[ ] Study why we need additive constant (+ c) in fit of 482 keV peak.
[ ] Is this constant caused by events from 976 keV peak which are in tail of Landau distribution? How do such event look like?
[ ] In brief first simulation we have seen something like gamma peak. Is this maybe caused by some gammas?
[ ] Which individual OM resolutions we need to plug into Falaise so with all the detector effects we can mimic the real data
spectra?
[ ] Can we exploit data from reference OMs? For example use some alpha source? Maybe study the optical effects?
[ ] IMPORTANT: Can we finally accept / reject a hypothesis that the worsening of the OM resolutions is caused by aging of the OMs?
[ ] We need to study the resolutions - how they develop over the time (1 year or so)
[ ] We need to search for articles which discuss the againg effect of polystyrene - maybe there is known curve (resolution vs. time). Then we need to compare our findings with these curves.
[ ] Try to work with "special cuts", for example only take 10 cm x 10 cm (or 5 cm x 5 cm) in center of each OM. In this region the correction factor of optical corrections is around ~1 (no correction) so we could study the energy loss corrections with data directly.
[ ] Similar thing could be achieved by taking into account only electrons which travelled similar distance (e.g. 550-600 mm)
[ ] Think about some other possible justifications of the corrections with real data.
[ ] Implement better charge integration using Gill´s and Khrystyna´s findings.
[ ] There is a possibility that we could profit from 3rd peak for calibration (around 1600 keV). It is weaker but maybe we could find a method how to fit it (maybe maximum likelihood method)?
[ ] Near third peak there should be some structure caused by gammas. If I remember right it should be Compton edge of the gammas from Bi-207 (discuss with Manu, he discussed this with us). Maybe we need to describe this properly before we try to work with the 3rd peak?
[ ] The composition of the gas will be precisely measured. The composition enters into the energy loss correction (Bethe-Bloch). Would it make a difference if we implement these small gas composition changes?
[ ] To discuss with Francois: We need to add estimation of sigma_a, sigma_b and sigma_ab of the calibration parameters of a and b (and maybe also fit quality flag - good, bad, questionable) into output. Discuss it with Francois
[ ] We need also to propagate sigma_a, sigma_b and sigma_ab into sigma_E - final uncertainty of the energy.
[ ] Finally resolve the question of the Bi-207 positions. There are very nice works by Vladyslav Yankovskyi, Ivan Kovalenko and Sam Pratt which need to be merged together. This task has an article potential.
[ ] Suggestion by Francois: Rename "calibration tools" to more precise name, something like "calocalibration tools". There will be more types of calibrations and it could be confusing.
Some quick scribbles - future challenges (in Czech) poznamky.odt