The names of all pipeline products follow a certain naming convention. This is done to have human-readable rather than technical 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 the product name.
Since the begin of period 75 (April 2005), both science and calibration product files are renamed. (Actually, there was a transition phase extending for some instruments from April towards the end of the year 2005).
Before that date only calibration products followed the common scheme which is described here. (Some instruments had their own naming scheme which is described below, if applicable).
The general format of user-oriented product file names is the same for all VLT/VLTI instruments.
Instrument code
All pipeline product names start with two letters which are specific for the instrument. For instance: UVES product names start with 'UV', VISIR names with 'VR'.
Type of product
Next, the product type is coded. The full value is coded in the fits header key HIERARCH.ESO.PRO.CATG. A short form of this tag is coded in four characters being unique per instrument:
1st letter
M or P
calibration product
S
science product
G
general calibration product (as of P82)
2nd to 4th letter
...
type of product
CALIBRATION
PRODUCT CODES
Naming scheme
The naming scheme has the product type, the date
of creation, and pipeline-relevant parameter values all recognisable from
its name. The general scheme is:
VI_<TYPE>_<DATE><VERSION>_<PARAMS>.<SUFFIX>
.
Type of product
The following types of calibration products presently
exist:
CODE
TYPE OF FILE
PRO_CATG
VIMOS MODE
VERSIONING?
MBIA
master bias
MASTER_BIAS
IMG, MOS, IFU
no
MDRK
master dark
MASTER_DARK
IMG, MOS, IFU
yes
MKFI
master sky flat
IMG_MASTER_SKY_FLAT
IMG
yes
PSTI
reduced standard star field
IMG_STANDARD_REDUCED
IMG
yes
PZPI
zeropoint table
PHOTOMETRIC_TABLE
IMG
no
Products of new MOS pipeline (V2.3.9 and later, since August 2010)
MSFM
master flat through MOS mask
MOS_MASTER_SCREEN_FLAT
MOS
yes
PDCM
dispersion coefficients
MOS_DISP_COEFF
MOS
yes
PCCM
slit curvature coefficients
MOS_CURV_COEFF
MOS
yes
PSLM
slit location table
MOS_SLIT_LOCATION
MOS
yes
PWXM
extracted arc lamp spectrum
MOS_ARC_SPECTRUM_EXTRACTED
MOS
yes
PRSM
spectrophotomtric response
MOS_SPECPHOT_TABLE
MOS
yes
PSRM
reduced standard star spectrum
MOS_STANDARD_REDUCED
MOS
yes
Products of old MOS pipeline (V2.2.8 or earlier, until May 2010)
MSFM
master flat through MOS mask
MOS_MASTER_SCREEN_FLAT
MOS
yes
PWDM
inverse dispersion solution
EXTRACT_TABLE
MOS
yes
PRSM
spectrophotometric response
MOS_SPECPHOT_TABLE or
MOS_MASTER_RESPONSE*
MOS
yes
PSRM
reduced standard star
MOS_STANDARD_REDUCED
MOS
yes
PTCF
fibre identification
IFU_TRACE
IFU
yes
PTNF
fibre transmission correction
IFU_TRANSMISSION
IFU
yes
PWDF
inverse dispersion solution
IFU_IDS
IFU
yes
MXFF
extracted flat spectrum per fibre
IFU_FLAT_SPECTRUM_EXTRACTED
IFU
yes
STRF
reduced fibre spectra
IFU_STANDARD_REDUCED
IFU
yes
STFF
reconstructed image of field of view
IFU_STANDARD_FOV
IFU
yes
PRSF
response curve
IFU_SPECPHOT_TABLE or
IFU_MASTER_RESPONSE*
IFU
yes
* master response curves are averages of several individual measurements
Date of origin,
version
The date of origin is identical to the date of the raw data measurement.
It is coded as, e.g., 051015 for Oct 15,
2005. The version of a file is indicated by capital letters always starting
with A.
Versioning is supported for most types of files (see table above). In
the remaining cases, only one version per day is created (version is always
A).
Instrumental
parameters
Those parameters which are relevant for the specific type of calibration
product are included in its name. The following schemes are used:
PARAMETER CODE
USED FOR FILE
TYPES
VIMOS MODE
Q<QUAD>_<GAIN>
MBIA, MDRK
IMG, MOS, IFU
<FILT>_Q<QUAD>_<GAIN>
MKFI, PSTI, PZPI
IMG
<ORDFLT>_<GRISM>_<MASK>_Q<QUAD>_<GAIN>
MSFM, PWDM, PRSM, PSRM
MOS
<ORDFLT>_<GRISM>_<IFUMAG><IFUSHUT>_Q<QUAD>_<GAIN>
PTCF, PTNF, PWDF
IFU
where
PARAMETER
EXPLANATION
VALUES
<QUAD>
instrument quadrant (channel)
1, 2, 3, 4
<GAIN>
detector gain
lo: low gain, used for imaging; hi: high gain,
used for spectroscopy
The master files have extension .fits, while most product files are tables
and have extension .tfits .
Examples
BIAS:
VI_MBIA_051002A_Q1_lo.fits is the (first and only) master bias for imaging
(low gain) for quadrant 1 from 2005-10-02.
VI_MBIA_051002A_Q3_hi.fits is the (first and only) master bias for spectroscopy
(high gain) for quadrant 3 from 2005-10-02.
IMG:
VI_MKFI_050912B_I_Q2_lo.fits is the second (from at least two) master
sky flats for the I filter and quadrant 2 from 2005-09-12.
MOS:
VI_PWDM_041212A_GG475_MR_200945_Q4_hi.tfits is a MOS dispersion solution
for the MR grism with filter GG475, taken for the mask ID 200945 in quadrant
4.
IFU:
VI_PTCF_051002C_GG435_HRo_1ON_Q1_hi.tfits is a fibre indentification
table for the HR_orange grism with filter GG435 for quadrant 1, IFU magnification
is 1, IFU shutter is on.
STATIC
PRODUCTS
Naming scheme
The naming scheme has the product type, a date,
and a name or relevant instrument parameters. The general scheme is:
VI_<TYPE>_<DATE><VERSION>_<PARAMS>.<SUFFIX>
or
VI_<TYPE>_<DATE><VERSION>_<NAME>.<SUFFIX>
.
Type of product
The following types of static calibrations presently
exist:
CODE
TYPE OF FILE
VIMOS MODE
GBPM
CCD table (bad pixel map)
ALL
GEXT
extinction table
ALL
GCFG
spectroscopic configuration table
MOS/IFU
GGRS
grism table
MOS/IFU
GIDT
IFU fibre identification
IFU
GRSF
IFU master response
IFU
GCAT
line catalog
MOS/IFU
GRSM
MOS master response
MOS
GPHO
photometric catalog
IMG
GFLX
spectrophotometric standards
MOS/IFU
SCIENCE
PRODUCT CODES
Naming scheme
The naming scheme has the product type, the ID
of the observation block, a time stamp, and pipeline-relevant parameter
values all recognisable from its name. The general scheme is:
VI_<TYPE>_<OB_ID>_<TIMESTAMP>_<PARAMS>.<SUFFIX>
.
Type of product
The following types of calibration products presently
exist:
CODE
TYPE OF FILE
PRO_CATG
VIMOS MODE
SREI
reduced science image
IMG_SCIENCE_REDUCED
IMG
Products of new MOS pipeline (V2.3.9 and later, since August 2010)
SREM
reduced spectra of detected objects
MOS_SCIENCE_REDUCED
MOS
SERM
error of reduced spectra
MOS_SCI_ERROR_REDUCED
MOS
SEXM
extracted spectra (2D) per slit
MOS_SCIENCE_EXTRACTED
MOS
SSKM
sky spectra per slit
MOS_SCIENCE_SKY
MOS
SSEM
sky+object per slit
MOS_SCIENCE_SKY_EXTRACTED
MOS
SSRM
sky spectra, 1D per slit
MOS_SCI_SKY_REDUCED
MOS
SOTM
table of detected objects
OBJECT_SCI_TABLE
MOS
SFRM
fringe map
MOS_SCI_FRINGES
MOS
SRFM
flux-calibrated spectra
MOS_SCIENCE_FLUX_REDUCED
MOS
SEFM
error of flux-calibrated spectra
MOS_SCI_ERROR_FLUX_REDUCED
MOS
Products of old MOS pipeline (V2.2.8 or earlier, until May 2010)
SREM
reduced spectra of objects found
MOS_SCIENCE_REDUCED
MOS
SRFM
flux calibrated spectra
MOS_SCIENCE_FLUX_REDUCED
MOS
SEXM
extracted spectra per slit
MOS_SCIENCE_EXTRACTED
MOS
SSKM
sky spectra per slit
MOS_SCIENCE_SKY
MOS
SSRM
sky spectra per object
MOS_SKY_REDUCED
MOS
SOTM
table for object identification
OBJECT_TABLE
MOS
SWTM
object positions on slit
WINDOW_TABLE
MOS
SFRM
fringe map*
MOS_FRINGES
MOS
SREF
reduced spectra per fibre
IFU_SCIENCE_REDUCED
IFU
SRFF
flux calibrated spectra
IFU_SCIENCE_FLUX_REDUCED
IFU
SSVF
reconstructed image of field of view
IFU_FOV
IFU
* The fringe map is produced only for jittered MOS observations with LR_red
or HR_red grisms
if the offset between the frames is at least four pixels.
OB ID
The ID of the observation block that has been used to measure the raw
science frame. It has usually six digits, e.g. 154718.
Time stamp
The time stamp has the form <YEAR>-<MONTH>-<DAY>T<HOUR>:<MINUTE>:<SECOND>.<MILLISEC>.
It has the same value that is used in the archive filename of the raw
file, e.g. 2005-01-18T04:45:19.435.
Instrumental
parameters
The instrumental parameters for the science frames are the same as for
the calibrations in order to identy matching files. These three schemes
are used:
PARAMETER CODE
USED FOR FILE
TYPES
VIMOS MODE
<FILT>_Q<QUAD>_<GAIN>
SREI
IMG
<ORDFLT>_<GRISM>_<MASK>_Q<QUAD>_<GAIN>
SREM, SEXM, SSKM, SSRM, SOTM, SWTM, SFRM
MOS
<ORDFLT>_<GRISM>_<IFUMAG><IFUSHUT>_Q<QUAD>_<GAIN>
SREF, SSVF
IFU
where
PARAMETER
EXPLANATION
VALUES
<QUAD>
instrument quadrant (channel)
1, 2, 3, 4
<GAIN>
detector gain
lo: low gain, used for imaging; hi: high gain,
used for spectroscopy
Most files have extension .fits, while some product files are tables
and have extension .tfits .
Example
VI_SREI_199201_2005-10-02T05:33:39.651_R_Q1.fits: reduced science image,
the ID of the OB was 199201, the raw file was measured on 2 October 2005
at 05:33:39.651 (UT). The R filter has been used; the file is from quadrant
1.