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
- 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
- Online data reduction – ORAC DR
- 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:
- Other calibration information: Ratio stars, line-lists, the Mauna Kea atmosphere