GammaLearn Results & Publications
Main Results
GammaPhysNet network architecture
The GammaPhysNet architecture (Jaquemont et al 2021) has been developed specifically for the analysis of Cherenkov Telescope Array (CTA) data. It is a multi-task architecture with attention mechanism composed of a convolutional encoder and a multi-task decoder. Therefore, all the main event reconstruction tasks are performed simultaneously. This presents several advantages:
- simplificity of use: only one network to train and to use for all the tasks
- better generalization and performances: the network learns to extract the relevant information for all the tasks at the same time
- less computational time and memory consumption: only one network to train and to use for all the tasks
- less degenaracy between tasks as they are performed simultaneously and share the same encoder
Application to Monte-Carlo simulations
The efficiency of the GammaPhysNet architecture has been proven on Monte-Carlo simulations of the CTA LST-1 telescope (Jaquemont et al 2021, Vuillaume et al 2021).
Application to real data
The Crab Nebula
Application to real data has been done on CTA LST-1 data (Jacquemont et al 2021, Vuillaume et al 2021) showing improvements in sensitivity compared to the standard analysis. This was the first time that a full-event reconstruction was performed on real data with a deep learning architecture, and the first time that sensitivity improvement was achieved on real data. To achieve this result, a careful modulation of the background noise in the MC simulations was necessary to match the real data night sky background (NSB).
Reconstruction | Excess | Significance | Background counts |
---|---|---|---|
Hillas+RF | 379 γ | 12.0 σ | 308 |
Hillas+RF+Poisson noise | 376 γ | 11.9 σ | 305 |
γ-PhysNet | 395 γ | 12.5 σ | 302 |
γ-PhysNet+Poisson noise | 476 γ | 14.3 σ | 317 |
Mrk 501
An analysis of Mrk 501 data has also been performed (Vuillaume et al 2021) showing here again an increased sensitivity, but with a greater bias in the reconstructed directionß.
Reconstruction | Excess | Significance | Background counts |
---|---|---|---|
Hillas+RF | 148.7 𝛾 | 7.6 𝜎 | 238.3 |
𝛾-PhysNet DA | 192.7 𝛾 | 9.8 𝜎 | 226.3 |
Application to real data with domain adaptation
In order to be less sensitive to differences between Monte-Carlo simulations and real data (NSB, broken pixels, telescope PSF…), domain adaptation techniques have been applied. These techniques consist in including unlabeled real data in the training process in order to increase the network robustness to the differences between the training and the test data. Validation of different approaches and architecture has been shown on modified Monte-Carlo simulations (Dell’aiera et al 2023).
Peer-reviewed publications:
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Dell’aiera, M., Jacquemont, M., Vuillaume, T., and Benoit, A., Deep unsupervised domain adaptation applied to the Cherenkov Telescope Array Large-Sized Telescope, International Conference on Content-Based Multimedia Indexing (CBMI), 2023
Open-source version: arXiv e-prints, 2023. doi:10.48550/arXiv.2308.12732. -
M. Jacquemont, T. Vuillaume, A. Benoit, G. Maurin, P. Lambert and G. Lamanna, First Full-Event Reconstruction from Imaging Atmospheric Cherenkov Telescope Real Data with Deep Learning, 2021 International Conference on Content-Based Multimedia Indexing (CBMI), 2021, pp. 1-6, doi: 10.1109/CBMI50038.2021.9461918
Open-source version: https://hal.archives-ouvertes.fr/hal-03241475 -
Jacquemont, M.; Vuillaume, T.; Benoit, A.; Maurin, G. and Lambert, P. (2021). Multi-Task Architecture with Attention for Imaging Atmospheric Cherenkov Telescope Data Analysis. In Proceedings of the 16th International Joint Conference on Computer Vision, Imaging and Computer Graphics Theory and Applications - Volume 5: VISAPP, ISBN 978-989-758-488-6 ISSN 2184-4321, pages 534-544. DOI: 10.5220/0010297405340544
Open-source version: https://hal.archives-ouvertes.fr/hal-03043188 -
Jacquemont M., Vuillaume T., Benoit A., Maurin G., Lambert P. (2021) Deep Learning for Astrophysics, Understanding the Impact of Attention on Variability Induced by Parameter Initialization. In: Del Bimbo A. et al. (eds) Pattern Recognition. ICPR International Workshops and Challenges. ICPR 2021. Lecture Notes in Computer Science, vol 12663. Springer, Cham. https://doi.org/10.1007/978-3-030-68796-0_13
Open-source version: https://hal.archives-ouvertes.fr/hal-03043058 -
Jacquemont, M.; Antiga, L.; Vuillaume, T.; Silvestri, G.; Benoit, A.; Lambert, P. and Maurin, G. (2019). Indexed Operations for Non-rectangular Lattices Applied to Convolutional Neural Networks. In Proceedings of the 14th International Joint Conference on Computer Vision, Imaging and Computer Graphics Theory and Applications - Volume 5 VISAPP: VISAPP, ISBN 978-989-758-354-4, ISSN 2184-4321, pages 362-371. DOI: 10.5220/0007364303620371
Open-source version: https://hal.archives-ouvertes.fr/hal-02087157 -
Mikaël Jacquemont. GAMMALEARN: DEEP LEARNING APPLIED TO THE CHERENKOV TELESCOPE ARRAY (CTA). ICVSS 2018 - Computer Vision after Deep Learning, Jul 2018, Punta Sampieri, Italy. ⟨hal-01841581v2⟩
PhD thesis:
- Mikaël Jacquemont. Cherenkov Image Analysis with Deep Multi-Task Learning from Single-Telescope Data. Machine Learning [cs.LG]. Université Savoie Mont Blanc, 2020. English. ⟨tel-03148673⟩
Proceedings:
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Michaël Dell’aiera, Cyann Plard, Thomas Vuillaume, Sami Caroff, Alexandre Benoit, Deep Learning and IACT: bridging the gap between Monte-Carlo simulations and LST-1 data using domain adaptation, ADASS 2023, proceeding
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Pietro Grespan, Mikael Jacquemont, Rubèn López-Coto, Tjark Miener, Daniel Nieto-Castaño, Thomas Vuillaume et al Deep-learning-driven event reconstruction applied to simulated data from a single Large-Sized Telescope of CTA,
37th International Cosmic Ray Conference. 12-23 July 2021. Berlin, Germany - [arxiv]( https://doi.org/10.48550/arXiv.2109.14262 -
Vuillaume T., Jacquemont M., de Bony de Lavergne M., Sanchez D.~A., Poireau V., Maurin G., Benoit A., et al., Analysis of the Cherenkov Telescope Array first Large-Sized Telescope real data using convolutional neural networks, arXiv e-prints, 2021.
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Mikaël Jacquemont, Thomas Vuillaume, Alexandre Benoît, Gilles Maurin, Patrick Lambert. Single Imaging Atmospheric Cherenkov Telescope Full-Event Reconstruction with a Deep Multi-Task Learning Architecture. Astronomical Data Analysis Software and Systems ADASS XXX, Nov 2020, Granada, Spain. ⟨hal-03043005⟩
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D. Nieto, A. Brill, Q. Feng, M. Jacquemont, B. Kim, et al. Studying deep convolutional neural networks with hexagonal lattices for imaging atmospheric Cherenkov telescope event reconstruction. 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.753, ⟨10.22323/1.358.0753⟩. ⟨hal-02440010⟩
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Mikaël Jacquemont, Thomas Vuillaume, A Benoit, Gilles Maurin, Patrick Lambert, et al. GammaLearn: a Deep Learning framework for IACT data. 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.705. ⟨hal-02197399⟩
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Vuillaume, T., “GammaLearn - first steps to apply Deep Learning to the Cherenkov Telescope Array data”, in European Physical Journal Web of Conferences, 2019, vol. 214. doi:10.1051/epjconf/201921406020.