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LIST OF PIPELINE PRODUCTS CODES

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
<FILT> name of broadband filter U, B, V, R, I, z
<ORDFLT> name of order sorting filter OS-blue, OS-red, GG435, GG475; "_" for "free"
<GRISM> name of grism LRb: LR_blue; LRr: LR_red; MR; HRb: HR_blue; HRo: HR_orange; HRr: HR_red
<MASK> identifier of MOS mask 6 digits, e.g. 100320
<IFUMAG> IFU magnification 1, 2
<IFUSHUT> IFU shutter ON, OFF

Extension

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
<FILT> name of broadband filter U, B, V, R, I, z
<ORDFLT> name of order sorting filter OS-blue, OS-red, GG435, GG475; "_" for "free"
<GRISM> name of grism LRb: LR_blue; LRr: LR_red; MR; HRb: HR_blue; HRo: HR_orange; HRr: HR_red
<MASK> identifier of MOS mask 6 digits, e.g. 100320
<IFUMAG> IFU magnification 1, 2
<IFUSHUT> IFU shutter ON, OFF

Extension

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.

 


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