|
AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
|
EDI_PSA |
 |
|
Message ID: 21
Entry time: Wed Jun 23 08:23:07 2021
|
Author: |
CB |
Subject: |
R14 analysis 2 |
|
|
Given very poor fit using line + power law + line, changes were made to the fitting algorithm.
- Starting paramters optimised for new typical wave shape
- Reverted to 3 lines, since signals are faster
- Subtracted wave minimum from all wave points to have a more realistic chi2 estimate
- Discarded all waves where 2nd half of signal > 1st half of signal. Should correspond to pick-up / noise
Fit: 3 lines
Free parameters: 2x boundary points between lines
Algorithm: Nelder-Mead, 20 iterations.
Attach 1: Wave amplitudes
Attach 2: Rise times
No major differences vs. power law method, but note candidate electron peak in rise time spectrum is now sharper.
Attach 3-9: Waveforms with H~90 and increasing rise times.
Note fit shown are via Solver's GRG, not NM.
Fits in waves 1-4 give same result for GRG and NM.
Fit in wave 5: NM-> H72 t102 vs. GRG-> H80 t25
Fit in wave 6: NM-> H96 t128 vs. GRG-> H90 t23
GRG risetimes are more realistic. This appears to be due to very short baseline pre-rise.
Will increase in next run.
Fit in wave 7 is rare pile-up event. Code cannot yet cope. Bad fit. |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|