Presentation + Paper
29 August 2022 Improving the photometric accuracy of JWST by limiting the dynamic range of integrations
Michael W. Regan, Louis Bergeron
Author Affiliations +
Abstract

The inherent nonlinear response of infrared detectors limits the ultimate photometric accuracy that can be obtained. In this paper we show that, by limiting the observations to a fraction of the full dynamic range, we can decrease the variance of the corrected residuals. This improvement is due both to a more accurate nonlinearity correction solution and to a reduction in the number of pixels affected by saturation in neighboring pixels.

We compare several metrics of goodness-of-fit for non-linearity corrected integrations over a range of full well fractions. We show that, by limiting the operational dynamic, we can improve the quality of the non-linearity corrections and increase the number of science-grade pixels. We find that when we limit the dynamic range to 80% of the full well, the variance of the residuals decreases by a factor of two and that other metrics of slope consistency show even larger improvements.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael W. Regan and Louis Bergeron "Improving the photometric accuracy of JWST by limiting the dynamic range of integrations", Proc. SPIE 12191, X-Ray, Optical, and Infrared Detectors for Astronomy X, 121911Q (29 August 2022); https://doi.org/10.1117/12.2630677
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KEYWORDS
James Webb Space Telescope

Sensors

Calibration

Photometry

Quality measurement

Space telescopes

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