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Record W3178740802 · doi:10.22323/1.395.0766

Identifying muon rings in VERITAS data using convolutional neural networks trained on images classified with Muon Hunters 2

2021· article· en· W3178740802 on OpenAlexfundno aff
Kevin C. Flanagan, Darryl Wright, H. J. Dickinson, P. Wilcox, Michael Laraia, S. Serjeant, M. Capasso, R. A. Ong, I. Sadeh, P. Kaaret, W. Jin, W. Benbow, R. Mukherjee, R. R. Prado, M. Lundy, S. Patel, P. Moriarty, G. Maier, A. Furniss, Ken Ragan, D. A. Williams, J. H. Buckley, L. Fortson, J. Quinn, J. Holder, C. Giuri, E. Pueschel, D. Nieto, Colin C Adams, S. O’Brien, D. Ribeiro, K. Pfrang, O. Gueta, G. M. Foote, A. J. Weinstein, S. Kumar, Tyler Williamson, D. Tak, Conor McGrath, T. K. Kleiner, M. Pohl, Paul F. Reynolds, B. Hona, D. Hanna, M. Santander, G. H. Sembroski, Sonal Ramesh Patel, M. Errando, Mary Kertzman, O. Hervet, M. Nievas Rosillo, M. J. Lang, E. Roache, T. B. Humensky, V. V. Vassiliev, Aleksey Cherman, Abe Falcone, Jodi Christiansen, A. N. Otte, A. Gent, A. Brill, James Ryan, K. A. Farrell, G. H. Gillanders, Qi Feng, A. Archer, D. Kieda

Bibliographic record

VenueProceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021) · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersOffice of ScienceNatural Sciences and Engineering Research Council of CanadaEuropean CommissionNational Energy Research Scientific Computing CenterAlfred P. Sloan FoundationU.S. Department of EnergySmithsonian InstitutionNational Science Foundation
KeywordsMuonConvolutional neural networkPhysicsArtificial intelligenceIdentification (biology)Computer scienceAlgorithmHough transformImage (mathematics)Pattern recognition (psychology)Computer visionParticle physics

Abstract

fetched live from OpenAlex

Muons from extensive air showers appear as rings in images taken with imaging atmospheric Cherenkov telescopes, such as VERITAS. These muon-ring images are used for the calibration of the VERITAS telescopes, however the calibration accuracy can be improved with a more efficient muon-identification algorithm. Convolutional neural networks (CNNs) are used in many state-of-the-art image-recognition systems and are ideal for muon image identification, once trained on a suitable dataset with labels for muon images. However, by training a CNN on a dataset labelled by existing algorithms, the performance of the CNN would be limited by the suboptimal muon-identification efficiency of the original algorithms. Muon Hunters 2 is a citizen science project that asks users to label grids of VERITAS telescope images, stating which images contain muon rings. Each image is labelled 10 times by independent volunteers, and the votes are aggregated and used to assign a `muon' or `non-muon' label to the corresponding image. An analysis was performed using an expert-labelled dataset in order to determine the optimal vote percentage cut-offs for assigning labels to each image for CNN training. This was optimised so as to identify as many muon images as possible while avoiding false positives. The performance of this model greatly improves on existing muon identification algorithms, identifying approximately 30 times the number of muon images identified by the current algorithm implemented in VEGAS (VERITAS Gamma-ray Analysis Suite), and roughly 2.5 times the number identified by the Hough transform method, along with significantly outperforming a CNN trained on VEGAS-labelled data.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.882
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.054
GPT teacher head0.282
Teacher spread0.229 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations2
Published2021
Admission routes1
Has abstractyes

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