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VIMOS trending system: HISTORY plot
Last update: 2010-01-10T04:32:36 (UT)
same group: dark_low dark_high gain fp-noise   detmon_gain
close window history: 2009 2010   2011 2012 2013 2014 2015 2016 2017 2018   HEALTH FULL
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Plot
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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 -0.0059 NONE VAL-0.01.0,0.01 18 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q2, low gain
2 QC1DB MEDIAN -0.0045 NONE VAL-0.01.0,0.01 19 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q1, low gain
3 QC1DB MEDIAN -0.0048 NONE VAL-0.01.0,0.01 14 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q2, high gain
4 QC1DB MEDIAN -0.0048 NONE VAL-0.01.0,0.01 14 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q1, high gain
5 QC1DB MEDIAN -0.006 NONE VAL-0.01.0,0.01 18 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q3, low gain
6 QC1DB MEDIAN -0.0012 NONE VAL-0.01.0,0.01 19 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q4, low gain
7 QC1DB MEDIAN -0.0059 NONE VAL-0.01.0,0.01 14 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q3, high gain
8 QC1DB MEDIAN -0.0037 NONE VAL-0.01.0,0.01 14 lineff this | last_yr | all eff. non-linearity at 40000ADU, Q4, high gain
*Data sources: QC1DB: QC1 database; LOCAL: local text file
This plot

Trending plot for non-linearity measurements of the VIMOS detectors.

Data are taken from detector monitoring calibrations which are series of flat fields with increasing exposure times. A second order polynomial is fit to the data (flux vs. exposure time for each pixel). The trending shows the average effective non-linearity at 40000 ADU. Effective non-linearity is the difference between the flux predicted at 40000 ADU by the linear term and the flux obtained from the polynomial, normalized by the polynomial flux.

Only the central 1600 x 1800 pixles are used for calculation of detector monitoring parameters (since 2009-10-09).

The average effective non-linearity should be near zero.

The non-linearity parameter showed strong scatter in 2011 and 2012 due to stability problems with the flat-fields. The highest flux for the high-gain read-out mode was also too low until January 2014 so that the non-linearity at 40000 ADU was not well determined.

Template ID: tec_DetLin. Pipeline recipe: vmdetlin.  


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