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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /pkg/images/imfit/doc/fit1d.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
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diff --git a/pkg/images/imfit/doc/fit1d.hlp b/pkg/images/imfit/doc/fit1d.hlp new file mode 100644 index 00000000..5b49f45f --- /dev/null +++ b/pkg/images/imfit/doc/fit1d.hlp @@ -0,0 +1,177 @@ +.help fit1d Jul85 images.imfit +.ih +NAME +fit1d -- fit a function to image lines +.ih +USAGE +.nf +fit1d input output type +.fi +.ih +PARAMETERS +.ls input +Images to be fit. The images may contain image sections. Only the region +covered by the section will be modified in the output image. +.le +.ls output +Output images to be created or modified. The number of output images +must match the number of input images. If an output image does not exist +it is first created and initialized to zero for fit types "fit" and +"difference" and to one for fit type "ratio". +.le +.ls type +Type of output. The choices are: +.ls fit +An image created from the function fits to the image lines. +.le +.ls difference +The difference between the image and the fit (i.e. residuals). +.le +.ls ratio +The ratio of the image and fit. +.le +.le +.ls bpm = "" +List of bad pixel masks. This may be a null string to not use a +bad pixel mask, a single mask that applies to all input images, or +a matching list. The value may also be !<keyword> to specify a keyword whose +value is the mask to use. +.le +.ls axis = 1 +Axis along which the one dimensional fitting is done. Axis 1 corresponds +to fitting the image lines and axis 2 corresponds to fitting the columns. +.le +.ls interactive = yes +If \fBinteractive\fR is set to yes, a plot of the fit is drawn and the +cursor is available for interactively examining and adjusting the fit. +.le +.ls sample = "*" +Lines or columns to be used in the fits. +.le +.ls naverage = 1 +Number of sample points to combined to create a fitting point. +A positive value specifies an average and a negative value specifies +a median. +.le +.ls function = spline3 +Function to be fit to the image lines or columns. The functions are +"legendre" (legendre polynomial), "chebyshev" (chebyshev polynomial), +"spline1" (linear spline), and "spline3" (cubic spline). The functions +may be abbreviated. +.le +.ls order = 1 +The order of the polynomials or the number of spline pieces. +.le +.ls low_reject = 0., high_reject = 0. +Rejection limits below and above the fit in units of the residual sigma. +.le +.ls niterate = 1 +Number of rejection iterations. +.le +.ls grow = 0. +When a pixel is rejected, pixels within this distance of the rejected pixel +are also rejected. +.le +.ls graphics = "stdgraph" +Graphics output device for interactive graphics. +.le +.ls cursor = "stdgcur" +Graphics cursor input. +.le +.ih +DESCRIPTION +A one dimensional function is fit to each line or column of the input images. +The function may be a legendre polynomial, chebyshev polynomial, +linear spline, or cubic spline of a given order or number of spline pieces. +The output image is of pixel type real and is formed from the fitted +function values, the difference or residuals of the fit (pixel value - +fitted value), or the ratio between the pixel values and the fitted values. + +The output image may exist in which case a section in the input image is +applied to the output image. Thus, a section on the input image causes only +that part of the output image to be changed. If the output image does not +exist it is first created with a size given by the full (without a section) +input image and initialized to zero for fit and difference output types +and one for ratio output types. + +A bad pixel mask may be specified to exclude data from the fitting. Any +non-zero value in the mask is excluded. It appears in the interactive +fitting in the same way as manually deleted points. The mask is matched to +the input image(s) as described by \fBpmmatch\fR. The default is matching +in physical coordinates. + +The points fit are determined by selecting a sample of lines or columns +specified by the parameter \fIsample\fR and taking either the average or +median of the number of points specified by the parameter \fInaverage\fR. +The type of averaging is selected by the sign of the parameter and the number +of points is selected by the absolute value of the parameter. +The sample points are specified relative to any image sections. + +If \fIlow_reject\fR and/or \fIhigh_reject\fR are greater than zero the sigma +of the residuals between the fitted points and the fitted function is computed +and those points whose residuals are less than \fI-low_reject\fR * sigma +and greater than \fIhigh_reject\fR * sigma are excluded from the fit. +Points within a distance of \fIgrow\fR pixels of a rejected pixel are also +excluded from the fit. The function is then refit without the rejected points. +This rejection procedure may be iterated a number of times given by the +parameter \fIniterate\fR. + +The fitting parameters (\fIsample, naverage, function, order, low_reject, +high_reject, niterate, grow\fR) +may be adjusted interactively if the parameter \fIinteractive\fR is yes. +Lines or columns from the image are selected to be fit with the \fBicfit\fR +package. A single column or line may be chosen or a blank-separated range +may be averaged. Note that the averaging applies only to the graphed +data used to set the fitting parameters. The actual image lines and columns +are fit individually. The interactive cursor mode commands for this package +are described in a separate help entry under "icfit". Line 1 is automatically +selected for one dimensional images and any number of lines or columns may be +selected for two dimensional images. Note that the lines or columns are +relative to the input image section; for example line 1 is the first line of +the image section and not the first line of the image. When an end-of-file or +no line(s) or column(s) are given then the last selected fitting parameters +are used on each line or column of the image. This step is repeated for +each image in the input list. +.ih +EXAMPLES +1. To create a smoothed version of an image by fitting the image lines: + + cl> fit1d image fitimage fit + +If the interactive flag is set and the image is two dimensional then a prompt +for an image line is printed: + + image: Fit line = 100 200 + +The selected lines are averaged, graphed, and the interactive options for +setting and fitting the line are used. Exiting with 'q' or return prompts for +another line if the image is two dimensional. When the fitting parameters +are suitably set then respond with end-of-file or return to fit all the lines +of the image and create the output image. + +2. To subtract a linear function fit to columns 10 to 20 and 80 to 100 from +columns 10 to 100 and to subtract another linear function fit to lines +110 to 120 and 180 to 200 from columns 110 to 200: + +.nf + cl> fit1d image1[10:100,*] output diff axis=2 sample="1:11,71:91" + cl> fit1d image1[110:200,*] output diff axis=2 sample="1:11,71:91" +.fi + +Pixels outside columns 10 to 100 and 110 to 200 are not affected. Note that the +sample points are specified relative to the image sections. The script +\fBbackground\fR is available in other packages for doing background +subtractions. + +3. To determine a small scale response image: + + cl> fit1d image1 flat ratio + +The task \fBimred.generic.flat1d\fR is available for making flat field images +by this method with the addition of an extra parameter to limit the data values +for which the ratio is computed. +.ih +SEE ALSO +imred.generic.background, imred.generic.flat1d +xtools.icfit, lineclean, imsurfit +.endhelp |