ESO
SINFONI Pipeline User Manual
Doc:
VLT-MAN-ESO-19500-3600
Issue:
Issue 1.0
Date:
Date 2005-10-19
Page:
38 of 88
7
Static Calibration Data
In the following section ancillary data required for SINFONI data reduction are listed. For each of them we
indicate the corresponding value of the HIERARCH ESO PRO CATG, in short PRO.CATG, FITS keyword.
This has to be used to identify the frames listed in the Set of Frames (see Section 4.2.2, page 22).
7.1
Line reference table
A reference list of arc lines is necessary to perform the wavelength calibration. Its PRO.CATG is REF_LINE_ARC.
This frame is an input of the recipes si_rec_distortion and si_rec_wavecal.
7.2
DRS setup table
There are a few data reduction parameters which are band dependent and are supposed not to change. Those are
collected in a table having PRO.CATG DRS_SETUP_WAVE. This frame is an input of the recipes si_rec_distortion
and si_rec_wavecal.
band
W_START
W_DISP1
W_DISP2
W_HW
W_FWHM
W_MIN_AMP
W_LOW_POS
W_HI_POS
H
1.65
-2.00018796022e-4
9.3034524287e-10
7
2.83
5
750
1000
H+K
1.95
-5.001433e-4
4.567277e-9
8
3.00
2
1100
1260
K
2.20
-2.51669e-4
1.77136e-9
4
2.00
1
760
900
J
1.25
-1.500581e-4
5.8870678e-10
8
2.00
2
980
1175
This table set the values for data reduction parameters which in section 10 are respectively called begin_wave,
guess_disp1, guess_disp2, half_width, fwhm, min_amp, lo_pos, hi_pos.
7.3
Reference bad pixel map
Detector defects are logged as bad pixels in a special mask having PRO.CATG REF_BP_MAP. This is an input
of the recipe si_rec_mflat.
7.4
First column reference table
The data reduction requires as input also a frame indication the first column of the first slitlet. Its PRO.CATG is
FIRST_COLUMN. It is an input of the recipes si_rec_wavecal, si_rec_objnod, si_rec_psf, si_rec_stdstar.
