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16576

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DataCite Commons2023-04-21 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/hst/16576.html
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The WFC3-IR detector exhibits a non-linear response to incident flux. The data reduction pipeline provides a correction for the non-linearity comma which depends on accurate characterization of the response of the detector. To monitor the non-linearity of the WFC3-IR detector comma we use a dark observation followed by two internal flats using the Tungsten lamp at different sampling rates comma and a trailing dark. Any changes measured in the non-linearity will be updated in the calibration reference file comma crucial to providing a correction for accurate photometry. This program is a continuation of the cycle 28 (program 16404) linearity calibration program.
提供机构:
European Space Agency
创建时间:
2023-04-21
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