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 |
muse_skyflat.py
|
|
VERSION |
1.0 -- copied from v. 0.1 when Muse became operational September 2014
|
|
SYNTAX |
PYTHON
|
|
CALL |
processQC
from $DFS_PRODUCT/SKY_FLAT/$DATE
/home/muse/python/muse_skyflat.py -i -a $AB
|
|
INSTRUMENT |
MUSE
|
|
RAWTYPE |
SKY_FLAT
|
|
PURPOSE |
QC check on raw and master sky flat frames
check done per CHANEL/IFU (x24) of the raw and master skyflat frames
|
|
PROCINPUT |
raw skyflat frames and MASTER_SKYFLAT product
|
|
QC1TABLE |
trending | table(s) in QC1 database:
muse_skyflat
|
|
TRENDPLOT |
trending | HealthCheck plot associated to this procedure: none
|
|
QC1PAGE |
trending | associated documentation: none
|
|
QC1PLOTS
top |
skyflat0.png
upper left panel: cuts through first raw frame and master skyflat in X direction
upper middle panel: cuts through first raw frame and master skyflat in Y direction
upper right panel: histrograms of first raw frame and master, Gauss fit to master
central left panel: cuts through first raw frame and master in X direction, central area
central middle panel: cuts through first raw frame and master in Y direction, central area
central right panel: row and column averages of master
lower left panel: comparison to reference (current master - reference), cut in X direction
lower middle panel: comparison to reference (current master - reference), cut in Y direction
lower right panel: comparison to reference, histogram
|
|
QC1PARAM |
QC1 parameters written in QC1 database:
QC1 DB names: skyflat_intflux | skyflat_median | skyflat_mean | skyflat_stdev | skyflat_min |
skyflat_max | skyflat_nsaturated | skyflat_slice1/../48_intflux
ALL parameters are calculated by the pipeline recipe
|
|
ALGORITHM |
Description of algorithms:
skyflat_intflux: flux integrated over the whole master skyflat (all slices)
skyflat_median: median of the master skyflat
skyflat_mean: mean of the master skyflat
skyflat_stdev: standard deviation of the master skyflat
skyflat_min: minimum value of the master skyflat
skyflat_max: maximum value of the master skyflat
skyflat_nsaturated: number of saturated pixels in output data
skyflat_slice1/../48_intflux: flux integrated over slice1/../48
|
|
CERTIF |
Reasons for rejection:
unusual high/low flux level
|
|
COMMENTS |
based on original Python script from March 2014
|
top |
[2015-11-05T15:00:15] created by qcDocu v1.1.2, a tqs tool
|