!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! ! ! SDDL Name: STIS_DISP.SDDL ! ! Purpose: This SDDL file defines the STIS_DISP relation. ! ! Modification History: ! ! Date OPR Who Reason ! -------- ------- --- ------------------------------------------------- ! 06/14/96 29753 Baum Original implementation ! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! ! ! LANGUAGE SQL RECORD STIS_DISP_TYPE !------------------------------------------------------------------------------ ! ! RECORD INFORMATION ! !------------------------------------------------------------------------------ DESCRIPTION "This relation is used to define the values OPUS needs for WCS calculations for observations using dispersive elements. There must be a record in this table for every STIS spectral element (except MIRROR and PRISM) and valid central wavelength (as listed in the proposal instructions). If significant MSM changes are made during the mission that requires different data for different observation times, the valid_date is used by OPUS to fetch the right record. " !------------------------------------------------------------------------------ ! ! FIELD INFORMATION ! !------------------------------------------------------------------------------ FIELD detector TYPE C8 DESCRIPTION "STIS/CCD, STIS/MA1, STIS/MA2 are the values of OPUS DGX keyword SS_DTCTR found in qelogsheet.config. " END_FIELD FIELD grating TYPE C8 DESCRIPTION "G140L,G140M,E140M,E140H,X140M,X140H,G230L,G230M,E230M, E230H,X230M,X230H,G230LB,G230MB,G430M,G750L,or G750M. These are the values from OPUS DGX keyword SS_GRTNG that come from qelogsheet.ap_1. " END_FIELD FIELD cen_wave TYPE I4 DESCRIPTION "The central wavelength supplied in the proposal and found in OPUS DGX keyword SS_CWAVE that comes from qelogsheet.min_wave. The allow values are in the proposal instructions. " END_FIELD FIELD valid_date TYPE C17 DESCRIPTION "YYYY.DDD:HH:MM:SS, the date-time of either the SMS which loads a new dither table or a time preceding the first STIS observation that uses a new dither table. " END_FIELD FIELD ref_wavelen TYPE R4 DESCRIPTION "Actual wavelength at reference pixel (Angstrom)" END_FIELD FIELD disp_angle TYPE R4 DESCRIPTION "Degrees from axis1 toward axis2 for dispersion. " END_FIELD FIELD dispersion TYPE R4 DESCRIPTION "Change is wavelength (Angstrom) per pixel. " END_FIELD FIELD scale TYPE R4 DESCRIPTION "Change in sky arcsec along slit per pixel. " END_FIELD FIELD spec_res TYPE R4 DESCRIPTION "Resolving power at central wavelength. " END_FIELD FIELD min_wave TYPE R4 DESCRIPTION "Minimum wavelength in spectrum. " END_FIELD FIELD max_wave TYPE R4 DESCRIPTION "Maximum wavelength in spectrum. " END_FIELD END_RECORD !------------------------------------------------------------------------------ ! ! RELATION DECLARATION ! !------------------------------------------------------------------------------ RELATION stis_disp TYPE STIS_DISP_TYPE DESCRIPTION "STIS Dispersion Relation" SUBSYSTEM_USING "OPUS" INDEX stis_disp_1 TYPE unique, clustered FIELDS detector,grating,cen_wave,valid_date END_INDEX END_RELATION !------------------------------------------------------------------------------ ! ! INSTANCE DECLARATION ! !------------------------------------------------------------------------------ INSTANCE stis_disp GLOBAL TYPE STIS_DISP_TYPE END_INSTANCE