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SINFONI trending system: HISTORY plot
Last update: 2010-09-24T16:26:19 (UT)
same group: DARK_dit=300   dit=10 dit=60 dit=600 dit=900
close window history: 2005   2006   2007 2008 2009 2010 2011   HEALTH FULL
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*Date on this monitor changes at 21:00 UT
Print: Information and research:
- png file - advanced studies: QC1 browser | QC1 plotter
Plot
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Symb
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Source
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Average ? Thresholds ? N_
data
QC1
parameter
Data
downloads
Remarks
method value unit method value
1 QC1DB MEDIAN 10.22329 ADU VAL0.0,25.0 34 qc_darkmed_ave this | last_yr | all median dark level, as computed from the master dark
2 QC1DB MEDIAN 0.38836 ADU VAL-3.0,4.0 34 qc_darkmed_stdev this | last_yr | all standard deviation of median dark level
3 QC1DB MEDIAN 3.07637 ADU VAL2.5,3.75 34 qc_ron2 this | last_yr | all rms noise derived by subtracting 2 consecutive raw darks (normalized to DET.DIT = 1 second)
4 QC1DB MEDIAN 2.5006 ADU VAL1.0,4.0 34 qc_gaf_fpn this | last_yr | all fixed pattern noise as computed by fitting a Gaussian to the master dark histogram
5 QC1DB MEDIAN 10011.0 number VAL2000,20000 34 qc_bpm_nbadpix this | last_yr | all number of pixels with a high dark current
6 QC1DB MEDIAN -0.03912 unitless VAL-2.,2. 34 qc_oes2 this | last_yr | all median ratio of odd-even column stripes in the area of slitlet #25
*Data sources: QC1DB: QC1 database; LOCAL: local text file
This plot

These are the trending plots for the SINFONI QC parameters derived from DARK frames.

These plots describe:

1. the median DARK level, as computed from each master dark frame.

2. the standard deviation of the median DARK level.

3. the root-mean-squared noise, as derived by subtracting two consecutive raw dark frames, computing a median standard deviation in
selected sub-windows, computing a median standard deviation in selected sub-windows in the difference image, and then normalizing to DET.DIT=1 second.

4. the fixed pattern noise, as computed by fitting a Gaussian to the histogram of the master dark frames. The fpn is simply the standard deviation of Gaussian.

5. the number of pixels with a high dark current.

6. the odd-even column stripes in the area of slitlet #25. If med(odd) = median of all odd columns in the area of slitlet #25
and med(even) = median of all even columns in the area of slitlet #25 then, this plot is defined as:
oes25 = 2 * (med(odd) - med(even)) / (med(odd) + med(even))

Find more information about SINFONI DARK frames here.

Other QC parameters related to detector properties (like dark level, linearity, gain, etc.) are also trended here.  


General information

Click on any of the plots to see a close-up version. The latest date is indicated on top of the plot, data points belonging to that date are specially marked.

If configured,

  • statistical averages are indicated by a solid line, and thresholds by broken lines
  • outliers are marked by a red asterisk. They are defined as data points outside the threshold lines
  • "aliens" (= data points outside the plot Y limits) are marked by a red arrow ( or )
  • you can download the data for each parameter set if the 'Data downloads' link shows up