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diff --git a/noao/twodspec/multispec/doc/fitfunc.hlp b/noao/twodspec/multispec/doc/fitfunc.hlp new file mode 100644 index 00000000..09510bb7 --- /dev/null +++ b/noao/twodspec/multispec/doc/fitfunc.hlp @@ -0,0 +1,73 @@ +.help fitfunction Jul84 noao.twodspec.multispec +.ih +NAME +fitfunction -- Fit a function to the spectra parameter values +.ih +USAGE +fitfunction image +.ih +PARAMETERS +.ls image +Image in which the parameter values are to be fitted. +.le +.ls parameter = "x0" +Parameter to be fit. The legal minimum match abbreviated parameters +are x0, s0, s1, s2. +.le +.ls lines = "*" +Sample image lines to be used in the function fit. +.le +.ls spectra = "*" +Spectra for which the parameters are to be fit. +.le +.ls function = "interpolation spline" +Fitting function to be used. The function is specified as a string +which may be minimum match abbreviated. The functions currently available +are: +.ls interpolation spline +Interpolation spline of specified order. +.le +.ls smoothing spline +Smoothing spline of specified order and number of polynomial pieces. +.le +.le +.ls spline_order = 4 +Order of the fitting spline. The order must be even. +The minimum value is 2 and maximum value is determined from the number of +sample lines in the fit. +.le +.ls spline_pieces = 1 +The number of polynomial pieces in a smoothing spline. +The minimum value is 1 and the maximum value is determined from the number of +sample lines in the fit. +.le +.ih +DESCRIPTION +A function is fit to the parameter values previously determined at the sample +lines for each spectrum. The function coefficients are stored in the +database and the fitted values replace the original values at all the sample +lines (not just the sample lines used in the fit). The type of function, +the parameter to be fitted, the sample lines used in the fit, and the +spectra to be fitted are all selected by the user. The function is +extrapolated to cover all image lines. + +The values of the function fit at arbitrary image lines may be listed +with \fBmslist\fR. +.ih +EXAMPLES +The extraction of the spectra requires that a fitting function be +determined for the spectra positions. This is done by: + + cl> fitfunction image + +To smooth the parameter "s0" in model \fIgauss5\fR with a cubic spline +and leave out a bad point at sample line 7: + +.nf + cl> fitfunction image parmeter=s0 function=smooth \ + >>> lines="1-6,8-" +.fi +.ih +SEE ALSO +mslist +.endhelp |