The Effect of Detector Nonlinearity on WFIRST PSF Profiles for Weak Gravitational Lensing Measurements

@article{Plazas2016TheEO,
  title={The Effect of Detector Nonlinearity on WFIRST PSF Profiles for Weak Gravitational Lensing Measurements},
  author={A A Plazas and Charles A. Shapiro and Arun Kannawadi and Rachel Mandelbaum and James Rhodes and R. W. M. Smith},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2016},
  volume={128}
}
Weak gravitational lensing (WL) is one of the most powerful techniques to learn about the dark sector of the universe. To extract the WL signal from astronomical observations, galaxy shapes must be measured and corrected for the point-spread function (PSF) of the imaging system with extreme accuracy. Future WL missions—such as NASA’s Wide-Field Infrared Survey Telescope (WFIRST)—will use a family of hybrid near-infrared complementary metal-oxide-semiconductor detectors (HAWAII-4RG) that are… 

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