Contribution List

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  1. Lucio Angelo Antonelli (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 11:30
  2. Roberta Zanin (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 11:40
  3. Massimo Cappi (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 12:00
  4. Francesco Longo
    29/05/2023, 12:20
  5. Antonio Stamerra (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 12:40
  6. Fabio Pintore (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 14:30
  7. Michela Rigoselli (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 15:00

    In recent years the number of known sources emitting in the TeV-PeV regime has increased significantly thanks to facilities like LHAASO and HAWC. The more natural candidates, for energetic and ambient properties, are pulsars and their environment.

    However, due to the limited angular resolution of the current instruments, many of the observed sources have more than one lower-energy...

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  8. 29/05/2023, 15:20
  9. Elisa Prandini (DFA Padova)
    29/05/2023, 16:30
  10. Paolo Giommi (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 16:50
  11. Dario Gasparrini (Istituto Nazionale di Fisica Nucleare sez. di Roma Tor Vergata)
    29/05/2023, 17:10
  12. Irene Burelli (University of Udine - INFN Trieste)
    29/05/2023, 17:30
  13. Alberto Ulgiati (Istituto Nazionale di Astrofisica (INAF)), Simona Paiano (Istituto Nazionale di Astrofisica (INAF))
    29/05/2023, 17:50
  14. 29/05/2023, 18:00
  15. Dr Sandro Mereghetti (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 09:00
  16. Alessandro Papitto (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 09:30
  17. Niccolo' Bucciantini (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 09:50
  18. 30/05/2023, 10:10
  19. 30/05/2023, 10:30
  20. Alessandro Carosi (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 11:30
  21. Biswajit Banerjee (Gran Sasso Science Institute (GSSI))
    30/05/2023, 12:00
  22. Lara Nava (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 12:20
  23. 30/05/2023, 12:40
  24. Dr Martina Cardillo (INAF- IAPS)
    30/05/2023, 14:30
  25. 30/05/2023, 15:20
  26. Fabio Pintore (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 16:30
  27. Gabriele Ponti (Istituto Nazionale di Astrofisica (INAF))
    30/05/2023, 17:10
  28. 30/05/2023, 17:30
  29. Gianfranco Brunetti (Istituto Nazionale di Astrofisica (INAF))
    31/05/2023, 09:00
  30. 31/05/2023, 09:40
  31. Elena Pian (Istituto Nazionale di Astrofisica (INAF))
    31/05/2023, 10:20
  32. Claudia Maria Raiteri (Istituto Nazionale di Astrofisica (INAF))
    31/05/2023, 10:40
    Oral contribution

    Born in 1997 to provide an optical follow-up of gamma-loud blazars observed by the Compton Gamma Ray Observatory, the Whole Earth Blazar Telescope (WEBT) is a large collaboration including several tens of astronomers around the northern hemisphere who monitor blazars mainly in the optical (including polarimetry), but also in the radio and near-infrared bands. Since 2000 the Collaboration has...

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  33. Dr Francesco Gabriele Saturni (Istituto Nazionale di Astrofisica (INAF))
    31/05/2023, 11:30
  34. Giorgio Galanti (Istituto Nazionale di Astrofisica (INAF))
    31/05/2023, 12:05
  35. Davide Miceli (University & INFN Padova)
    31/05/2023, 12:25
  36. 31/05/2023, 12:45
  37. Dr Michela Rigoselli (Istituto Nazionale di Astrofisica (INAF))
    Oral contribution

    In recent years the number of known sources emitting in the TeV-PeV regime has increased significantly thanks to facilities like LHAASO and HAWC. The more natural candidates, for energetic and ambient properties, are pulsars and their environment.

    However, due to the limited angular resolution of the current instruments, many of the observed sources have more than one lower-energy...

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  38. Niccolo' Bucciantini (Istituto Nazionale di Astrofisica (INAF))
    Oral contribution

    Despite the long held assumption that PWNe at high energy could be counted as "stable candles", detection of gamma-ray flares in the Crab nebula, led us to revisit our ideas about the working of such systems. Given the lack of resolution of current gamma-ray observations, analysis of variability was performed at other wavelengths in search for possible counterparts that could guide us to the...

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  39. Dr Elena Pian (INAF-OAS, Bologna)
    Oral contribution

    TeV emitters are typically multi-wavelength sources, generally highly variable and occasionally highly polarized. This makes it critical to line up ground-based dedicated facilities for identification, follow-up and monitoring of CTA targets in polarized and total radio-to-optical light. Furthermore, the CTA itself provides suitable infrastructure for the implementation of specific observing...

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