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- W3100290530 abstract "As planning for the next generation of high contrast imaging instruments (e.g., WFIRST, HabEx, and LUVOIR, TMT-PFI, EELT-EPICS) matures and second-generation ground-based extreme adaptive optics facilities (e.g., VLT-SPHERE, Gemini-GPI) finish their principal surveys, it is imperative that the performance of different designs, post-processing algorithms, observing strategies, and survey results be compared in a consistent, statistically robust framework. In this paper, we argue that the current industry standard for such comparisons—the contrast curve—falls short of this mandate. We propose a new figure of merit, the performance map, that incorporates three fundamental concepts in signal detection theory: the true positive fraction, the false positive fraction, and the detection threshold. By supplying a theoretical basis and recipe for generating the performance map, we hope to encourage the widespread adoption of this new metric across subfields in exoplanet imaging." @default.
- W3100290530 created "2020-11-23" @default.
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- W3100290530 date "2017-12-14" @default.
- W3100290530 modified "2023-10-15" @default.
- W3100290530 title "A New Standard for Assessing the Performance of High Contrast Imaging Systems" @default.
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- W3100290530 doi "https://doi.org/10.3847/1538-3881/aa97e4" @default.
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