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Health Check monitor

 

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HealthCheck Monitor
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SPHERE trending system: HEALTH CHECK report
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Last update: 2024-04-24T04:45:05 (UT)
  | now: 2024-04-24T13:00:21 (UT) muc03 QC pipeline: spher-0.52.0 (installed 2024-03-22)
same group: med_master ron NumHotPix persistence persist/temp   Background NormPersist
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.
SPHERE news: Note that the current Health Check monitor runs with an incomplete pipeline and an incomplete set of QC1 parameters. QCG can currently not guarantee completeness and significance at the usual level.
Report news:
DATE*: [?] 2024-04-17
report | NLT
2024-04-18
report | NLT
2024-04-19
report | NLT
2024-04-20
report | NLT
2024-04-21
report | NLT
2024-04-22
report | NLT
2024-04-23
no data | NLT
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*Date on this monitor changes at 21:00 UT
png: Information and research:
- png file - advanced studies: QC1 browser | QC1 plotter
Plot
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Symb
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Source
*
Average ? Thresholds ? N_
data
QC1
parameter
Data
downloads
Remarks
method value unit method value
1 QC1DB none   ADU none  23 qc_persistence this | last_yr | all DARK, DIT=2, NDIT=40
1 QC1DB none   ADU none  66 qc_persistence this | last_yr | all DARK, DIT=5, NDIT=10
2 QC1DB none   ADU none  23 qc_persistence this | last_yr | all DARK, DIT=8, NDIT=25
2 QC1DB none   ADU none  66 qc_persistence this | last_yr | all DARK, DIT=11, NDIT=10
3 QC1DB none   ADU none  23 qc_persistence this | last_yr | all DARK, DIT=30, NDIT=15
3 QC1DB none   ADU none  0 qc_persistence this | last_yr | all DARK, DIT=64, NDIT=20
4 QC1DB none   ADU none  22 qc_persistence this | last_yr | all BACKGROUND, DIT=2, NDIT=40
4 QC1DB none   ADU none  44 qc_persistence this | last_yr | all BACKGROUND, DIT=4, NDIT=20
5 QC1DB none   ADU none  22 qc_persistence this | last_yr | all BACKGROUND, DIT=8, NDIT=25
5 QC1DB none   ADU none  74 qc_persistence this | last_yr | all BACKGROUND, DIT=16, NDIT=20
6 QC1DB none   ADU none  22 qc_persistence this | last_yr | all BACKGROUND, DIT=30, NDIT=15
6 QC1DB none   ADU none  38 qc_persistence this | last_yr | all BACKGROUND, DIT=64, NDIT=20
*Data sources: QC1DB: QC1 database; LOCAL: local data source
Plot 1
scores: not implemented
data source:sphere_ifs_dark
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:23
[click plot for closeup]
Plot 2
scores: not implemented
data source:sphere_ifs_dark
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:23
[click plot for closeup]
Plot 3
scores: not implemented
data source:sphere_ifs_dark
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:23
[click plot for closeup]
Plot 4
scores: not implemented
data source:sphere_ifs_background
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:22
[click plot for closeup]
Plot 5
scores: not implemented
data source:sphere_ifs_background
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:22
[click plot for closeup]
Plot 6
scores: not implemented
data source:sphere_ifs_background
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_persistence
average:none
thresholds:none
N_data plotted:22
[click plot for closeup]
This plot

This plot monitors the persistence in both IFS dark and IFS background calibrations which can be generated by previously acquired IFS optical distortion calibrations. These optical distortion calibrations can leave a pinhole slice pattern in the IFS dark or background pipeline product.

The QC parameter is simply: the median counts in the pipeline product in a window P = [770, 1300 --- 850, 1440] minus the median counts in window B = [640, 1470 --- 720, 1570].

Window P (pinhole) is the area where the pinhole slice pattern can show up and window B (background) is the area off the pinhole slice pattern areas on the detector.

This kind of monitoring was introduced 2018-01-01.

IFS_DARK master frames are not used to calibrate observations, only the ancillary IFS_DARK product IFS_STATIC_BADPIXEL is used. IFS_BACK calibrations are used to calibrate science observations.  


General information

Click on any of the plots to see a close-up version.

The latest date is indicated on top of the plot.

If configured,

  • data points belonging to the latest date are specially marked
  • 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