SPHERE: IFS instrument flat
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HC PLOTS |
counts in the YJ raw ifu flat frame |
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counts in the YJH raw ifu flat frame |
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QC1 database (advanced users):
browse |
plot
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IFS raw flat field is acquired during day time. The pipeline recipe requires imaging flats field products and the wavelength calibration product.
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Image of the IFS_IFU_FLAT_FIELD product to be used in all subsequent steps of the calibrations cascade.
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Zoom of the IFS_INSTRUMENT FLAT_FIELD product.
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IFS Spectroscopic Flats
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
DRS.RAW.MED.MEDIAN | sphere_ifs_flat..qc_rawmed_med | of det.plane product | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The median counts of the raw flat is monitored.
For setup YJ values of about 2500 ADU are generated by the template with TPL NAME = 'Static Weekly Flats for IFS', using DIT=2sec.
Scoring&thresholds IFS Spectroscopic Flats
The QC parameters are scored.
The pipeline reports the frame plane average counts. The counts in the indiviual slices is ~4 times larger than the frame plane average counts
for the YJH prism (3 times for the YJ prism). Using NDIT=10 the total counts in the slice in the raw frame cube is a factor 40 larger (30 for the YJ prism).
Therefore 1300 ADU (1000 ADU for YJ) must be achieved as average counts number in one plane of a raw frame cube to gain sqrt ( 1000 * 10 * 4 ) = 200 S/N for the YJH prism.
For the upper threshold, the counts in the indiviual slice of a raw frame plane should be well below 40000 ADU, hence the plane average should be less than 10000 ADU.
History
Date |
event |
2018-04-10 | INS4.OPTI1.ID = LAMP_QL2, (before it was LAMP_QL1) |
2018-06 | lamp counts begin to decrease |
2019-01-06 | LAMP_QL1 is used again. |
Algorithm IFS Spectroscopic Flats
The raw median raw counts is retrieved.
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