29 June 2026 to 3 July 2026
Hospederia San Martin Pinario
Europe/Rome timezone

Session

Parallel session - MM

2 Jul 2026, 16:30
Salon Peregrinos (Hospederia San Martin Pinario)

Salon Peregrinos

Hospederia San Martin Pinario

Presentation materials

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  1. Alan Andrew Watson
    02/07/2026, 16:30
    MM - Multimessenger: Gamma-rays, Neutrinos, Dark Matter
    Oral contribution

    Cygnus X-3 Revisited
    A A Watson
    School of Physics and Astronomy, University of Leeds, UK
    a.a.watson@leeds.ac.uk
    During the 1980s there were reports of emission of γ-rays at TeV and PeV energies from the X-ray binary system, Cygnus X-3. However, following these claims, more detailed studies with purpose-built detectors, such as those with the GREX array at Haverah Park and with the much...

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  2. Francesco Loparco (Universita e INFN, Bari (IT))
    02/07/2026, 16:45
    1
    MM - Multimessenger: Gamma-rays, Neutrinos, Dark Matter
    Oral contribution

    We search for possible line-like and box-shaped spectral features in the Galactic gamma-ray spectra measured by the Fermi Large Area Telescope in its first 17 years of operation in the 1 GeV – 1 TeV energy range. Such features could be produced by dark matter particles accumulated in the Milky Way halo, which could either self-annihilate or decay, yielding gamma rays in the final state....

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  3. Costanza Marinelli (Gran Sasso Science Institute, Istituto Nazionale di Fisica Nucleare)
    02/07/2026, 17:00
    MM - Multimessenger: Gamma-rays, Neutrinos, Dark Matter
    Oral contribution

    We present a new statistical approach to search for ultra-high-energy photons in extensive air-shower data, aimed at enhancing sensitivity in regimes dominated by hadronic background, where the identification of individual photon candidates is challenging. The method quantifies the collective deviation of the data from the background expectation through a likelihood-ratio hypothesis test...

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  4. Dr Chaitanya Priyadarshi (Instytut Fizyki Jadrowej PAN, Kraków)
    02/07/2026, 17:15
    MM - Multimessenger: Gamma-rays, Neutrinos, Dark Matter
    Oral contribution

    Direction-time clustering methods for neutral particle searches are motivated by the possibility that ultra-high-energy (UHE) neutral particles are produced during flaring periods of various astrophysical sources. In this scenario, clusters of events correlated in both arrival direction and time would be generated, which, when observed, would indicate a neutral-particle flare, and a...

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  5. Enrique Zas
    02/07/2026, 17:30
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