Table of Contents
SwapWidths
This algorithm is to be used on a BayesQuasi widths
workspace where the 2 widths cross over for ascending Q value. The
swap point is selected and a new workspace created which is then
suitable for use in JumpFit.Shift x-values of container by adding
option to allow
for the use of non aligned peak centres between Sample and Container.Shift x-values of container by adding
option to allow
for the use of non aligned peak centres between Sample and Container.Shift x-values of container by adding
option to allow
for the use of non aligned peak centres between Sample and Container.Use
in the parameter under Delta Function
,
this now displays the centre of the Delta Function.nxs
files.Many of the algorithms in Mantid have been given progress tracking. This means that it is now easy to see the progress of an algorithm while it is running in terms of percentage of completion and labels detailing the current process. You can also cancel these algorithms while they are running. So far the algorithms that have been given progress tracking include:
ApplyPaalmanPingsCorrections
BayesQuasi
ConvolutionFitSequential
CylinderPaalmanPingsCorrection
EVSDiffractionReduction
FlatPlatePaalmanPingsCorrection
Indirect Calibration
Indirect Energy Transfer
Indirect Resolution
PlotPeakByLogValue
ResNorm
SofQWMoments
Symmetrise
TimeSlice
TransformToIqt
ISIS Energy Transfer
ContainerSubtraction
Quasi
ConvFit
ResNorm
Absorption
CalculatePaalmanPings
TOSCABankCorrection
IndirectFlatPlateAbsorption
IndirectCylinderAbsorption
IndirectAnnulusAbsorption
EVSDiffractionReduction
MuscatSofQW
OSIRISDiffractionReduction
FlatPlatePaalmanPingsCorrection
FuryFitMultiple
ProcessIndirectFitParameters
[full instrument name] + [run number] + _ + [analyser] + [reflection] + _red
- This should all be lower case and any leading zeros should be
removed.FABADA
Multi Data Set Fitting
_red
at the end of files produced in Indirect Corrections
so they can be used in other interfaces.Resolution
input is a workspace not a file.IN16B
instrument at the ILL no longer cause Mantid
to crash when loaded and now can be used in ConvFit
.I(Q, t)
regardless of the name of Input workspaces.ConvFit
the resolution workspace is now extended to match the
number of spectra in the sample workspace when the algorithm is run
rather than when the workspaces are loaded. This makes ConvFit more
robust when the interface is being manipulated quickly.ISIS Diagnostics
, Moments
and JumpFit
when variables in
the property tree are changed.ContainerSubtraction
interface now allows for _multi_
files to be used (those which are reduced from multiple run numbers).
This was previously being incorrectly stopped due to validation.Quasi
interface now works correctly with _ResNorm
files_sqw
files in to the ConvFit
interfaceRemoval of Background (ToF)
is now also validated when Plot Time is called not only on a call to
Run.Scale Container by factor
option in the interface.Fold Multiple Frames
is no longer checked by default for IRIS and
OSIRIS in ISIS Energy Transfer.FileFinder
in LoadVesuvio
.I(Q, t) Fit
have been reordered to be
consistent with other interfaces in Indirect.FWHM
and Fitting Range
in the plot and parameter tree
in ConvFit
update automatically based on the resolution of the
instrument in the IDF and the range of the data being fitted in the
mini plot.ResNorm
can now accept files of the old or new naming convention.
It even works with a combination of the two.ProcessIndirectFitParameters
algorithm no longer produces a
__TMP
workspace when executed.Absorption Corrections
interface now has improved default values
for Scale
(1.000) and Shift
(0.000).Moments
interface now has an improved default value for Scale
(1.000).ConvFit