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Examples of Calibration Data

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  • Plots of CuAr spectra to assist with wavelength calibration
  • Imaging flat fields for GMOS-N and GMOS-S
  • Bias images for GMOS-N and GMOS-S

    The GMOS-N DD E2V detectors, which were in operation until February 2017, and the new GMOS-N and GMOS-S Hamamatsu detectors exhibit much less fringing than the original EEV detectors. See GMOS-N fringing and GMOS-S fringing for examples.

  • Gemini Observatory Participants