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- Info
technical
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This describes the Astrometry in WFCAM.
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An explanation of how the dark and reset anomaly correction is carried out
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An explanation of how the flatfield correction is carried out. Also includes calculation of the confidence maps.
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An explanation of decurtaining
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An explanation of how sky subtraction is carried out
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A description of how the data is dithered (or jittered)
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This summarizes the PSF fitting work for WFCAM (TBD)
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The released documentation and reports for WFCAM
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This describes the Photometry in WFCAM.
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Linearity correction issues
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Defringing is not required
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How crosstalk is measured and removed
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A description of persistence in WFCAM data
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A description of how the data is interleaved (or interlaced or microstepped)
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A description of the catalogue products and their generation
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A broad description of the pipeline
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