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1. Chasing Gravitational Waves with the Cherenkov Telescope Array

2. The Real Time Analysis framework of the Cherenkov Telescope Array's Large-Sized Telescope

3. Analysis of the Cherenkov Telescope Array first Large-Sized Telescope real data using convolutional neural networks

4. First Full-Event Reconstruction from Imaging Atmospheric Cherenkov Telescope Real Data with Deep Learning

5. rta-dq-lib: a software library to perform online data quality analysis of scientific data

6. Polynomial data compression for large-scale physics experiments

7. pschitt! - A Python package for the modelling of atmoSpheric Showers and CHerenkov Imaging Terrestrial Telescopes

8. Deep Learning for Astrophysics, Understanding the Impact of Attention on Variability Induced by Parameter Initialization

9. Embedded star clusters as sources of high-energy cosmic rays: Modelling and constraints

10. Long term variability of the blazar PKS 2155-304

12. The northwestern ejecta knot in SN 1006

13. Nonthermal X-rays from low-energy cosmic rays: Application to the 6.4 keV line emission from the Arches cluster region

14. The Eta Carinae 2020 periastron passage as seen by H.E.S.S.

15. Detailed Design Of the Science Alert Generation of the ACADA System

16. Requirement Verification for Science Alert Generation Pipeline of the ACADA subystem

17. GammaLearn - first steps to apply Deep Learning to the Cherenkov Telescope Array data

18. Astronomy outreach in Namibia: H.E.S.S. and beyond

19. The young massive stellar cluster Westerlund 1 in gamma rays as seen with H.E.S.S.

20. Camera Calibration of the CTA-LST prototype

21. Detection of new Extreme BL Lac objects with H.E.S.S. and Swift XRT

22. Science verification of the new FlashCam-based camera in the 28m telescope of H.E.S.S.

23. The Science Alert Generation system of the Cherenkov Telescope Array Observatory.

27. The Array Control and Data Acquisition System of the Cherenkov Telescope Array

31. Algorithmes haute performance pour les télescopes atmosphériques Cherenkov

43. X-raying hadronic acceleration at the SN 1006 shock front

44. Origine du rayonnement cosmique : études multi-messagers, multi-longueurs d’onde

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