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FORS2 Pipeline:
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List of codes for calibration products
(master files and other products)
Names of calibration products follow a certain naming
convention. This is done to have 'speaking names' for those products 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 instrumental, pipeline-relevant,
parameter values all recognizable from its name.
The type of product is coded with four letters:
1st letter | M or P | master file or product file |
2nd , 3rd letter | ... | type of product |
4th letter | I, L, M, S, X | mode (IMG, LSS, MOS, LSS-like MOS, MXU) |
The following types of calibration products presently exist:
Code | Type of file | Template Name | |
MBIA | master bias | F2_MBIA_<DATE>#_<C><GAIN>_<BIN> | |
MDRK | master dark | F2_MDRK_<DATE>#_<C><GAIN>_<BIN> | |
MSFI* | master screen flat (IMG) | F2_MSFI_<DATE>#_<FILT>_<C><GAIN>_<BIN><COLL> | |
MKFI | master sky flat (IMG) | F2_MKFI_<DATE>#_<FILT>_<C><GAIN>_<BIN><COLL> | |
MNFI | master night flat (IMG) | F2_MNFI_<DATE>#_<FILT>_<C><GAIN>_<BIN><COLL> | |
PSTI | reduced standard star (IMG) | F2_PSTI_<DATE>#_<C><GAIN>_<BIN><COLL> | |
PZPI | aligned photometry table (IMG) | F2_PZPI_<DATE>#_<C><GAIN><COLL> | |
PFLL* | reduced LAMP CHECK data (LSS) | F1_PFLL_<DATE>#<LAMP>_G<GRISM>_<FILT>_S<SLIT>_<GAIN>_<BIN>_<COLL> | |
MNFL | normalized master flat field (LSS) | F1_MNFL_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PWCL | dispersion coefficients (LSS) | F1_PWCL_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PSRL | spectral resolution table (LSS) | F1_PSRL_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PRLL | reduced arc lamp image (LSS) | F1_PRLL_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PWML | wavelength map image (LSS) | F1_PWML_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PSLL | slit location table (LSS) | F1_PSLL_<DATE>#_G<GRISM>_<FILT>_S<SLIT>_<C><GAIN>_<BIN>_<COLL> | |
PSOL | line shifts from sky lines (STD-LSS) | F1_PSOL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWSL | wavelength map image (STD-LSS) | F1_PWSL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PDCL | dispersion coefficients from sky line correction (STD-LSS) | F1_PDCL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PUKL | unmapped sky background (STD-LSS) | F1_PUKL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMAL | mapped image (STD-LSS) | F1_PMAL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMKL | mapped sky background (STD-LSS) | F1_PMKL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PUSL | unmapped image (STD-LSS) | F1_PUSL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMSL | mapped image (STD-LSS) | F1_PMSL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
POTL | table with object positions (STD-LSS) | F1_POTL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRKL | reduced sky spectrum (STD-LSS) | F1_PRKL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRSL | reduced object spectra (STD-LSS) | F1_PRSL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PREL | error of reduced object spectra (STD-LSS) | F1_PREL_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
MNFM | normalized master flat field (MOS) | F1_MNFM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWCM | dispersion coefficients (MOS) | F1_PWCM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSRM | spectral resolution table (MOS) | F1_PSRM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRLM | reduced arc lamp image (MOS) | F1_PRLM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWMM | wavelength map image (MOS) | F1_PWMM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSLM | slit location table (MOS) | F1_PSLM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PCCM | curvature coefficients table (MOS) | F1_PCCM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSMM | spatial map image (MOS) | F1_PSMM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
MNFS | normalized master flat field (LSS-like MOS) | F1_MNFS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWCS | dispersion coefficients (LSS-like MOS) | F1_PWCS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSRS | spectral resolution table (LSS-like MOS) | F1_PSRS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRLS | reduced arc lamp image (LSS-like MOS) | F1_PRLS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWMS | wavelength map image (LSS-like MOS) | F1_PWMS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSLS | slit location table (LSS-like MOS) | F1_PSLS_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSOM | line shifts from sky lines (STD-MOS) | F1_PSOM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWSM | wavelength map image (STD-MOS) | F1_PWSM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PDCM | dispersion coefficients from sky line correction (STD-MOS) | F1_PDCM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PUKM | unmapped sky background (STD-MOS) | F1_PUKM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMAM | mapped image (STD-MOS) | F1_PMAM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMKM | mapped sky background (STD-MOS) | F1_PMKM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PUSM | unmapped image (STD-MOS) | F1_PUSM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PMSM | mapped image (STD-MOS) | F1_PMSM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
POTM | table with object positions (STD-MOS) | F1_POTM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRKM | reduced sky spectrum (STD-MOS) | F1_PRKM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRSM | reduced object spectra (STD-MOS) | F1_PRSM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PREM | error of reduced object spectra (STD-MOS) | F1_PREM_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
MNFX | normalized master flat field (MXU) | F1_MNFX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWCX | dispersion coefficients (MXU) | F1_PWCX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSRX | spectral resolution table (MXU) | F1_PSRX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PRLX | reduced arc lamp image (MXU) | F1_PRLX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PWMX | wavelength map image (MXU) | F1_PWMX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSLX | slit location table (MXU) | F1_PSLX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PCCX | curvature coefficients table (MXU) | F1_PCCX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> | |
PSMX | spatial map image (MXU) | F1_PSMX_<DATE>#_G<GRISM>_<FILT>_S<MASK>_<C><GAIN>_<BIN><COLL> |
* These files are only used for internal purpose (quality control) and are not distributed in the Service Mode DVDs.
where:
<DATE>=Observing date as YYMMDD, e.g. 030401
#=sequential counter, e.g. A, B ...
<C>=chip number, e.g. C2
<GRISM>=Grism Name, e.g. 150I
<FILT>=Filter Name, e.g. V_BE or GG435
<SLIT>=Slit Width, e.g. 07 for 0.7"
<MASK>=MOS Checksum, e.g. m1955 (MOS), or MASK ID, e.g. p915243 (MXU)
<BIN>=Binning, e.g. 1x1
<COLL>=Collimator, e.g. s(tandard) or h(igh)
<LAMP>=Lamp Name, e.g. FlatBlue+1
<GAIN>=gain e.g. lo(w) or hi(gh)
Examples
F2_MBIA_030425B_C2lo_1x1.fits
F2_MDRK_030420A_C1hi_2x2.fits
F2_MSFI_030420A_VBE_C2lo_2x2s.fits
F2_MKFI_030423A_VBE_C2lo_2x2s.fits
F2_PSTI_030421A_VBE_C2lo_2x2s.fits
F2_PZPI_030421A_VBE_C2lo_2x2s.tfits
F2_PFLL_061023A_FlatRed3_G300V_GG435_S10C2hi_2x2s.fits
F2_MNFL_061026A_G300I_OG590_S13_C2hi_2x2s.fits
F2_PRLL_061026A_G300I_OG590_S13_C2hi_2x2s.fits
F2_PSLL_061026A_G300I_OG590_S13_C2hi_2x2s.tfits
F2_PSRL_061026A_G300I_OG590_S13_C2hi_2x2s.tfits
F2_PWCL_061026A_G300I_OG590_S13_C2hi_2x2s.tfits
F2_PWML_061026A_G300I_OG590_S13_C2hi_2x2s.fits
F2_MNFM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.fits
F2_PCCM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.tfits
F2_PRLM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.fits
F2_PSLM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.tfits
F2_PSMM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.fits
F2_PSRM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.tfits
F2_PWCM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.tfits
F2_PWMM_061020A_G300I_OG590_Sm2432_C1hi_2x2s.fits
F2_MNFS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.fits
F2_PRLS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.fits
F2_PSLS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.tfits
F2_PSRS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.tfits
F2_PWCS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.tfits
F2_PWMS_061029A_G300V_GG375_Sp33693_C1hi_2x2s.fits
F2_MNFX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.fits
F2_PCCX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.tfits
F2_PRLX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.fits
F2_PSLX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.tfits
F2_PSMX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.fits
F2_PSRX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.tfits
F2_PWCX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.tfits
F2_PWMX_061027A_G600z_OG590_Sp915243_C2hi_2x2s.fits
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