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WFIRST coronagraph optical modeling

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dc.contributor.author Krist, John
dc.contributor.author Riggs, A. J.
dc.contributor.author McGuire, James
dc.contributor.author Tang, Hong
dc.contributor.author Amiri, Nikta
dc.contributor.author Gutt, Gary
dc.contributor.author Marchen, Luis
dc.contributor.author Marx, David
dc.contributor.author Nemati, Bijan
dc.contributor.author Saini, Navtej
dc.contributor.author Sidick, Erkin
dc.contributor.author Zhou, Hanying
dc.date.accessioned 2020-03-23T20:23:54Z
dc.date.available 2020-03-23T20:23:54Z
dc.date.issued 2017-08-08
dc.identifier.citation 2017 SPIE Optics and Photonics, San Diego, California, August 6-10, 2017 en_US
dc.identifier.clearanceno CL#17-3883
dc.identifier.uri http://hdl.handle.net/2014/47762
dc.description.abstract End-to-end numerical optical modeling of the WFIRST coronagraph incorporating wavefront sensing and control is used to determine the performance of the coronagraph with realistic errors, including pointing jitter and polarization. We present the performance estimates of the current flight designs as predicted by modeling. We also describe the release of a new version of the PROPER optical propagation library, our primary modeling tool, which is now available for Python and Matlab in addition to IDL. 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, 2017 en_US
dc.title WFIRST coronagraph optical modeling en_US
dc.type Preprint en_US


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