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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 /math/slalib/doc/pxy.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
Diffstat (limited to 'math/slalib/doc/pxy.hlp')
-rw-r--r-- | math/slalib/doc/pxy.hlp | 56 |
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diff --git a/math/slalib/doc/pxy.hlp b/math/slalib/doc/pxy.hlp new file mode 100644 index 00000000..e2764150 --- /dev/null +++ b/math/slalib/doc/pxy.hlp @@ -0,0 +1,56 @@ +.help pxy Jun99 "Slalib Package" +.nf + + SUBROUTINE slPXY (NP,XYE,XYM,COEFFS,XYP,XRMS,YRMS,RRMS) + + - - - - + P X Y + - - - - + + Given arrays of "expected" and "measured" [X,Y] coordinates, and a + linear model relating them (as produced by slFTXY), compute + the array of "predicted" coordinates and the RMS residuals. + + Given: + NP i number of samples + XYE d(2,np) expected [X,Y] for each sample + XYM d(2,np) measured [X,Y] for each sample + COEFFS d(6) coefficients of model (see below) + + Returned: + XYP d(2,np) predicted [X,Y] for each sample + XRMS d RMS in X + YRMS d RMS in Y + RRMS d total RMS (vector sum of XRMS and YRMS) + + The model is supplied in the array COEFFS. Naming the + elements of COEFF as follows: + + COEFFS(1) = A + COEFFS(2) = B + COEFFS(3) = C + COEFFS(4) = D + COEFFS(5) = E + COEFFS(6) = F + + the model is applied thus: + + XP = A + B*XM + C*YM + YP = D + E*XM + F*YM + + The residuals are (XP-XE) and (YP-YE). + + If NP is less than or equal to zero, no coordinates are + transformed, and the RMS residuals are all zero. + + See also slFTXY, slINVF, slXYXY, slDCMF + + Called: slXYXY + + P.T.Wallace Starlink 22 May 1996 + + Copyright (C) 1996 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |