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First IACT waveform analysis based on deep convolutional neural networks using CTLearn

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00646040" target="_blank" >RIV/67985815:_____/25:00646040 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/25:00646040 RIV/61989592:15310/25:73635264

  • Result on the web

    <a href="https://pos.sissa.it/501/758/pdf" target="_blank" >https://pos.sissa.it/501/758/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.0758" target="_blank" >10.22323/1.501.0758</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    First IACT waveform analysis based on deep convolutional neural networks using CTLearn

  • Original language description

    Imaging atmospheric Cherenkov telescopes (IACTs) detect extended air showers (EASs) generated when very-high-energy (VHE) gamma rays or cosmic rays interact with the Earth's atmosphere. Cherenkov photons produced during an EAS are captured by fast-imaging cameras, which record both the spatial and temporal development of the shower, along with calorimetric data. By analyzing these recordings, the properties of the original VHE particle—such as its type, energy, and direction of arrival—can be reconstructed through machine learning techniques. This contribution focuses on the Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array Observatory, a next-generation ground-based gamma-ray observatory. LSTs are responsible for reconstructing lower-energy gamma rays in the tens of GeV range. We explore a novel event reconstruction technique based on deep convolutional neural networks (CNNs) applied on calibrated and cleaned waveforms of the IACT camera pixels using CTLearn. Our approach explicitly incorporates the time development of the shower, enabling a more accurate reconstruction of the event. This method eliminates the need for charge integration or handcrafted feature extraction, allowing the model to directly learn from waveform data.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Proceedings of Science

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    10

  • Pages from-to

    758

  • Publisher name

    Sissa Medilab srl

  • Place of publication

    Trieste

  • Event location

    Ženeva

  • Event date

    Jul 15, 2025

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article