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| SINFONI has four gratings,
(see the User Manual for details concerning grating properties). Our QC1 checks
using flat frames can be divided in several categories: - PRODUCT QC
PLOT. For each dark pipeline product and its associated raw frames we create
a plot with the most significant features.
- DIFFERENCE FRAMES. A
simple and efficient method to check short-term and long-term variations is to
construct difference frames
- TRENDING This means that selected QC1
parameters are monitored as a function time. The purpose is to find long term
variations which cannot detected on a single product frame.
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| Trending describes the variation
of a QC1 parameter with time. Trending plots don't consist of control limits.
Their purpose is more to document long term changes of QC1 parameters, which cannot
be detected in process control charts. Trending plots can be subject of 'time
series analysis'. The same QC1 parameters as the ones shown under the 'control
chart' section are trended. More parameters are available via the interfaces of
our QC1 parameter database. - Lamp flux. The flux of the halogen
lamp as measured by the detector depends on the lamp flux itself but also on the
spectroscopic setting and the alignment of optical elements in the ray path. The
lamp=off frame subtracted lamp=on fluxes as calculated by the recipe is monitored.
Day-time spflat calibrations come in five pairs of lam=on/off frames. Night time
calibrations (attached calibrations) come as one pair. The plots show HIERARCH
ESO QC SPECFLAT NCNTSAVG. For each raw lamp-on frame the corresponding lamp-off
frame is subtracted and the median is calculated. The QC parameter is the average
of these 5 values.The lamp efficiency would be the lamp flux divided by DIT to
get the count rate. Monitoring the lamp efficiency would make sense when monitoring
in parallel the lamp amplifier value, an operationally defined value to get for
the operational DIT for lamp flats the desired lamp flux.
- Bad Pixel, as derived from the NORM method of the sinfo_rec_mflat recipe
- Lamp-off flux, is used to monitor light/heat contamination in the
optical path. The flux measured in lamp-off frames is usually a few counts above
the reset anomaly of the same DIT (the dark counts), since a broad band filter
is used for the lamp-off frames, wile the dark frames are taken with two excluding
narrow band filters.The plots show HIERARCH ESO QC SPECFLAT OFFFLUX, that is the
average of the (five) off-lamp medians.
- Fixed Pattern noise, in as selected region on the array. This is a
simple standard deviation of the flat product frame. The region is specified in
the sinfo_rec_mflat.rc file. In P75 it was the central quarter [@512,@512:@1536,@1536]
- Fixed Pattern noise, in as selected region (another region than region
1) on the array. This is a simple standard deviation of the flat product frame.
The region (region 2) is specified in the sinfo_rec_mflat.rc file. In P75 it was
a area on one single slitlet [@1350,@1000:@1390,@1200]
- Vignetting in slitlet #1 and #32:
slitlet #1 and slitlet #32 corresponding
to the uppermost and lowermost slitlet in the FOV, and are projected onto the
central part of the detector and are subject of vignetting, meaning the
countrate can be a few 10% lower than in the other slitlets. The light loss
is dependent on the grating and the pre-optics. We monitor the relative countrate
(e.g. median counts in slitlet #1 devided by median count rate of the whole
frame that should be 1 ) in a selected window of slitlets #1 and slitlet #32
in the master flat frame.
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