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Health Check monitor

 

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FORS2:
image quality science
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FORS2 trending system: HEALTH CHECK report
Last update: 2012-06-21T14:24:36 (UT)
| now: 2024-12-22T12:38:15 (UT)
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same group: bH_TEL vH_TEL R_TEL I_TEL   bH_DIMM vH_DIMM R_DIMM I_DIMM
General news: NOTE: The Health Check and calChecker services are moved to qcFlow on an instrument by instrument basis. The current pages will not be updated any longer once the move has been finished.
FORS2 news:  
Report news: 2011-10-01 trending stopped as SCIENCE data are no longer processed by QC
DATE*: [?] 2024-12-15
no data | NLT
2024-12-16
no data | NLT
2024-12-17
no data | NLT
2024-12-18
no data | NLT
2024-12-19
no data | NLT
2024-12-20
no data | NLT
2024-12-21
no data | NLT
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Raw CAL displays:
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CAL product quality:
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  no OPSLOG data  

scores&comments | history ... | plot tutorial ... | contact | HC_docu...               [?]
*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
*
OPS?
**
Average ? Thresholds ? N_
data
QC1
parameter
Data
downloads
Remarks
method value unit method value
1 QC1DB no none   arcsec none  126 iq this | last_yr | all Observed Image Quality in b_HIGH vs Active Optics Image Quality with 1:1 line overplotted (chip1)
2 QC1DB no none   arcsec none  117 iq this | last_yr | all Observed Image Quality in b_HIGH vs Active Optics Image Quality with 1:1 line overplotted (chip2)
*Data sources: QC1DB: QC1 database; LOCAL: local text file | **OPS: to indicate that OPSLOG data are included
Plot 1
scores: not implemented
data source:fors2_sci_img
(QC1 database)
dataset:iq
average:none
thresholds:none
N_data plotted:126
[click on plot for closeup]
Plot 2
scores: not implemented
data source:fors2_sci_img
(QC1 database)
dataset:iq
average:none
thresholds:none
N_data plotted:117
[click on plot for closeup]
This plot

Starting with Period 71 (April 2003), all reduced FORS2 science images taken in Service Mode are analyzed in order to estimate their Image Quality (hereafter IQ). This is done in a fully automatic way using a stand-alone procedure based on the Sextractor object detection algorithm (Bertin and Arnouts 1996 A&A 117,393). Stars are identified based on Sextractor parameters (Stellarity Index > 0.5, ellipticity <0.5 and quality FLAG=0) and their FWHM is measured by the program. Then the mode of the IQ distribution is computed and the RMS deviation is estimated using the left wing of the distribution only. Only IQ measurements obtained with the Standard Resolution (SR) collimator and taken through the broad-band UBVRI filters are trended here. To reduce the uncertainty, only image quality values are plotted, which result from more than 10 stars and have at at least one DIMM seeing measurement during their exposure time. To avoid a bias from deep exposures, where galaxies dominate the field, we require in addition that the average ellipticity is less than 0.3 and the rms of the image quality is below 0.2. For comparison we use the image quality as reported by the Active Optics, corrected to the airmass of the respective science images. More information can be found on the plot tutorial page  


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