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 |
vimos_sciifu.py
|
|
VERSION |
1.0 -- copied from vimos_stdifu.py (December 2009/February 2010)
1.0.1 -- bug fix in case of empty MASSOC list (2010-09-14)
1.0.2 -- skip call of scoreQC (2011-05-31)
1.0.3 -- create cover sheet (2011-09-01)
|
|
SYNTAX |
PYTHON
|
|
CALL |
processQC
from $DFS_PRODUCT/STD_IFU/$DATE
/home/vimos/python/vimos_ifusci.py -i -a $AB
|
|
INSTRUMENT |
VIMOS
|
|
RAWTYPE |
SCI_IFU
|
|
PURPOSE |
QC check of IFU science products
|
|
PROCINPUT |
products: IFU_SCIENCE_REDUCED, IFU_FOV
static: GRISM_TABLE
|
|
QC1TABLE |
trending | table(s) in QC1 database:
vimos_ifu_sci
|
|
TRENDPLOT |
trending | HealthCheck plot associated to this procedure: none
|
|
QC1PAGE |
trending | associated documentation: none
|
|
QC1PLOTS
top |
sciifu1.png
upper panels: extracted spectra for three fibres
lower left panels: details of sky spectrum with comparison to nominal wavelengths
of sky lines
lower right panel: reconstructed field of view; combined image for all 4 quadrants
sciifu2.png
upper panel: IFU_SCIENCE_REDUCED, 2D image of all fibre spectra
lower panel: IFU_SCIENCE_REDUCED, detail of central area
|
|
QC1PARAM |
QC1 parameters written in QC1 database: ids_rms | num_lost_total
|
|
ALGORITHM |
Description of algorithms:
ids_rms: rms of dispersion solution, taken from calibration
num_lost_total: total number of fibres that could not be calibrated
|
|
CERTIF |
Reasons for notes in GEN_INFO/NOTES.txt:
IFU image not well reconstructed (zigzag pattern);
not well wavelength-calibrated, i.e. skylines at wrong positions
|
|
COMMENTS |
NONE
|
top |
[2016-03-11T12:31:33] created by qcDocu v1.1.2, a tqs tool
|