Eventdisplay: an Analysis and Reconstruction Package for VERITAS
Authors/Creators
-
Maier, Gernot1
- Holder, Jamie2
- McCann, A.
- Behera, B.
- Duke, C.
- Giuri, C.
- Skole, C.
- Tak, D.
- Aliu, E.
- Pueschel, E.
- Pizlo, F.
- Decerpri, G.
- Finneagan, G.
- Foote, G.
- Hughes, G.
- Fleischhack, H.
- Krawczynski, H.
- Prokoph, H.
- Grube, J.
- Tyler, J.
- Berger, K.
- Pfrang, K.
- Gerard, L.
- Beilicke, M.
- Kherlakian, M.
- Krause, M.
- McCutcheon, M.
- Nievas-Rosillo, M.
- Schroedter, M.
- Shayduk, M.
- Hakasson, N.
- Kelley-Hoskins, N.
- Gueta, O.
- Ivo, P.
- Guenette, R.
- Patel, S.
- Prado, R.
- Welsing, R.
- Griffin, S.
- Griffiths, S.
- O'Brian, S.
- Vincent, S.
- Vorobiov, S.
- Hassan, T.
- Khassen, Y.
- 1. DESY
- 2. Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA
Description
Eventdisplay is a reconstruction and analysis pipeline for data of the VERITAS Imaging Atmospheric Cherenkov Telescopes (IACT).
v492.0-rc4 is the 4th candidate for v492. Do not use for science analysis
New Features
Improve DispBDT reconstruction by adding
loss^2andloss*distas training variables. This improves sensitivity to truncated images. (#318)Feature: Machine learning interface for direction reconstruction
- Adds an interface to run machine learning models (e.g., scikit-learn).
- Provides an example using XGBoost regression trees to estimate directions in camera coordinates.
- Introduces a Python environment and a scripts directory to support training and inference.
The new XGBoost-based training and reconstruction methods estimate the gamma‑ray arrival direction in camera coordinates. They support
DispBDTand intersection methods, combining image parameters to computeXoff/Yoff.Compared to previous approaches that averaged over all
DispBDTdirections, this implementation better handles edge cases (e.g., truncated images).(#322)
Add print out average run zenith angle to
printRunParameteroption-runinfo. (#334)Improve TMVA interpolation from average zenith to average airmass. (#336)
Allow to choose energy and direction reconstruction methods:
Stereo reconstruction --------------------- Method ids: 0 (DispBDT), 1 (LT Tables), 2 (XGB stereo) * ENERGYRECONSTRUCTIONMETHOD 0 Method ids: 0 (DispBDT), 1 (Intersection Method), 2 (XGB stereo) * DIRECTIONRECONSTRUCTIONMETHOD 0Consistently use
CDatamethods to get variables.(#339)
Improve mscw plotting macro for consistent comparison of different analysis sets. (#340)
Introduction of average zenith angle calculation per run in VTMVAEvaluator (fAverageZenithPerRun, calculate_average_zenith_angle()). (#281)
Introduced new functionality for reconstructing events using any three telescopes out of four (primarily for Monte Carlo data and effective area calculations). Added new class:
VMeanScaledVariablesfor mean scaled variable calculations. Updated VDispAnalyzer and VSimpleStereoReconstructor to support new reconstruction modes and calculation methods. Updated VInstrumentResponseFunctionRunParameter and related code to include new parameters for 3-telescope reconstruction. (#289)Add new command line parameter
--minpedestaleventsto set the minimum number of required pedestal events (default: 50). (#298)
Maintenance
Improve efficiency of IRF calculation (lower storage footprint; introduce possibility to re-calculate all stereo parameters (MSCW, MSCL, emission height, direction, core, energy) on the
mscw_energylevel for 3-telescope events from 4-telescope MC simulations. This is for MC events only and used to simplify and accelerate the analysis required for the generation of effective areas.) (#293)- reduced storage impact of
mscw_energybranch (mostly due to change of doubles to floats; removal of unused variables); reduction is on storage requirements is ~25%. - efficiency improvement in running
mscw_energy-> 20% faster - fine-tuning of docker build scripts to improve build efficiency
- add code to redo stereo reconstruction to
CData.cpp. Functions are namedreconstruct_3tel_images* - generalized calculation of MSCW, MSCL, MWR, MWL variables in new classes
VMeanScaledVariables - allow to recalculate
dispBDTDirectionanddispBDTEnergyinVDispAnalyzerfrom values per image - several important improvements and bug fixes in stereo reconstruction code in
VTableLookupDataHandler:Chi2from direction reconstruction not correctly filled fromshowerparstrees- bug fix in setting of
NImagesand selected telescopes for 3-telescope runs (functionfill_selected_images_before_redo_stereo_reconstruction)
- clarified that
Erecis fromdispBDTEnergywhileErecSis from simple lookup table reconstruction. Change default values forEnergyReconstructionMethodtoErec(method ID0) foranasumandeffective areacode. - introduced consistent naming of tree reader support classes. Moved them from
.Cto.cpp. Removed obsolete code in these files. - removed
VersionfromCDataclass initialize (as it is read from tree doc string). - removal of
CEffFit.hclasses (not used anywhere) - bug fix in SizeSecondMax calculation for 3-tel reconstruction using in
mscw_energytherec_idoption (no image selection was applied) - maintenance and cleanup of obsolete files (see PR #294)
(#303)
- reduced storage impact of
- minor updates to run with root 6.38.
- switch default ROOT docker image to ubuntu
(#323)
Change location of ROOT macros from ./macros/VTS to ./macros. (#330)
Removed deprecated smoothing and interpolation functionality for MVA cut values. Cleaned up unused parameters and obsolete code related to box smoothing and TMVA optimization. (#336)
Update URL for SOFA download. (#317)
Update SOFA to version 2023-10-11. (#284)
Changes in tree structure and variable types to reduce size of output trees (mostly due to change of doubles to floats; removal of unused variables); reduction is on storage requirements is ~25%. (#288)
Replaced many ROOT auto-generated header/source files (e.g., CData.h, CEffArea.h, CRunSummary.h, Cshowerpars.h, Ctpars.h, Ctelconfig.h) with hand-edited or cleaner C++ code, improving maintainability and readability. Moved implementation code from
.Cfiles to.cppfiles, and deleted the old.Cfiles. Adjusted several functions and constructors to reflect changes in how data and reconstruction methods are handled (e.g., CData and related classes now use cleaner, more explicit constructors). Functions that previously accepted "version" or "short" flags via integers now use explicit booleans for clarity. Removed the CEffFit class and related files. Pruned unused variables and methods, including some internal variables in VTMVAEvaluator, VTableLookupDataHandler, and others. Removed outdated warnings, TODO comments, and deprecated features. (#289)Introduce towncrier for changelogs. (#300)
Fix github action worklows to compile Eventdisplay. Add cpp11 workflow. (#307)
Performance improvements for mscw energy stage. (#312)
Bugfixes
- Fix segmentation fault when exiting on error due to an empty tree in anasum. (#286)
- Limit number of errors printed when reading faulty VBF files to avoid TB large log files. (#298)
- Add cut to wobble offset 0.5 for calculation of MC-derived gamma-ray rates used for BDT cut optimization. (#314)
Documentation
Notes
Files
VERITAS-Observatory/EventDisplay_v4-v492.0-rc4.zip
Files
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Additional details
Related works
- Is supplement to
- Software: https://github.com/VERITAS-Observatory/EventDisplay_v4/tree/v492.0-rc4 (URL)
Software
- Repository URL
- https://github.com/VERITAS-Observatory/EventDisplay_v4