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ISAAC
pipeline:
old (up to 2005) product naming scheme |
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List
of codes for ISAAC pipeline products
Names
of calibration products follow a certain naming convention. This is done to have
human-readable names rather than archive or original file names. The naming scheme
has been chosen to have the type of product, its date of creation, and its pipeline-relevant
parameter values all recognizable from its name. With period 67, also an
instrument code is added. Instrument code
With the begin of period 67
(2001-04-01), all ISAAC calibration product names start with IS_ in order to be
able to distinguish between, e.g., spectroscopic flat frames from FORS and ISAAC
in case of archive downloads. The other VLT instruments follow the same scheme,
i.e. their calibration products also start with a 2letter instrument code.
All
earlier files delivered carry the old names without instrument code.
Type
of product
The type of product is coded
with four letters:
1st
letter | S or L | short or long wavelength
arm | 2nd letter | .I,
S.or G | imaging, spectroscopy or generic | |
The following types of calibration products
presently exist *)
Code | Type
of file | IS_SIDK | short
wavelength imaging dark | IS_SITF | short
wavelength imaging twilight flat | IS_GIZP | short
wavelength generic imaging zero point | IS_SSDK | short
wavelength spectroscopic dark | IS_SIIL | short
wavelength imaging illumination | | |
IS_SSFL | short wavelength spectroscopic
flat low resolution | IS_SSFM | short
wavelength spectroscopic flat medium resolution | IS_SSAL | short
wavelength spectroscopic arc table low resolution | IS_SSAM | short
wavelength spectroscopic arc table medium resolution | IS_SSSL | short
wavelength spectroscopic standard low resolution | IS_SSSM |
short wavelength spectroscopic standard medium resolution |
IS_SSST | short wavelength
spectroscopy startrace | | |
IS_LGDD | long
wavelength generic dark DoubleCorrelatedHigh readout | IS_LGDU | long
wavelength generik dark Uncorr readout | IS_LGDF | long
wavelength generic dark Fowlersampling readout | IS_LITF | long
wavelength imaging twilight flat | IS_LISF | long
wavelength imaging sky flat | IS_LIZP | long
wavelength imaging zero point | IS_LIIL | long
wavelength imaging illumination | IS_LILI | long
wavelength imaging linearity | | |
IS_LSAL | long wavelength
spectroscopic arc tabler low resolution | IS_LSAM | long
wavelength spectroscopic arc table medium resolution | IS_LSFL | long
wavelength spectroscopic flat low resolution | IS_LSFM | long
wavelength spectroscopic flat medium resolution | IS_LSST | long
wavelength spectroscopy startrace | |
The following types of science products presently
exist:
Code | Type
of file | IS_SIJC | short
wavelength imaging jittered coadded | IS_SSCL | short
wavelength spectroscopy coadded LowRes grating | IS_SSCM | short
wavelength spectroscopy coadded MedRes grating | | |
IS_LIJC | long
wavelength imaging jittered coadded | IS_LSCL | long
wavelength spectroscopy coadded LowRes grating | IS_LSCM | long
wavelength spectroscopy coadded MedRes grating | |
Date
of origin, version
The date of origin is identical to the
date of the raw data measurement. It is coded as, e.g., YYMMDD (e.g. 000915 for
Oct 15, 2000). The version of a file is indicated by capital letters always starting
with A.
Instrumental
parameters
Those parameters which are relevant for the specific
type of calibration product are included in its name.
- Darks, like SIDK,
SSDK, LGDU, LGDF and LGDD, the DIT (discrete integration time) is given (e.g.
IS_SIDK_011025B_DIT=10.fits)
- GIZP is coded as <UT>_<STD>_<FILTER>
(e.g. IS_GIZP_011104A_08_S842E_Js.paf)
- SITF, the filter is given (e.g.
IS_SITF_012212_Ks.fits)
- spectroscopic arcs use <FILTER>_<SLIT>_<WLEN>_<LAMP>
(e.g. IS_SSAL_012205A_SK_s06t_2202_Xe.tfits)
- spectroscopic flats use <FILTER>_<SLIT>_<WLEN>
(e.g. IS_SSFM_011104A_J_sl1_1253.fits)
- science images use <FILTER>_<OB>
- science
spectroscopy use <FILTER>_<SLIT>_<WLEN>_<OB>
- spectroscopic
standards use <STD>_<FILTER>_<SLIT>_<WLEN>_<OB>
where
- STD is the name of the standard,
- WLEN is the central wavelength
in microns (2.102 micron is coded as 210 and 0.903 micron is coded as 090),
-
(since 2004-04-01) WLEN is the central wavelength in microns (2.102 micron is
coded as 2102 and 0.903 micron is coded as 0903),
- FILTER is either a
broad band or narrow band filter (e.g. Ks),
- SLIT is coded as sl1, sl2,
or s03t, where t is the abbreviation for tilted
- LAMP is coded as Xe or
Ar or Xe+Ar, dependent oln which calibration lamp is used.
- UT is coded
as hh (e.g. 03)
Extension
2D product images contain the .fits extension. 1D data with the
.tfits extension are given in fits table format. The pipeline provides
in addition VLT compliant plain ASCII parameter files with the .paf extension.
Extractions of the eclipse log file are given with a .log extension. The
pipeline jitter and spjitter recipes produce in addition ini files with the .ini
extension and a status file with the .ascii extension. The calibration
associtiation tools provide a calibration list with the .calibs extension.
Last update: Apr.. 23, 2004
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