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   distorsion(shift)
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MATISSE: Shift Map
 
HC PLOTS
Shift
QC1 database (advanced users): browse | plot

The shift map provides the distorsion and dispersion calibration laws. The measurement is made using plastic foils which provides a good estimate of the WL to pixel relation at low spectral resolution. For higher resolution, this measurement is not accurate enough and the fine spectral calibration is performed by means of sky measurements which are systematically recorded during the scientific observations.

The input data contains a series of images containing the laboratory background for each pinehole and for the slit (DISTOR_HOTDARK and SPECTRA_HOTDARK), a serie of images of the three pinholes (DISTOR_IMAGES), a serie of spectral images (SPECTRA_IMAGES), the static bad pixel map (BADPIX), the static nonlinearity map (NONLINEARITY) and the observation specific flatfield map (OBS_FLATFIELD).


detector shift

Due to the different optical paths, the photometrics and interferometric channels are not aligned in spectral and spatial directions. The optical elements produce different distorsions in the different channels.
This plugin calculates the distorsion coefficients of the photometric and interferometric channels, and it determines the relative shifts between each photometric channel and the interferometric one.
The input data are:

  • a series of images containing the laboratory background for each pinehole and for the slit (DISTOR_HOTDARK and SPECTRA_HOTDARK),
  • a series of images of the three pinholes (DISTOR_IMAGES),
  • a series of spectral images (SPECTRA_IMAGES),
  • the observation specific flatfield map (OBS_FLATFIELD),
  • the static calibrations BADPIX, NONLINEARITY

QC1_parameters

FITS key QC1 database: table, name definition class* HC_plot** more docu
QC.DET..PICOV1 matisse_shift..cov_shift_intphot1 relative coverage of the interferometric channel by the photometric channel 1 HC [docuSys coming]
QC.DET..PICOV2 matisse_shift..cov_shift_intphot2 relative coverage of the interferometric channel by the photometric channel 2 HC [docuSys coming]
QC.DET..PICOV3 matisse_shift..cov_shift_intphot3 relative coverage of the interferometric channel by the photometric channel 3 HC [docuSys coming]
QC.DET..PICOV4 matisse_shift..cov_shift_intphot4 relative coverage of the interferometric channel by the photometric channel 4 HC [docuSys coming]
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one.

Trending

The QC parameters cov_shift_intphot for the 4 different photometric channels and the defferent setup are shown in the trending plots.

Scoring&thresholds detector shift

The HC plots are not scored. For the individual AB, the thresholds values are set to detect jumps

History

The evolution of the shifts will be shown under "FULL" once more data have been accumulated.

Algorithm detector shift

The recipe used is mat_est_shift.

  • The static calibrations are applied on the input data to remove the reference subwindow, the badpixels, correct for non linearity and flatfield,
  • the frames of the corrected input files are summed for each region
  • the distorsion coefficients and the spectral shifts are calculated


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