This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey).
|
|
|
|
|
bottom
plots
|
contact
|
|
NAME |
kmos_acq.py
|
|
VERSION |
0.9 -- copied from kmos_acq.py v1.0.5 (2013-11-28)
0.9.1 -- usage of qc_imaovw instead of kmos_ifudsp (2014-01-28)
0.9.2 -- usage of argparse module (2014-03-10)
1.0 -- ingest into QC1 database
|
|
SYNTAX |
PYTHON
|
|
CALL |
processQC
from $DFS_PRODUCT/ASTROMETRY/$DATE
/home/python/kmos_ast.py -i -a $AB
|
|
INSTRUMENT |
KMOS
|
|
RAWTYPE |
ASTROMETRY
|
|
PURPOSE |
QC check of astrometry exposures
|
|
PROCINPUT |
reconstructed astrometry frames
|
|
QC1TABLE |
trending | table(s) in QC1 database:
kmos_acq
|
|
TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_AST_XCENT_1_HC.html |
trend_report_AST_XCENT_2_HC.html |
trend_report_AST_XCENT_3_HC.html |
trend_report_AST_YCENT_1_HC.html |
trend_report_AST_YCENT_2_HC.html |
trend_report_AST_YCENT_3_HC.html
|
|
QC1PAGE |
trending | associated documentation: none
|
|
QC1PLOTS
top |
ast1.png
reconstructed images for 24 IFUs;
not all IFUs are always used
|
|
QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: fit_xcent_ifu01 | ... | fit_xcent_ifu24
fit_ycent_ifu01 | ... | fit_ycent_ifu24
|
|
ALGORITHM |
fit_xcent_ifun: x centroid of target in IFUn
fit_ycent_ifun: y centroid of target in IFUn
|
|
CERTIF |
Astrometry frames are processed for trending purposes.
They are used to on Paranal to update the LUTs that are used during the acquisition process
for image reconstruction.
Only frames without any targets or with an obvious malfunctioning
of the instrument would be rejected and the QC1 parameters hidden.
|
|
COMMENTS |
None
|
top |
[2015-10-29T10:47:09] created by qcDocu v1.1.2, a tqs tool
|