001     600611
005     20231221211936.0
024 7 _ |a ATLAS:2023mnn
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024 7 _ |a inspire:2636611
|2 inspire
024 7 _ |a 10.3204/PUBDB-2023-08035
|2 datacite_doi
037 _ _ |a PUBDB-2023-08035
041 _ _ |a English
088 _ _ |a ATL-PHYS-PUB-2023-001
|2 Atlas
100 1 _ |a ATLAS Collaboration
|0 P:(DE-HGF)0
|b 0
|e Collaboration author
245 _ _ |a Electron Identification with a Convolutional Neural Network in the ATLAS Experiment
260 _ _ |c 2023
300 _ _ |a 33
336 7 _ |a report
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336 7 _ |a REPORT
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336 7 _ |a Report
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336 7 _ |a Output Types/Report
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336 7 _ |a Report
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|s 1703152023_12800
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336 7 _ |a TECHREPORT
|2 BibTeX
500 _ _ |a All figures including auxiliary figures are available at https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PUBNOTES/ATL-PHYS-PUB-2023-001. The authors list may be incomplete!
520 _ _ |a The identification of electrons plays an important role for a large fraction of the physics analyses performed at the ATLAS experiment. An improved electron identification algorithm is presented that is based on convolutional neural networks (CNN), a type of machine learning architecture specialized in image recognition. It takes as input the images of the deposited energy in the calorimeter cells around the reconstructed electron candidates for each of the electromagnetic and hadronic calorimeter layers. Additional input features include the same high-level variables that are used by the likelihood (LLH) and deep neural network (DNN) algorithms developed in ATLAS, as well as the information of up to five inner detector tracks that are matched to an electron candidate during its reconstruction. The output of the network corresponds to the probability that a reconstructed electron belongs to six classes of signals and backgrounds. A significant improvement in identification performance is observed when the CNN algorithm is used in the simulation. For example, for a working point that corresponds to the same signal efficiency as the LLH 'Loose' working point, the CNN improves the rejection against charged hadrons faking signal electrons, the dominant electron background at the LHC, by factors of 5 to 8 (depending on the electron kinematics) with respect to the LLH. For the most difficult background constituted of electrons originating from heavy flavour hadron decays, the background rejection of the CNN is improved by factors varying between about 2 to 3.5 with respect to the LLH.
536 _ _ |a 611 - Fundamental Particles and Forces (POF4-611)
|0 G:(DE-HGF)POF4-611
|c POF4-611
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588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a p p: scattering
|2 INSPIRE
650 _ 7 |a p p: colliding beams
|2 INSPIRE
650 _ 7 |a electron: background
|2 INSPIRE
650 _ 7 |a electron: particle identification
|2 INSPIRE
650 _ 7 |a hadron: decay
|2 INSPIRE
650 _ 7 |a calorimeter: hadronic
|2 INSPIRE
650 _ 7 |a ATLAS
|2 INSPIRE
650 _ 7 |a neural network
|2 INSPIRE
650 _ 7 |a network
|2 INSPIRE
650 _ 7 |a calorimeter: electromagnetic
|2 INSPIRE
650 _ 7 |a tracks
|2 INSPIRE
650 _ 7 |a machine learning
|2 INSPIRE
650 _ 7 |a particle identification: efficiency
|2 INSPIRE
650 _ 7 |a CERN LHC Coll
|2 INSPIRE
650 _ 7 |a kinematics
|2 INSPIRE
650 _ 7 |a particle identification: performance
|2 INSPIRE
650 _ 7 |a heavy quark: decay
|2 INSPIRE
650 _ 7 |a statistical analysis
|2 INSPIRE
650 _ 7 |a data analysis method
|2 INSPIRE
650 _ 7 |a numerical calculations: Monte Carlo
|2 INSPIRE
650 _ 7 |a experimental results
|2 INSPIRE
650 _ 7 |a EGAMMA
|2 autogen
693 _ _ |a LHC
|e LHC: ATLAS
|1 EXP:(DE-588)4398783-7
|0 EXP:(DE-H253)LHC-Exp-ATLAS-20150101
|5 EXP:(DE-H253)LHC-Exp-ATLAS-20150101
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856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/600611/files/ATL-PHYS-PUB-2023-001.pdf
856 4 _ |y OpenAccess
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909 C O |o oai:bib-pubdb1.desy.de:600611
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
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|6 P:(DE-HGF)0
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-611
|3 G:(DE-HGF)POF4
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914 1 _ |y 2023
915 _ _ |a OpenAccess
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915 _ _ |a Creative Commons Attribution CC BY 4.0
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920 1 _ |0 I:(DE-H253)ATLAS-20120731
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980 _ _ |a report
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)ATLAS-20120731
980 1 _ |a FullTexts


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