PIONIER: Spectral calibration
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HC PLOTS |
Spectral Calibration |
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QC1 database (advanced users):
browse |
plot
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This measures the effective wavelength of each spectral channel by measuring the actual fringes spacing for long scans. This is only possible if the internal piezo scanner is well calibrated/known and linear
Data can be taken on sky (used to calibrate sky/interferometric data). or on the internal lamp (to monitor the instrument).
The spectral calibration should be stable (around 2% in the GRISM mode)
Spectral Calibration
The spectral calibration measure the effective weavelength of each spectral channel by measuring the actual fringe spacing during a piezzo scan.
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.EFFWAVE | pionier_spectral_calib..spec_cal_effwave | effective wavelength [m], | HC | | [docuSys coming] |
QC.EFFBAND | pionier_spectral_calib..spec_cal_effband | effective band [m], | HC | | [docuSys coming] |
QC.EFFWAVE.PTP | pionier_spectral_calib..spec_cal_effwave_ptp | effective wavelength PTP [m], | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The value for the spectral calibration is plotted in the trending
plot.
The spectral calibration parameters are plotted for the different set-up
Scoring&thresholds Spectral Calibration
The value of the thresholds have been defined together with the Instrument scientist
History
The evolution of the central wavelength for the different setups is shown here
Algorithm Spectral Calibration
The pipeline computes a Fourier Transform spectrometry on the fringes recorded on long scans and calculates the effective WL and its width for the central Channel.
The value of the central wavelength depends of the accuracy of the knowledge of the scan rate of the piezzo .
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