TABLE /MATH

###
TABLE /MATH

            TABLE /MATH Expression1 [... ExpressionN]

        Instead of storing the spectrum (channels) for each entry in the current
        index,  you  can use any Sic mathematical formula (e.g. involving some R
        buffer variables).

        The following functions are also predefined (see e.g. HELP FUNCTION SDTV
        for details):
            STDV(dummy)   integrated area (K.Km/s)
            TPEAK(dummy)  peak temperature (K)
            VPEAK(dummy)  velocity at peak (Km/s)
            TDV(v1,v2)    integrated area (K.Km/s) between velocities V1 and V2
            TPEAKV(v1,v2) peak temperature (K) between velocities V1 and V2
            VPEAKV(v1,v2) velocity at peak (Km/s) between velocities V1 and V2

        For  example,  to  create a table containing the integrated area of each
        spectra, you can use:
            TABLE Filename /MATH STDV(0)

        To create a table of the RMS of each spectrum measured  during  BASElin-
        ing, use:
            TABLE Filename /MATH R%HEAD%BAS%SIGFI

        And  to create a table of the area, position, and width of the line fit-
        ted with the command MINIMIZE for all the spectra, use:
            TABLE Filename /MATH R%HEAD%GAU%RESULT[1] R%HEAD%GAU%RESULT[2] -
              R%HEAD%GAU%RESULT[3]

        Once used in XY_MAP, these tables will  result  in  maps  of  integrated
        area, RMS, line width, etc.