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FORS1:
detector: monitoring
old CCD
(before 2007-03-25)
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FORS1 trending system: History Plots
Last update: 2009-04-09T06:51:36 (UT)
| now: 2024-04-19T19:31:06 (UT)  
same group: dark linearity gain   conad fp_noise
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- png file - advanced studies: QC1 browser | QC1 plotter
 
Plot
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Symb
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Source
*
OPS?
**
Average ? Thresholds ? N_
data
QC1
parameter
Data
downloads
Remarks
method value unit method value
1 QC1DB no MEDIAN 0.00166 NONE VAL0,0.003 18 FPN_rel this | last_yr | all C1, high gain
2 QC1DB no MEDIAN 0.00135 NONE VAL0,0.003 18 FPN_rel this | last_yr | all C2, high gain
3 QC1DB no MEDIAN 0.0025 NONE VAL0.002,0.003 18 FPN_rel this | last_yr | all C1, low gain
4 QC1DB no MEDIAN 0.00203 NONE VAL0.0015,0.0025 18 FPN_rel this | last_yr | all C2, low gain
*Data sources: QC1DB: QC1 database; LOCAL: local text file | **OPS: to indicate that OPSLOG data are included
This plot

The fixed-pattern noise is computed in the following way: The difference of two 100x100 sub-frames of the same master flat field image is determined. These two sub-frames are are shifted with respect to each other by 10 pixels in X- and Y-direction. The population standard deviation of the difference frame, divided by the square root of 2, minus the photon noise (geometrically subtracted) yields the fixed-pattern noise, which is then divided by the median of the respective region.  


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