r13616 - /branches/gui_testing/prompt/spectrum.py -- July 14, 2011 - 12:36

Author: bugman
Date: Thu Jul 14 12:36:07 2011
New Revision: 13616

URL: http://svn.gna.org/viewcvs/relax?rev=13616&view=rev
Log:
Fix for the spectrum.error_analysis user function documentation.


Modified:
    branches/gui_testing/prompt/spectrum.py

Modified: branches/gui_testing/prompt/spectrum.py
URL: 
http://svn.gna.org/viewcvs/relax/branches/gui_testing/prompt/spectrum.py?rev=13616&r1=13615&r2=13616&view=diff
==============================================================================
--- branches/gui_testing/prompt/spectrum.py (original)
+++ branches/gui_testing/prompt/spectrum.py Thu Jul 14 12:36:07 2011
@@ -98,14 +98,10 @@
         |          |                                        |                
                      |
         | Volumes  | All replicated + variance averaging    | One sigma per 
replicated spectra set |
         
|__________|________________________________________|______________________________________|
-
-
-        Peak heights with baseplane noise RMSD
-        ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-        When none of the spectra have been replicated, then the peak height 
errors are calculated using the RMSD of the baseplane noise, the value of 
which is set by the spectrum.baseplane_rmsd() user function.  This results in 
a different error per peak per spectrum.  The standard deviation error 
measure for the peak height, sigma_I, is set to the RMSD value.
         """
     error_analysis._doc_additional = [
+        ["Peak heights with baseplane noise RMSD", """
+        When none of the spectra have been replicated, then the peak height 
errors are calculated using the RMSD of the baseplane noise, the value of 
which is set by the spectrum.baseplane_rmsd() user function.  This results in 
a different error per peak per spectrum.  The standard deviation error 
measure for the peak height, sigma_I, is set to the RMSD value."""],
         ["Peak heights with partially replicated spectra", """
         When spectra are replicated, the variance for a single spin at a 
single replicated spectra set is calculated by the formula