon flux in actual flight environment, and estimate detection noise and estimation accuracy of the complex electric field if the wavefront sensing algorithm is used based on the pair-wise difference imaging. Then, we introduce our improved scheme to mitigate this photon-starved flight-like low flux environment. As a result, we generate a dark hole that meets the WFIRST raw contrast requirements using the 2nd magnitude star light. We establish the key ideas, describe test setups, and demonstrate test results with data analysis. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2018 en_US
dc.subject WFIRST en_US
dc.subject HLC en_US
dc.subject Coronagraph en_US
dc.subject Testbed en_US
dc.subject Exoplanet en_US
dc.title Hybrid Lyot Coronagraph for WFIRST: High Contrast Testbed Demonstration in Flight-like Low Flux Environment en_US
dc.type Preprint en_US


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