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GIRAFFE trending system: HEALTH CHECK report
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Last update: 2024-05-27T16:34:58 (UT)
  | now: 2024-05-27T19:59:05 (UT) muc02 QC pipeline: giraf-2.16.10 (installed 2023-06-22)
same group: SIM-lamp FF-lamp ARC-lamp   NAS-lamp
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.
The links to KMOS, UVES, and ESPRESSO have been moved to a new section (qcFlow operational) at the lower part of the navigation bar.
GIRAFFE news:  
Report news:
DATE*: [?] 2024-05-20
report | NLT
2024-05-21
report | NLT
2024-05-22
report | NLT
2024-05-23
report | NLT
2024-05-24
report | NLT
2024-05-25
report | NLT
2024-05-26
report | NLT
r...
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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
?
Symb
?
Source
*
Average ? Thresholds ? N_
data
QC1
parameter
Data
downloads
Remarks
method value unit method value
1 QC1DB MEAN   counts/sec VAL100,600 0 flux this | last_yr | all NASMYTH flat lamp, Argus L543.1 setting
2 QC1DB none   counts/sec none  2 flux this | last_yr | all flux vs. wavelength, for all Argus LR
2 QC1DB none   counts/sec none  0 flux this | last_yr | all same, for all Argus HR
2 QC1DB none   counts/sec none  0 flux this | last_yr | all same, for Argus L543.1
*Data sources: QC1DB: QC1 database; LOCAL: local data source
Plot 1
scores: 1|
data source:giraffe_flat
(QC1 database)
dataset:flux
mean:no datacounts/sec
fixed thresholds:100...600counts/sec
N_data plotted:0
[click plot for closeup]
Plot 2
scores: not implemented
data source:giraffe_flat
(QC1 database)
dataset:
(numbers below apply to this dataset)
flux
average:none
thresholds:none
N_data plotted:2
[click plot for closeup]
This plot

This is the trending plot for the stability of the GIRAFFE nasmyth flat calibration lamp. It is based on NASMYTH flats (flattype=NAS) taken in the L543.1 setting of the Argus IFU.

These data are acquired everytime the standard star efficiency monitoring is executed (every 1-2 months). Furthermore it may also be triggered by a SCIENCE OB and a standard star exposure.

The average flux is obtained by dividing the average signal in the first raw file by the EXPTIME.

The last plot in the trending report collects all existing nasmyth lamp data for Argus, to give an indication about the wavelength dependency of the lamp efficiency.  


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