CRIRES
Quality Control: wavelength calibrations |
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Wavelength calibration for CRIRES can be obtained with several different methods: from sky lines in science frames, from dedicated wavelength calibration frames using an arc lamp or a gas cell, or from a physical model. This page describes QC checks on arc lamp and gas cell exposures. CRIRES offers a ThAr arc lamp for measuring emission line spectra and a gas cell which is filled with N2O gas and illuminated by the halogen (flat-field) lamp for absorption line spectra. Wavelength calibration frames are measured during daytime according to the settings used during the night. They are also frequently attached to science OBs. For settings above 2400 nm, wavelength calibrations are usually not taken because the density of sky lines is sufficiently high. For health check purposes, a ThAr exposure with reference wavelength 1090.4 nm and an N2O exposure with 4092.9 nm are measured daily. In April 2008, a fibre bundle was mounted in front of the ThAr lamp. The light is projected as separate traces on the detector. Since June 2009, also a metrology fibre is present (on the very top). The pipeline recipe performs a cross-correlation between the observed frame and a template which is derived from the line lists. The cross-correlation value is a unitless number between 0 and 1. A value above 0.2 is regarded as a successful solution. In case of a failure, the recipe gives -1 as cross-correlation result.
QC1 parameters for CRIRES arc lamp and gas cell exposures are measured for each detector array separately. QC1 parameters
Trending QC1 parameters for wavelength calibration are trended for the daily health check settings with 1090.4 nm (ThAr) and 4092.9 nm (N2O). Trending consists of the cross-correlation result, of the central wavelength on each detector array, the dispersion, spectral resolution (ThAr lamp only), and the lamp efficiency (ThAr lamp only). History April 2008: fibres are mounted in front of ThAr lamp |
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