Re #11868 Minor updates

mantidproject · Oct 2, 2015 · 71769ec · 71769ec
1 parent 0898098
commit 71769ec
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Showing 3 changed files with 4 additions and 4 deletions.
diff --git a/Code/Mantid/Framework/Algorithms/inc/MantidAlgorithms/CalMuonDetectorPhases.h b/Code/Mantid/Framework/Algorithms/inc/MantidAlgorithms/CalMuonDetectorPhases.h
@@ -6,7 +6,7 @@
 namespace Mantid {
 namespace Algorithms {
 
-/** CalMuonDetectorPhases : Calculate asymmetry and phase for each spectra in a workspace
+/** CalMuonDetectorPhases : Calculates asymmetry and phase for each spectra in a workspace
 
   Copyright &copy; 2015 ISIS Rutherford Appleton Laboratory, NScD Oak Ridge
   National Laboratory & European Spallation Source

diff --git a/Code/Mantid/Framework/Algorithms/src/CalMuonDetectorPhases.cpp b/Code/Mantid/Framework/Algorithms/src/CalMuonDetectorPhases.cpp
@@ -25,11 +25,11 @@ void CalMuonDetectorPhases::init() {
       "Name of the reference input workspace");
 
   declareProperty("FirstGoodData", EMPTY_DBL(),
-                  "The first good data point in units of micro-seconds",
+                  "First good data point in units of micro-seconds",
                   Direction::Input);
 
   declareProperty("LastGoodData", EMPTY_DBL(),
-                  "The last good data point in units of micro-seconds",
+                  "Last good data point in units of micro-seconds",
                   Direction::Input);
 
   declareProperty("Frequency", EMPTY_DBL(), "Starting hint for the frequency",

diff --git a/Code/Mantid/docs/source/algorithms/CalMuonDetectorPhases-v1.rst b/Code/Mantid/docs/source/algorithms/CalMuonDetectorPhases-v1.rst
@@ -21,7 +21,7 @@ spectrum index), the asymmetry and the phase. This table is intended to be used
 *PhaseTable* to :ref:`PhaseQuad <algm-PhaseQuad>`. In addition, the fitting results are returned
 in a workspace group, where each of the items stores the original data (after removing the
 exponential decay), the data simulated with the fitting function and the difference between data
-and fit as spectrum 0, 1 and 2 respectively.
+and fit as spectra 0, 1 and 2 respectively.
 
 There are three optional input properties: *FirstGoodData* and *LastGoodData* define the fitting range.
 When left blank, *FirstGoodData* is set to the value stored in the input workspace and *LastGoodData*