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UKIRT

United Kingdom Infrared Telescope

Spectroscopy with UIST

Spectroscopy with UIST

Instrument Parameters

  • Available SLITS
  • Available GRISMS: Resolution and wavelength coverage
  • Sensitivity tables
  • Readout modes and noise
  • Read speed, exposure times and efficiency
  • Gain and linearity
    • Non-linearity corrections
  • Saturation and sky counts

You may also view the above sections on a Single Page; from this page, click on the link at the top of the lilac side-bar for a printable version.

Observing

  • Running up and down
  • Preparing an observing programme – the UKIRT OT
    • Available template observations
    • OT Programme checklist
  • Online data reduction – ORAC DR
    • Available DR Recipes
  • Data format, orientation and location at UKIRT
  • Target acquisition

You may also view the above sections on a Single Page; from this page, click on the link at the top of the lilac side-bar for a printable version.

Calibration

  • UIST arc spectra for each grism
  • OH Sky Line spectra for Mauna Kea
  • In the L and M-band, methane and water lines are more prevelant. Sky-spectra are available here:
    • Short-L data: JPG , FITS or NDF
    • Long-L data: JPG , FITS or NDF
    • M data: JPG , FITS or NDF
  • Other calibration information: Ratio stars, line-lists, the Mauna Kea atmosphere

Recent Posts

  • New UKIRT Website!
  • 18 May 2012 – UKIRT’s Productivity Continues to Rise
  • 11 April 2012 – A New Customer for UKIRT
  • 15 March 2011 – UKIRT Sets New Productivity Record
  • 27 December 2010 – Remote Operations Implemented for UKIRT
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