 
 
 
 
 
    
![$[\,x,y\,]$](img20.gif) coordinates, and a
         linear model relating them (as produced by sla_FITXY), compute
         the array of predicted coordinates and the RMS residuals.
 coordinates, and a
         linear model relating them (as produced by sla_FITXY), compute
         the array of predicted coordinates and the RMS residuals.
| NP | I | number of samples | 
|---|---|---|
| XYE | D(2,NP) | expected ![$[\,x,y\,]$](img20.gif) for each sample | 
| XYM | D(2,NP) | measured ![$[\,x,y\,]$](img20.gif) for each sample | 
| COEFFS | D(6) | coefficients of model (see below) | 
| XYP | D(2,NP) | predicted ![$[\,x,y\,]$](img20.gif) for each sample | 
|---|---|---|
| XRMS | D | RMS in X | 
| YRMS | D | RMS in Y | 
| RRMS | D | total RMS (vector sum of XRMS and YRMS) | 
![$[x_{m},y_{m}\,]$](img113.gif) into predicted coordinates
 into predicted coordinates
        ![$[x_{p},y_{p}\,]$](img144.gif) as follows:
 as follows:
        xp = a + bxm + cym
yp = d + exm + fym
 
 
 
 
 
    
SLALIB --- Positional Astronomy Library