VLT-MAN-ESO-14650-4942
P96
24.06.2015
104 of 161
ESO, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
6. Calibrating and reducing X-shooter data
6.1 X-shooter calibration plan
The calibration plan has been revised during P86, P87, P88, P89, it is now implemented as
indicated below. A better follow-up of and new long term calibrations have been included.
A summary of the calibration plan manual is given in Table 15 and 17.
Table 15: X-shooter calibration plan summary
Master bias and check CCD bias
properties
Master dark, bad pix. map
IFU FF for monitoring of the
UVB/VIS ADCs and the IFU
5/setting D
2
lamp
5/setting halo.
lamp
Pixel-to-pixel variations, blaze
function correction when triggered
by science
Arcs single
pinhole (Th/Ar or
Ar/Xe/Hg/Kr)
Pipeline calibration: first guess
disp. solution.
FMCK
Pipeline calibration: order
localization ORDERDEF
1x1 binning in UVB/VIS
Arcs multi-pinhole
(Th/Ar or
Ar/Xe/Hg/Kr)
Wavelength and spatial scale
determination/calibration
WAVE
Arcs through
slit/IFU
(Th/Ar or
Ar/Xe/Hg/Kr)
Wavelength shift between multi-
pinholes and slits, spectral
resolution, ARC, none taken in
2x2 due to remnants.
Multi-order definition taken on
request
Pipeline calibration: cube
reconstruction
Radial velocity
standard
c
Accurate radial vel. calibration
Correct for telluric abs. Only in
stare mode in SM up to P90, in
nodding starting from P91. No 5”
slits observations
Spectro-
photometric
standard
Response curve, absolute flux
calib. In nodding mode, in slit
mode it is taken every time the
instrument is used, in IFU mode,
only when the science performed
at night did it.
Twilight spectroscopic skyflats