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Health Check monitor

 

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SINFONI:
image quality
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SINFONI trending system: HEALTH CHECK report
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Last update: 2019-06-28T05:03:59 (UT)
  | now: 2024-11-25T21:04:47 (UT) muc04 QC pipeline: sinfo-3.2.5 (installed 2019-05-09)
same group: STD_image_quality:_J H K H+K   PSF_image_quality:_J H K H+K
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.
SINFONI news: 2019-06-26: SINFONI taken out of operations
Report news:
DATE*: [?] 2019-06-24
report | NLT
2019-06-25
report | NLT
2019-06-26
no data | NLT
2019-06-27
no data | NLT
2019-06-28
no data | NLT
2019-06-29
no data | NLT
2019-06-30
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
The STD stars are not from an homogenous set
If an outlier is detected, this could be a problem with atmospheric conditions or a known instrumental issue,
- atmospheric conditions or know instrumental issues should be indicated in the NR
- after analysis by QC (this could take a few days), the reason will be visible under "scores&comments", if this is a false alert (object too faint for ex.), the QC scientist will force the flag to become green
NOTE: Large negative outliers in the delta FWHM values of the Delta_IQ plot are the result of a missing DIMM keyword in the STD image.
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   arcsec none  100 qc_fwhm_sinfo this | last_yr | all sinfoni STD fwhm vs. corrected DIMM seeing (arcsec) with line of equivalence plotted [H+K-band].
CLOSED loop AO.
1 oQC1DB none   arcsec none  18 qc_fwhm_sinfo this | last_yr | all sinfoni STD fwhm vs. corrected DIMM seeing (arcsec) with line of equivalence plotted [H+K-band].
OPEN loop AO.
2 QC1DB MEDIAN -0.32 arcsec VAL-1000.0,0.15 100 qc_delta_fwhm this | last_yr | all delta FWHM = (sinfoni STD fwhm - corrected DIMM seeing) (arcsec) [H+K-band].
CLOSED loop AO. This data set is scored!
3 oQC1DB MEDIAN 0.176 arcsec VAL-1000.0,1.0 18 qc_delta_fwhm this | last_yr | all delta FWHM = (sinfoni STD fwhm - corrected DIMM seeing) (arcsec) [H+K-band].
OPEN loop non-AO. This data set is scored!
*Data sources: QC1DB: QC1 database; LOCAL: local data source
Plot 1
scores: not implemented
data source:sinfoni_std
(QC1 database)
dataset:
(numbers below apply to this dataset)
qc_fwhm_sinfo
average:none
thresholds:none
N_data plotted:100
[click plot for closeup]
Plot 2
scores: 8|
data source:sinfoni_std
(QC1 database)
dataset:qc_delta_fwhm
median:-0.32arcsec
fixed thresholds:-1000.0...0.15arcsec
N_data plotted:100
[click plot for closeup]
Plot 3
scores: 3|
data source:sinfoni_std
(QC1 database)
dataset:qc_delta_fwhmo
median:0.176arcsec
fixed thresholds:-1000.0...1.0arcsec
N_data plotted:18
[click plot for closeup]
This plot

These are the trending plots for the SINFONI QC parameters defined for the image quality as measured for the telluric standard stars
(H+K-band / all pixel scales).

Plot #1 is a one-to-one comparison of the image quality achieved by SINFONI and the seeing as measured by the DIMM site-monitor. The DIMM seeing has been adjusted to the wavelength and airmass of the standard star observation. The image quality (IQ) plot shows the FWHM of the STD star and the corrected DIMM plotted against one another. CLOSED loop (AO) observations are plotted as solid circles, while OPEN loop (non-AO) observations are shown as open circles.

Plot #2 shows Delta_IQ = sinfoni telluric standard star FWHM - DIMM seeing for all observations with SINFONI in CLOSED loop mode.
This parameter is scored.

Plot #3 shows Delta_IQ = sinfoni telluric standard star FWHM - DIMM seeing for all observations with SINFONI in OPEN loop mode.
This parameter is scored.

NOTE: The conversion from pixels to arcsec for the image FWHM takes into account the fact that the reconstructed SINFONI cube has rectangular pixels. The reconstructed pixels are such that on-sky Delta_X = 0.5*Delta_Y.
The correct conversion, in terms of the source position angle (PA), is given by:
SINFONI FWHM computation the pixel_scale is given by the keyword INS.OPTI1.NAME.

Find more information about SINFONI STD calibration data here.
Other QC parameters are also trended here.  


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