QC documentation system: QC procedure xshooter_sci_slit_nodoff.py for XSHOOTER

This documentation is intended both for QC scientists and SciOps astronomers (who may want to ignore the technical information displayed in grey).
 
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xshooter_bias.py xshooter_dark.py xshooter_dark_nir.py xshooter_detlin.py
xshooter_fmtchk.py xshooter_orderdef.py xshooter_wave.py xshooter_flexure.py
xshooter_flat_slit.py xshooter_arc_slit.py xshooter_flat_ifu.py xshooter_arc_ifu.py
xshooter_std_slit_stare.py xshooter_std_slit_nodoff.py
xshooter_sci_slit_stare.py xshooter_sci_slit_nodoff.py
xshooter_sci_ifu.py
 
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NAME xshooter_sci_slit_nodoff.py
VERSION 1.0 -- September 2009
SYNTAX PYTHON
CALL processQC
from $DFS_PRODUCT/<RAWTYPE>/$DATE
/home/python/xshooter_sci_slit_nod.py -i -a $AB
INSTRUMENT XSHOOTER
RAWTYPE SCI_SLIT_NOD_NIR | SCI_SLIT_NOD_UVB | SCI_SLIT_NOD_VIS
SCI_SLIT_OFF_NIR | SCI_SLIT_OFF_UVB | SCI_SLIT_OFF_VIS
PURPOSE QC check of processed science exposures, extracted spectra, and other products
PROCINPUT product science frames
QC1TABLE trending | table(s) in QC1 database:
xshooter_sci_slit
TRENDPLOT trending | HealthCheck plot associated to this procedure: none
QC1PAGE trending | associated documentation:
standard_qc1.html
QC1PLOTS
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sci_slit_nod_VIS_A02.png
full display of merged 2D frame, broken in four parts
sci_slit_nod_VIS_A03.png
full display of merged 2D frame
sci_slit_nod_VIS_X00.png
1D spectrum, orders highlighted by shifts
sci_slit_nod_VIS_X04.png
Moffat function fit to line spread function to monitor spectrum curvature
sci_slit_nod_VIS_X14.png
molecfit best fit to wavelength fitting regions
sci_slit_nod_VIS_X10.png
telluric std transmission applied spectrum part1 (very blue)
sci_slit_nod_VIS_X11.png
telluric std transmission applied spectrum part2 (blue)
sci_slit_nod_VIS_X12.png
telluric std transmission applied spectrum part3 (red)
sci_slit_nod_VIS_X13.png
telluric std transmission applied spectrum part4 (very red)

sci_slit_nod_NIR_A02.png
full display of merged 2D frame, broken in four parts
sci_slit_nod_NIR_A03.png
full display of merged 2D frame
sci_slit_nod_NIR_X00.png
1D spectrum, orders highlighted by shifts
sci_slit_nod_NIR_X04.png
Moffat function fit to line spread function to monitor spectrum curvature
sci_slit_nod_NIR_X14.png
molecfit best fit to wavelength fitting regions
sci_slit_nod_NIR_X10.png
telluric std transmission applied spectrum part1 (very blue)
sci_slit_nod_NIR_X11.png
telluric std transmission applied spectrum part2 (blue)
sci_slit_nod_NIR_X12.png
telluric std transmission applied spectrum part3 (red)
sci_slit_nod_NIR_X13.png
telluric std transmission applied spectrum part4 (very red)
QC1PARAM QC1 parameters written in QC1 database:
# QC1db names: flux<i> (i=1...3) | err<i> (i=1...3) | sn<i> (i=1...3) | npix_sat | npix_high
FITS key names: QC.FLUXi.VAL (i=1...3) | QC.FLUXi.ERR (i=1...3) | QC.FLUXi.SN (i=1...3) | QC.NPIXSAT | num_sat
ALGORITHM
CERTIF Reasons for rejection:
saturation
COMMENTS
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