WFD --> Main Survey

ap_procbounds.tex

@@ -27,7 +27,7 @@ \section{Potential Processing Boundaries}\label{sec:procbounds}
 
 \subsection{Exposure Times}\label{ssec:procbounds_expt}
 
-Images which deviate significantly from the $15$ second duration for the WFD main survey 
+Images which deviate significantly from the $15$ second duration for the Main Survey 
 may encounter issues in the instrument signature removal routine, in the correction for 
 differential chromatic refraction, in the difference imaging analysis pipeline, and/or in 
 the photometric and astrometric calibrations due to a differently sampled set of standard 
@@ -75,7 +75,7 @@ \subsubsection{Long Exposures (Non-Standard Visits of $>$30 sec)}
 should be fine.
 
 However, a $2\times150$ second exposure would saturate at $r \approx 18.3$, perhaps 
-leaving too few stars overlapping with e.g., templates or WFD images, for astrometric and 
+leaving too few stars overlapping with e.g., templates or Main Survey images, for astrometric and 
 photometric calibrations.
 
 Furthermore, cosmic-ray rejection completeness might be reduced for longer exposures