Index: trunk/doc/pslib/psLibSDRS.tex
===================================================================
--- trunk/doc/pslib/psLibSDRS.tex	(revision 3163)
+++ trunk/doc/pslib/psLibSDRS.tex	(revision 3174)
@@ -1,3 +1,3 @@
-%%% $Id: psLibSDRS.tex,v 1.177 2005-02-08 20:04:56 price Exp $
+%%% $Id: psLibSDRS.tex,v 1.178 2005-02-09 22:00:38 price Exp $
 \documentclass[panstarrs,spec]{panstarrs}
 
@@ -2716,13 +2716,15 @@
     PS_INTERPOLATE_FLAT, 
     PS_INTERPOLATE_BILINEAR, 
-    PS_INTERPOLATE_BICUBIC, 
-    PS_INTERPOLATE_SINC,
+    PS_INTERPOLATE_LANCZOS2,
+    PS_INTERPOLATE_LANCZOS3,
+    PS_INTERPOLATE_LANCZOS4,
     PS_INTERPOLATE_BILINEAR_VARIANCE,
-    PS_INTERPOLATE_BICUBIC_VARIANCE,
-    PS_INTERPOLATE_SINC_VARIANCE
+    PS_INTERPOLATE_LANCZOS2_VARIANCE,
+    PS_INTERPOLATE_LANCZOS3_VARIANCE,
+    PS_INTERPOLATE_LANCZOS4_VARIANCE
 } psImageInterpolateMode mode;
 \end{verbatim}
 
-The first four are fairly straightforward.  The last three, however,
+The first five are fairly straightforward.  The last four, however,
 require some explanation.  When attempting to account for noise in a
 CCD image, it is customary to carry an additional image containing the