The Analytical Performance Model and Error Budget for the Roman Coronagraph Instrument
Bijan Nemati, John Krist, Ilya Poberezhskiy, Brian Kern

TL;DR
This paper presents an analytical performance model and error budget for the Roman Coronagraph Instrument, aiding system optimization for high-contrast exoplanet imaging in space.
Contribution
It introduces a comprehensive analytical model and error budget framework specifically designed for the Roman Coronagraph, facilitating performance prediction and system optimization.
Findings
The error budget enables rapid performance calculations.
The model supports trade-offs in system design.
It guides the optimization of high-contrast imaging performance.
Abstract
The Nancy Grace Roman Space Telescope (Roman), under development by NASA, will investigate possible causes for the phenomenon of dark energy and detect and characterize extra-solar planets. The 2.4 m space telescope has two main instruments: a wide-field, infra-red imager and a coronagraph. The coronagraph instrument (CGI) is a technology demonstrator designed to help bridge the gap between the current state-of-the-art space and ground instruments and future high-contrast space coronagraphs that will be capable of detecting and characterizing Earth-like planets in the habitable zones of other stars. Using adaptive optics, including two high-density deformable mirrors and low- and high-order wavefront sensing and control, CGI is designed to suppress the star light by up to 9 orders of magnitude, potentially enabling the direct detection and characterization of Jupiter-class exoplanets.…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Systems and Laser Technology · Advanced optical system design
