SEE_ALSO
NAME
xyztable  Interpolate table values, writing results to a table.
USAGE
xyztable intable1 intable2 outtable
DESCRIPTION
This routine reads tables  or text files in row/column format  and writes output tables. An input table or file contains columns of X, Y (if 2D), and Z values. This task fits a surface to Z as a polynomial function of X and Y. From a second input table, the (X, Y) independent variable values are read, the fit is evaluated for those arguments, and the (X, Y) and function values are written to the output table. The function that is to be fit may be expressed as a Chebyshev or Legendre polynomial or as an ordinary power series. The IRAF gsurfit package is used to fit and evaluate the function.
Header parameters are added to the output tables to give some information on the fit.
PARAMETERS
 intable[file name template]
 List of input tables or text files containing the data to which the surface will be fit. See also xname, yname, zname, which are used to specify the column names. The same names are used for all input tables.
 intable[file name template]
 Names of input tables or text files containing the independent variable values at which the fitted surface will be evaluated. The number of names in this list must be the same as the number given in intable1. The same column names xname (and yname if 2D) as for intable1 are used for the columns of independent variable values, but zname need not be present.
 outtable [file name template]
 List of output tables. The number of output files must be the same as the number of input files given in intable1. The output table is created as a copy of intable2, except that history records are added, and the zname column is added to contain the results of the fit.
 (xname = "c1") [string]
 Name of column for X values. This parameter is used to specify which column in the input tables (both intable1 and intable2) contains the X values. X and Y are the independent variables (or just X for 1D), and Z is the dependent variable. The default of "c1" is appropriate for the case that intable1 and intable2 are text files with X values in the first column. If intable1 lists more than one file name, the same column names are used for all files.
 (yname = "c2") [string]
 Name of column for Y values. For a onedimensional fit, you can either set yorder to zero or set yname to null or blank. Note that zname is the column name for the dependent variable regardless of whether a 1D or 2D fit is desired. See also the description for xname.
 (zname = "c3") [string]
 Name of column for Z values. This column contains the dependent variable values. For a 1D fit, values should be specified for xname and zname, and yname will not be used. See also the description for xname.
 (xorder = [integer, min=1, max=INDEF]
 Number of coefficients for function in X.
This number does not include coefficients for cross terms.
For example, if xorder and yorder are both equal to two,
the function will be

 c+ c2*X + c3*Y if cross_terms = no,
and it will be

 c+ c2*X + c3*Y + c4*X*Y if cross_terms = yes,
where c1, c2, c3, and c4 are the coefficients of the fit.
 (yorder = [integer, min=1, max=INDEF]
 Number of coefficients for function in Y. For a onedimensional fit, set yorder to zero.
 (x= INDEF) [real]
 The fit is performed over the range x1 to x2 and y1 to y2. If x1 is INDEF, the minimum X value in intable1 will be used.
 (x= INDEF) [real]
 If x2 is INDEF, the maximum X value in intable1 will be used.
 (y= INDEF) [real]
 If y1 is INDEF, the minimum Y value in intable1 will be used. In the 1D case (i.e. if yorder is zero), y1 and y2 are ignored.
 (y= INDEF) [real]
 If y2 is INDEF, the maximum Y value in intable1 will be used.
 (cross_terms = yes) [boolean]
 Include crossterms? If this is set to no, the function will consist of the sum of a polynomial in X and a polynomial in Y. If cross_terms = yes, the function can include terms such as X*Y or (X**2)*Y.
 (function = "chebyshev") [string]
 [allowed values: chebyshev  legendre  polynomial]
Function to be fit. The default value of "chebyshev" is almost always appropriate. Numerical roundoff may be severe if "polynomial" is selected, so this choice is not recommended.
 (verbose = yes) [boolean]
 Print the names of the input and output tables?
 (coefficients = no) [boolean]
 Print the coefficients? The coefficients are not printed in userfriendly format. They are the values returned by the dgssave subroutine in gsurfit. The first eight numbers describe the fit (e.g. xorder, yorder), and the remaining values are the coefficients. These may be passed to the dgsrestore subroutine in order to restore these coefficients to a gsurfit structure.
EXAMPLES
1. Suppose the input file "test.lis" contains X, Y, and Z values in the first three columns as follows:
# x y z 0. 0. 0. 1. 0. 1. 0. 1. 2.
Fit a plane, i.e. polynomial with two coefficients for each axis and no cross terms. Use the same file "test.lis" for the list of X, Y values at which to evaluate the function.
im> xyztable test.lis test.lis test \ >>> cross_terms=no function="Chebyshev" test.lis > test; rms = 0.
2. Table "1d.tab" contains the following:
x z 5 17.5 4 14.6 3 11.9 2 9.4 1 7.1 0 5.0 1 3.1 2 1.4 3 0.1 4 1.4 5 2.5 6 3.4
Do a 1D quadratic fit to these data, and evaluate the fit for the same X values, writing the output to "1dout.tab".
im> xyztable 1d.tab 1d.tab 1dout.tab \ >>> xname="x" zname="z" xorder=3 yorder=0 1d.tab, 1d.tab > 1dout.tab; rms = 1.84047E15 im> tprint 1dout.tab prp+ Table 1dout.tab Tue 14:40:19 11Jan94 HISTORY t Created Tue 14:40:14 11Jan94 XORDER i 3 RMSERR d 1.840467264049248E15 HISTORY t input table name 1d.tab HISTORY t X column name x HISTORY t Z column name z HISTORY t a Chebyshev function was fit
BUGS
REFERENCES
This task was written by Phil Hodge.