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Suggestions from JL following testing of #227:
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On failed fits, return
NaNas fit parameters- Requires some work to 'chase through' various consumers who will be upset by NaNs, e.g.
lmfitat outer level will neednan_policy="omit"
- Requires some work to 'chase through' various consumers who will be upset by NaNs, e.g.
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Want to expose a "figure of merit" which is
(asymmetry)^2 * (count rate)fromMuonAsymmetryReducer- Should be relatively easy to expose this from
MuonAsymmetryReducer - If the asymmetry fit fails on a low stats run, the asymmetry shouldn't exceed 1 anyway so a good substitute is just to put Figure of Merit=rate in this case. Assuming other scan points have a large flux and fit successfully, it'll be close to the baseline for the outer peak fit.
- For the two-oscillation function there will be figure_of_merit_0 and figure_of_merit_1 derived from A_0 and A_1 respectively. I'll want to choose to plot/optimise one of these.
- Should be relatively easy to expose this from
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Expose
r_squaredfromMuonAsymmetryReducer. -
Give more decimal places on the soft signals that hold fitting results
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Once Argus: configuration based on double/single pulse mode IBEX#8809 is done, read
$t_0$ and$t_{good}$ PVs and use these to set the start of the data rebinning range (this is an adjustment in the inst scripts side, not inibex_bluesky_core).- Adjust all DAE time coordinates by subtracting
$t_0$ , then set rebinning to start at$t_{good}$
- Adjust all DAE time coordinates by subtracting
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