SPHERE: IFS wavelength calibration
|
HC PLOTS |
resolving power |
|
dispersion |
|
QC1 database (advanced users):
browse |
plot
|
IFS wavelength calibration spectra raw frames are acquired in IFU mode and show
arc line spectra. Spectra come in two different setups: prism_YJ and prism_YJH.
There are four monochromatic laser lamps, each once produces one arc line in the spectrum
at the following nominal wavelengths:
0.9877 mu, 1.1237 mu, 1.3094 mu and 1.5451 mu,
The latter one is only covered by the wider wavelength range of the prism_YJH.
The pipeline recipe generates a product with PRO.CATG=IFS_WAVECALIB to be used to
calibrate science spectra and a product with PRO.CATG=IFS_WAVECALIB_CUBE, an
IFU fits cube which is analyzed by QC scripts in the following.
|
Median arc spectrum of the IFS wavelength cube product for prism_YJ with three arc lines.
Each arc line is fit by a Gaussian to monitor resolving power, arc line flux and measured wavelength.
|
|
Median arc spectrum of the IFS wavelength cube product for prism_YJH with four arc lines.
Each arc line is fit by a Gaussian to monitor resolving power, arc line flux and measured wavelength.
|
IFS resolving power
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[QC script] | sphere_ifs_wave..respow1 | laser lamp1 arc line respow | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..respow2 | laser lamp2 arc line respow | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..respow3 | laser lamp3 arc line respow | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..respow4 | laser lamp4 arc line respow | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
The QC script analyses the median extracted spectrum out of the pipeline cube product.
Each arc line is fit by a Gaussian and the best fit sigma is scaled to a FWHM an divided by
the central arc line wavelength. By this, from each arc line a value of the resolving power is retrieved.
Trending
The resolving power of the up to four arc lines is monitored
The resolving power of the individual arc line show a strong but small dependence of the IFS optical temperature, which monitored in a
< a href="/qc/SPHERE/reports/HEALTH/trend_report_IFS_REPO_TEMP_HC.html"> separate plot.
Scoring&thresholds IFS resolving power
All QC parameters are not scored.
History
- 2021-06-11: new pipeline version from 2021-03-16 on. The pipeline based resolving power is now given in units of FWHM (before in units of Gaussian Sigma)
- 2019-05-27: The pipeline (version 0.37) reports only the mean initial guess resolving power, which is not senistive to any real resolving power
variations.
The QC script analyses the cube product and provides the best fit values in the QC1 DB.
- 2017-11-29: The spos pipeline products are based on V0.28 (before V0.18). The initial guess of the
dispersion and the resolving power has changed.
Algorithm IFS resolving power
The QC script fits a Gaussian to each of the monochromatic laser lamp arc lines.
IFS arc line flux
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[QC script] | sphere_ifs_wave..flux1 | laser lamp1 arc line flux | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..flux2 | laser lamp2 arc line flux | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..flux3 | laser lamp3 arc line flux | HC | | [docuSys coming] |
[QC script] | sphere_ifs_wave..flux4 | laser lamp4 arc line flux | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
The QC script analyses the median extracted spectrum out of the pipeline cube product.
Each arc line is fit by a Gaussian and the best fit sigma is scaled to a FWHM an divided by
the central arc line wavelength. By this, from each arc line a value of the resolving power is retrieved.
Trending
Each arc line is generated by a separate laser lamp. The integrated flux is monitored
Scoring&thresholds IFS arc line flux
The QC parameters are not scored.
Some of the laser lamp fluxed are correlated with the IFS optical bench temperature, which is
monitored in a separate plot.
History
Algorithm IFS arc line flux
The QC script fits a Gaussian to each of the monochromatic laser lamp arc lines.
IFS dispersion
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[QC script] | sphere_ifs_wave..dispersion | wlenbin dispersion [mu/wlenbin] | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
|
Linear regression based on the Gaussian best fit positions.
|
|
Linear regression based on the Gaussian best fit positions.
|
Trending
Both plots for YJ .
The plots show in black the pipeline resultsi and in red the best fit dispersion performed by the QC script.
Scoring&thresholds IFS dispersion
QC parameters are not scored.
History
- In 2018 the QC scripts have been tested and in 2019 put in operation in order to monitor the health of the instrument.
- From 2019-07 on the QC.DISPERSON keyword value is shows, which is
the same value as given in the CD_3_3 keyword (= scale of the wavelength in the cube product).
For data acquired before 2019-07 the QC.MED.DISPERS keyword value is given, which is essntially the initial guess.
Algorithm IFS dispersion
The best fit positions of arc arc lines and their wavelength bins in the cube is used to derive a linear
regression to retrieve the wavelength of the first wavelength bin and the dispersion in mu/wlenbin.
|