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Trapping correction module and app - #184
sophieehaight wants to merge 10 commits into
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fhagemann
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It looks like the units of depth_val (mm) and m_Depths (cm) do not match..
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Can we also remove |
fhagemann
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Here is my feedback from just looking at the code.
I will also try to compile and run both the module and the app to provide more feedback on that as well! :)
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fhagemann
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Final code-style review, will give it a run to see that it compiles.
But then this should be good to go (tackling reading trapping parameters for multiple detectors in a follow-up PR)
| m_Name = "Trapping Correction"; // - correcting energies for charge trapping (by Sophie); | ||
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| // Set the XML tag --- has to be unique --- no spaces allowed | ||
| m_XmlTag = "TrappingCorrection"; |
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Let's be consistent with XML tag naming here (see #193)
| m_XmlTag = "TrappingCorrection"; | |
| m_XmlTag = "XmlTagTrappingCorrection"; |
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I'm actually not seeing this convention in the depth or energy calibration modules? It looks like the XML tag is just the name of the module
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This is tackled in #197 once it is merged
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Once I change the name of the xml tag, nuclearizer can no longer recognize the module. Is there somewhere else in assembly I need to update the xml tag? I was looking but I couldn't find anything
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This will affect reading in a nuclearizer config file (*.cfg). In those, you might need to update all occurences of TrappingCorrection with XmlTrappingCorrection.
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So either update the .nuclearizer.cfg in your home directory, or the respective .cfg that you load when running nuclearizer.
| cout << "\n" << m_XmlTag << " --- " << titleLabel << " ---" << endl; | ||
| cout << " Centroid (Mu) : " << mu << " keV" << endl; | ||
| cout << " Fitted Gaussian FWHM : " << fwhm << " keV" << endl; | ||
| cout << " Direct Histogram FWHM: " << directFWHM << " keV" << endl; |
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I use this output to evaluate how well the trapping correction is working. If I change the verbosity to info, the comand line becomes overloaded (I believe w info from the depth cal) and nuclearizer crashes. I agree this info doesn't need to be repeated so I can change the verbosity for the following comments but I do need it read out somewhere.
I think we probably need to clean up the outputs for the info verbosity right now because right now it's outputting so much info that I can't receive the info I'm trying to get from the trapping correction.
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@zoglauer maybe we can introduce the chatty verbosity from megalib also to nuclearizer, and move some of the info messages to chatty?
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yeah that could be a good idea!
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This would be good from my side. Just gathering here the open TODOs (for follow-up PRs):
- Allow for a charge trapping parameters file for multiple detectors, at not just one
- Think about flushing output to
c_Infowithout overloading the output - Maybe find an alternative to
Interpolateto avoid code duplication (maybe from an existing package or another module --> the depth calibration also used some sort of interpolation algorithm to interpolate the CTD-to-depth spline).
fhagemann
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Some code-style and some more major comments.
One general comment:
you are using a lot of snake-case when assigning variable names, we might want to use camel-case consistently here (e.g. SimCCESortedHoles instead of sim_cce_sorted_h)
| // Evaluate full function FWHM over the fit window (645 keV to 675 keV) | ||
| double xMinFit = 645.0; | ||
| double xMaxFit = 675.0; |
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This seems to be tailored to Cs137. Is this what we want? What if we pass data from other isotopes through MModuleTrappingCorrection?
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I set it up in commits 8f30f9b, b95dc1e, and f191838 (took a couple tries to get my axes to update correctly here). I let the user define the energy of the photopeak they are tryting to fit on the nuclearizer expo. The trapping correction module then takes that input and uses it to define the Mu and min and max energies for the photopeak fits measuring resolutions pre and post trapping correction. I kept the default energy for Cs-137 as a benchmark.
| @@ -605,7 +600,7 @@ TF1* MModuleTrappingCorrection::GeneratePhotopeakFunction() | |||
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| // Provide initial sensible guesses for a Cs137 photopeak | |||
| PhotopeakFunction->SetParameter("Amplitude", 1000); | |||
| PhotopeakFunction->SetParameter("x0 (Mu)", muInitial); | |||
| PhotopeakFunction->SetParameter("x0 (Mu)", 661.7); | |||
| PhotopeakFunction->SetParameter("Sigma Gauss", 2.0); | |||
| PhotopeakFunction->SetParameter("BoverA", 0.05); | |||
| PhotopeakFunction->SetParameter("Gamma", 0.5); | |||
| @@ -615,7 +610,7 @@ TF1* MModuleTrappingCorrection::GeneratePhotopeakFunction() | |||
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| // Set boundary limits to stabilize convergence | |||
| PhotopeakFunction->SetParLimits(0, 1, 1e8); | |||
| PhotopeakFunction->SetParLimits(1, fitMin, fitMax); // Keeps peak centered around Mu | |||
| PhotopeakFunction->SetParLimits(1, 645, 675); // Keeps peak centered around 662 keV | |||
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Your last pushes reverted back to the fixed window around 662keV.
Is this intended?
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my mistake! I was testing the fit with and without the dynamic fitting window. This is fixed in 6321870
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I've lost track. Is this ready for a final review? |
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If the last changes conclude this PR, we might want to clean up the commit history and reduce the ~100 commits to a few major commits (adding the module, adding the GUI options, adding example files, ...), as this PR changes only a handful of files and adds a handful to the Happy to help here! |
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fhagemann
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Comments on the Cs137 trapping app only:
| double g_MinCTD = -250; | ||
| double g_MaxCTD = 250; |
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Is there ever a scenario where this range might no be enough?
For payload calibrations, we will have slightly higher temperatures than in unit-level calibrations, resulting in lower charge carrier mobilities, that might push the CTD out of the [-250,250] range (maybe?)
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Perhaps on the AC side we would see CTD >250. On the DC side most detectors can only get the required number of counts in a Cs-137 photopeak at CTD = -200 so it is not an issue. Right now the keeping CTD < +250 allows me to place an upper limit on the CTD value when map depth values to CTD values for the CCE parameterization.
Getting data at CTD >250 is something I want to take a look at in the future but right now we get plenty of counts on that side of the detector. I'll add a TO DO comment for this but for the purposes of this pull request I think we can leave these limits as is.
| MString m_TACCalFile; | ||
| MString m_TACCalibrationFile; |
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What is the difference between TACCalFile and TACCalibrationFile?
Edit: looks like m_TACCalibrationFile is used for what used to be the TAC cut file, so this can go:
| MString m_TACCalFile; | |
| MString m_TACCalibrationFile; | |
| MString m_TACCalFile; |
| Usage<<" --emax: maximum Event energy (default 700 kev)"<<endl; | ||
| Usage<<" -e: energy calibration file (.ecal)"<<endl; | ||
| Usage<<" --tcal: TAC calibration file"<<endl; | ||
| Usage<<" --tcut: TAC cut file"<<endl; |
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I don't think that we need TAC cut files anymore with the latest changes in #194
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| // First check if each option has sufficient arguments: | ||
| // Single argument | ||
| if ((Option == "-i") || (Option == "-o") || (Option == "--emin") || (Option == "--emax") || (Option == "--tcal") || (Option == "--tcut") || (Option == "-m") || (Option == "--ctdmin") || (Option == "--ctdmax")) { |
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| if ((Option == "-i") || (Option == "-o") || (Option == "--emin") || (Option == "--emax") || (Option == "--tcal") || (Option == "--tcut") || (Option == "-m") || (Option == "--ctdmin") || (Option == "--ctdmax")) { | |
| if ((Option == "-i") || (Option == "-o") || (Option == "--emin") || (Option == "--emax") || (Option == "--tcal") || (Option == "-m") || (Option == "--ctdmin") || (Option == "--ctdmax")) { |
| if (Option == "--tcut") { | ||
| m_TACCalibrationFile = argv[++i]; | ||
| cout<<"Accepting file name: "<<m_TACCalibrationFile<<endl; | ||
| } | ||
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| if (Option == "--tcut") { | |
| m_TACCalibrationFile = argv[++i]; | |
| cout<<"Accepting file name: "<<m_TACCalibrationFile<<endl; | |
| } |
| cout << "Creating energy calibrator" << endl; | ||
| EnergyCalibrator = new MModuleEnergyCalibration(); | ||
| EnergyCalibrator->SetFileName(m_EcalFile); | ||
| S->SetModule(EnergyCalibrator, MNumber); | ||
| ++MNumber; |
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Do you require any sort of energy (slow) thresholds to be set here?
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Yes, I set a slow threshold at 30 keV. I had originally had this set locally in the ecal module but I will add it to the app.
| MStripHit* TrappingCorrectionCs137::GetDominantStrip(vector<MStripHit*>& Strips, double& EnergyFraction) | ||
| { | ||
| double MaxEnergy = -numeric_limits<double>::max(); | ||
| double TotalEnergy = 0.0; | ||
| MStripHit* MaxStrip = nullptr; | ||
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| // Iterate through strip hits and get the strip with highest energy | ||
| for (const auto SH : Strips) { | ||
| double Energy = SH->GetEnergy(); | ||
| TotalEnergy += Energy; | ||
| if (Energy > MaxEnergy) { | ||
| MaxStrip = SH; | ||
| MaxEnergy = Energy; | ||
| } | ||
| } | ||
| if (TotalEnergy == 0) { | ||
| EnergyFraction = 0; | ||
| } else { | ||
| EnergyFraction = MaxEnergy/TotalEnergy; | ||
| } | ||
| return MaxStrip; | ||
| } |
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This seems like it's an identical copy of MModuleDepthCalibration::GetDominantStrip, which is a public function, so you can probably use that here instead:
- Load
#include "MModuleDepthCalibration.h" - In
Analyze, define (with all other modules)MModuleDepthCalibration* Depth = new MModuleDepthCalibration, maybe with a comment that you're not running the module, just using its functions here. - Call
Depth->GetDominantStripwhere you just haveGetDominantStrip. - Remove this function here (plus its declaration in the class).
| signal(SIGINT, CatchSignal); | ||
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| // Initialize global MEGALIB variables, especially mgui, etc. | ||
| MGlobal::Initialize("Standalone", "a standalone example program"); |
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You could be more explicit here:
| MGlobal::Initialize("Standalone", "a standalone example program"); | |
| MGlobal::Initialize("TrappingCorrectionCs137", "A standalone program to determine CTD-dependent shifts of the Cs137 peak"); |
or something like that.
fhagemann
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And some general comment on the file format (header lines starting with # or not)
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| # A_HV,A_LV,B,C | |||
| 1.0009264205609762,1.00084829470918,1.288689028046797,0.3010529785474152 | |||
| # z_depth_cm,e_CCE_HV,h_CCE_HV,e_CCE_LV,h_CCE_LV | |||
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The example files here in resource/dee and in resource/calibration are a bit inconsistent when it comes to the line defining the headers z_depth (in terms of if they should start with a # or not).
I would prefer the line to always start with a #,
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I guess this file won't work because it doesn't start with ### 0 ?
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| ### 0 | |||
| 1.0008508757266585,1.0009808031358887,1.1384578503113774,0.3538332986513531 | |||
| z_depth_cm,e_CCE_HV,h_CCE_HV,e_CCE_LV,h_CCE_LV | |||
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Here and elsewhere in resource/calibration:
| z_depth_cm,e_CCE_HV,h_CCE_HV,e_CCE_LV,h_CCE_LV | |
| # z_depth_cm,e_CCE_HV,h_CCE_HV,e_CCE_LV,h_CCE_LV |
| // Skip text column headers | ||
| if (Line.BeginsWith("z_depth")) continue; |
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This could go if we force the header lines to start with #.
Or is there any reason you chose not to?
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created app to return depth dep centroid energy shift for Cs-137 data
Created charge trapping correction module with GUI options
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The missing MGUIOptionsTrappingCorrection files were added
ckierans
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This is a ton of good work, @sophieehaight !
I've done a review of just the Nuclearizer App for now, I'll try to get through the rest tomorrow.
It looks like there are a few things that you need to update to account for recent merged PRs as identified in Felix's comments and the ones below.
I've run the app, but it took a bit of editing to make things work. Do you usually run with or without the "-n" option for nearest neighbors?
At first I was getting strange results, namely a double peaked spectra.
The double peak goes away when I don't use the -n option, but the resulting photopeak is much broader and shifted higher in energy, similar to what Julian has shown when we add NN strip hits without an appropriate energy threshold in at higher energy).
I then tried with a SlowThresholdCut of 15 keV and the double peak structure goes away. How were you doing this without the SlowThresholdCut?
| //////////////////////////////////////////////////////////////////////////////// | ||
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| //! The user interface for the universal energy calibration |
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//! The user interface for the trapping correction
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yes, I am using the -n option to exclude nearest neighbors and I am applying a slowthreshold cut at 30 keV. I had originally just updated my Ecal module locally to apply the slow threshold cut but I am going to code the cut into the trapping app itself when I define the instance of the energy calibration. Will push that version soon!
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Do we actually want to have the option to run this without excluding NN strip hits? Maybe we should force that in the analysis?
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It still says "The user interface for the universal energy calibration" here. Update it to "trapping correction"
| /* | ||
| * MGUIOptionsTrappingCorrection.h | ||
| * | ||
| * Copyright (C) by Andreas Zoglauer. |
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| if (m_Interrupt == true) return false; | ||
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| // [CTD, HV Energy, LV Energy] for full detector values |
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Missing the DetID map in the comment:
// [CTD][DetID][HV Energy, LV Energy] for full detector values
| MString InputFile = FileNames[0]; | ||
| cout << " input file stored as: " << InputFile << endl; | ||
| vector<MString> HDFNames; | ||
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Add comment:
"// Enable sum of weights squared for TH1 by default"
| EventFilter->SetMinimumHits(0); | ||
| EventFilter->SetMaximumHits(100); | ||
| EventFilter->SetMinimumTotalEnergy(m_MinEnergy); | ||
| EventFilter->SetMaximumTotalEnergy(m_MaxEnergy * 2); |
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Why *2 for the MaxEnergy? Maybe add a comment in the code to explain this logic?
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This is limiting the event level energy (summed over hv and lv) so it need to be twice our desired max for a hit energy. Let me add that comment!
| MStripHit* HVSH = GetDominantStrip(HVStrips, HVEnergyFraction); | ||
| MStripHit* LVSH = GetDominantStrip(LVStrips, LVEnergyFraction); | ||
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| if ((LVSH->HasCalibratedTiming() == true) && (HVSH->HasCalibratedTiming() == true) && (LVSH != nullptr) && (HVSH != nullptr)) { |
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HasCalibratedTiming is depreciated after PR #171. See #171 (comment)
I had to change this line to get any data in the histograms.
| if ((LVSH->HasCalibratedTiming() == true) && (HVSH->HasCalibratedTiming() == true) && (LVSH != nullptr) && (HVSH != nullptr)) { | |
| if ((LVSH->HasFastTiming() == true) && (HVSH->HasFastTiming() == true) && (LVSH != nullptr) && (HVSH != nullptr)) { |
| } | ||
| } | ||
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| // Place this outside/before your CTD bin and Detector loops! |
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Change this comment to be descriptive of the following functionality. I.e. "// Define an output file to save the photopeak fitting results"
| } | ||
| } | ||
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| // Place this at the absolute end of your Analyze() function |
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"// Close output fit parameter file"
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| cout << "Creating energy calibrator" << endl; | ||
| EnergyCalibrator = new MModuleEnergyCalibration(); | ||
| EnergyCalibrator->SetFileName(m_EcalFile); |
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I needed to add the following lines to include a SlowThreshold to remove the double peak spectra I was getting
| EnergyCalibrator->SetFileName(m_EcalFile); | |
| EnergyCalibrator->SetFileName(m_EcalFile); | |
| EnergyCalibrator->SetSlowThresholdCutMode(MSlowThresholdCutModes::e_Fixed); | |
| EnergyCalibrator->SetSlowThresholdCutFixedValue(15); |
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I had been make a cut at 30 keV originally to solve this but it has the same effect at 15 keV so I can set the value there : )
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I believe you still need the line
EnergyCalibrator->SetSlowThresholdCutMode(MSlowThresholdCutModes::e_Fixed);?
| if ((InputFile.GetSubString(InputFile.Length() - 4)) == "hdf5") { | ||
| HDFNames.push_back(InputFile); | ||
| cout << "hdf names loaded correctly" << endl; | ||
| } else if ((InputFile.GetSubString(InputFile.Length() - 3)) == "txt") { |
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Are you ever expecting to combing data from different runs?
If this .txt file option is only meant to load multiple files from the same run, then the MModuleLoaderMeasurementsHDF already has the SetLoadContinuationFiles option that should handle this.
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Having the txt file as an input for loading the HDF files allows me to control how many files I'm using to characterize the data. I have more data (30+ files of Cs data) for some of the detectors so I've been using only 20 data files via the txt file option to characterize individual detectors.
cleaned up outputs and added a check for fast timing
Created a trapping correction expo
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ckierans
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Continuing on with comments on the Nuclearizer Module for the forward pipeline...
Some larger comments, and plenty of more below:
I'm a bit confused at where the .csv files that are uploaded in the resource folder come from. When running the TrappingCorrectionCs137 app, I get a parameters file that has the Det_ID, CTD_Bin CTD_BinMidpoint_ns, HV_Centroid_keV, HV_Centroid_error_keV, LV_Centroid_keV, LV_Centroid_error_keV. But the csv file has the parameters from the z_depth_cm, e_CCE_HV, h_CCE_HV, e_CCE_LV, h_CCE_LV from a fit to the simulated CCE curves. Where does that fitting happen? That should be within the Nuclearizer app so that it generates the file that is then read into the forward pipeline.
You use the name SimCCEFile to describe the trapping correction files that you have. I know the shape is based on simulations, but you modify those simulated curves based on measurements. So I find this naming confusing. Can you change this to CCECorrectionFile or something instead? That's a lot of variables to modify, but it might be more easy to understand what those files are.
In the Nuclearizer Module Expo you have an automatic photopeak fit to report the FWHM of the uncorrected and corrected spectra. While this is a very nice confirmation that the module is doing what it's supposed to, I don't think this validation belongs in the general pipeline so I think that piece of code can be removed.
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| // Local Position: | ||
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| //! Set the local/raw position of the hit |
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| //! Set the local/raw position of the hit | |
| //! Set the position of the hit in local detector coordinates |
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| //! Set the local/raw position of the hit | ||
| void SetLocalPosition(const MVector& Position) { m_LocalPosition = Position; } | ||
| //! Return the local/raw position of the hit |
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| //! Return the local/raw position of the hit | |
| //! Retrurn the position of the hit in local detector coordinates |
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| //! Set the photopeak mu value | ||
| void SetPhotopeakMu(double mu) { m_PhotopeakMu = mu; } | ||
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Remove the line between the Set/Get functions.
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| //! Read the XML configuration | ||
| bool ReadXmlConfiguration(MXmlNode* Node); | ||
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Remove the line between the related Read/Create XML node functions
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| //! Initialize the module | ||
| virtual bool Initialize(); | ||
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Move Finalize after Initialize to keep the similar functions close together
| //! Finalize the module | |
| virtual void Finalize(); | |
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| ///////////////////////////////////////////////////////////////////////////////// | ||
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| double MModuleTrappingCorrection::GetSimBasedCorrectedEnergy(double depth_val, double uncorrected_energy, const std::vector<double>& depths, const std::vector<double>& sim_cce_sorted_e, const std::vector<double>& sim_cce_sorted_h, double paramB, double paramC) |
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This function should use upper camel case to follow the coding conventions, e.g. "sim_cce_sorted_e" -> "SimCCESortedE"
Can you modify the variables to match the convention?
| return uncorrected_energy; | ||
| } | ||
| double cce_base_e = Interpolate(depth_val, depths, sim_cce_sorted_e); | ||
| double cce_base_h = Interpolate(depth_val, depths, sim_cce_sorted_h); |
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You're calling Interpolate for each event. This might be slow, so a more efficient way to do this is to store a ROOT Interpolator object in your DetectorTrappingData struct and initialize the Interpolators in the LoadSimCCEFile function at the beginning of the analysis. Then you can then evaluate them quickly for each event and not interpolating for each and every event. But, unless we should that this module is too slow, I wouldn't worry about that. I just wanted to mention it as a potential future improvement.
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sg! The module usually runs in a matter of seconds so I don't think it's an issue right now. Happy to update in the future though if we decide it's necessary.
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| ### 0 | |||
| 1.0008508757266585,1.0009808031358887,1.1384578503113774,0.3538332986513531 | |||
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What are these numbers at the top of the file? Can you add a comment to define them?
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I was waiting to correct this until I could produce the param files with the Cs137 trapping app but it's an easy fix for me in python too so I can just upload new param files with added comments :)
| // Check depth bounds using this specific detector's CCE grid limits | ||
| double min_param_depth = std::min(detData.m_Depths.front(), detData.m_Depths.back()); | ||
| double max_param_depth = std::max(detData.m_Depths.front(), detData.m_Depths.back()); | ||
| bool is_depth_out_of_bounds = (depth_val < min_param_depth || depth_val > max_param_depth); |
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It would be preferred if you used upper camel case here:
"min_param_depth" -> "MinParamDepth", etc.
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Same as for the HV loop below
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I also updated is_depth_out_of_bounds -> IsDepthOutofBounds to match
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| double correctedLVEnergy = rawLVEnergy; | ||
| if (is_depth_out_of_bounds == false) { |
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I'm wondering about this forced bounds. The DepthCalibration should push the position of each hit into the active detector volume. If you find a hit outside of that, what should you do? I think it might be better if you do not place any constraints and assume the closest position, i.e. if the depth value is < min_param_depth, then just use min_param_depth as the z for the correction. That way you'll always analyze each event that the DepthCalibration passes on to you without making another down select on the position of the hit.
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Yes, I think this makes sense.
I originally put this check in because my old CCE were not simulating all the way to the detector edges and it was messing up the corrected energy when depths were not associated with a CCE.
Since updating the simulated CCEs and trapping param files, I haven't seen any events outside of the depth boundaries.
Still, in case it we do get out of bounds depths, I will add a corrected energy assignment for the depth.
The Cs-137 trapping at app produces an output files with the experimental line shifts in each depth bin. Then the fitting to the simulated CCE is done in python so the param generation process. In the calibrations meeting in the past we discussed putting the entire parameter generation process in nuclearizer but decided against it because the we will only use Cs-137 to characterize electron trapping for pre-flight calibrations. To characterize in-flight trapping we will need to develop another method likely using the continuum. I would argue that it's probably not necessary to put the CCE fitting process in nuclearizer since I may be the only one who produces these pre-flight parameter files characterizing electron trapping but happy to discuss more! |
Added trapping parameter files for unit level as well as dummy payload and single detector files
Record a local position in depth cal to access in trapping correction Updated comments on local position
changed depth cal functions to public for use in the trapping correction
Created MGUIOptionsTrappingCorrection src file Create MGUIOptionsTrappingCorrection.h
Updated for clarity and to align with TAC cut / TAC cal separation cleaned up the trapping app comments + functionality
Removed energy histogram fits and resolution outputs Added comments + Updates to formatting + style Added corrected energy assignment for out of bounds depths
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ckierans
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Thanks for the changes, Sophie! A few small corrections.
Where are you at with getting the CCE fits in there? I'm wondering if it makes sense to have this complete before merging, or accept it as is with the expectation that there will be modifications coming.
I'm troubleshooting the CCE fitting now. I'm hoping to have it done either today or tomorrow but that will depend on when I find the fix. I think it is okay to merge as is, since the parameter generation pipeline is working (just not fully contained to nuclearizer). And then we can merge the updated trapping app/ param generation pipeline once I have it ironed out. |
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Someone should check if all the comments in this PR ended up being resolved (and flag the ones that might not have been). Is someone looking into this, or want me to do it? |
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I'd also be interested to see the plots of the 16 fits to determine the charge trapping correction parameters 😇 |
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I just went through this pr now and it looks like all the comments have been addressed except concerning adding comments the trapping param files. I was hoping to fix this once I get the trapping app outputting accurate trapping parameter fits (I'm still having trouble with the fitting functions in ROOT). I've uploaded a presentation describing the unit level charge trapping pipeline, showing the fitted trapping parameter plots, and summarizing the improvement to resolution for each detector to the COSI drive. It can be found here. |









Contains a new module for applying depth-based charge trapping correction to individual hit energies along with modules with GUI options and GUI expos. The branch also includes an app for characterizing trapping with Cs-137 data. The trapping correction module requires a csv parameter file as input:
detector_0_trapping_parameters.csv
This file can also be found in resource/dee