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 |
qc_IFS_SPOS.sh
|
|
VERSION |
1.0 -- 2015-04-01 begin of operations
1.1 -- 2017-09-05 docu updated
|
|
SYNTAX |
SHELL
|
|
CALL |
called by processQC from $DFS_PRODUCT/IFS_SPOS/$DATE as
qc_IFS_SPOS -a $AB -level 1 2\>\&1 \> $DFS_LOG/$AB.qclog
meaning output is logged to $DFS_LOG/$AB.qclog !!!
|
|
INSTRUMENT |
SPHERE
|
|
RAWTYPE |
IFS_SPOS
|
|
PURPOSE |
quality control script for SPHERE IFS spectral positions pipeline products
level 0 : debug, implicit call of writeQC scoreQC.
level 1 : calls qc_mstplt.py -a $AB
|
|
PROCINPUT |
-a AB -level level
|
|
QC1TABLE |
trending | table(s) in QC1 database:
sphere_ifs_specpos
|
|
TRENDPLOT |
trending | HealthCheck plot(s) associated to this procedure:
trend_report_IFS_SPOS_YJ_HC.html |
trend_report_IFS_SPOS_YJH_HC.html |
../../../ALL/ref_frames/ref_sphere.html
|
|
QC1PAGE |
trending | associated documentation:
SP_IFS_spos_qc1.html
|
|
QC1PLOTS
top |
r.SPHER.2015-03-23T09:14:54.836_tpl_X00.png
standard cross sections and image zoom
|
|
QC1PARAM |
QC1 parameters written into QC1 table:
QC.NUMBER.SPECTRA, qc_number_spectra, number of used spectra
QC.SCALE.MEASURED qc_scale_measured, correcting scale
DRS.OFFSETX.MEASURED, qc_offset_x, offset applied to transformation
DRS.OFFSETY.MEASURED, qc_offset_y, offset applied to transformation
DRS.IFS.MAX.LAMBDA, qc_max_lambda
DRS.IFS.MIN.LAMBDA, qc_min_lambda
DRS.IFS.DISPERSION dispersion
DRS.DIST.X/Y.COEFF.0/3_0/3, qc_dist_x/y_0/3_0/3, polynomial coefficients for optical disrotion correction
|
|
ALGORITHM |
Description of algorithms:
see pipeline user manual
|
|
CERTIF |
Reasons for rejection
|
|
COMMENTS |
the lamp counts are not monitored
|
top |
[2017-12-22T12:30:38] created by qcDocu v1.1.2, a tqs tool
|