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@INPROCEEDINGS{Schlter:640179,
      author       = {Schlüter, Felix and Laub, Philipp and Nelles, Anna and
                      Bouma, S. and Bray, J. and Buitink, S. and Corstanje, A. and
                      De Henau, V. and Desmet, M. and Dickinson, E. and van
                      Dongen, L. and Hare, B. M. and He, H. and Hörandel, J. R.
                      and Huege, T. and James, C. W. and Jetti, M. and Mathes, H.
                      J. and Mulrey, K. and Scholten, O. and Sterpka, C. and ter
                      Veen, S. and Terveer, K. and Turekova, P. and Trinh, T. N.
                      G. and Saha, S. and Sharma, S. and Spencer, R. and Veberič,
                      D. and Watanabe, K. and Waterson, M. and Zhang, C. and
                      Zhang, P. and Zhang, Y.},
      title        = {{U}sing {SKA}-low to detect {P}e{V} gamma-rays from
                      {G}alactic {S}ources},
      journal      = {Proceedings of Science / International School for Advanced
                      Studies},
      volume       = {(ICRC2025)},
      issn         = {1824-8039},
      address      = {Trieste},
      publisher    = {SISSA},
      reportid     = {PUBDB-2025-04729},
      series       = {3067336},
      pages        = {835},
      year         = {2025},
      abstract     = {The Square Kilometre Array (SKA) is a next-generation radio
                      telescope, and upon construction in 2030 the world's most
                      sensitive one. SKA will comprise a low frequency component
                      with almost 60 000 radio antennas on an extremely densely
                      instrumented area of about 1 km$^2$ located in Australia.
                      Sensitive to the radio emission in the 50 to 350 MHz band,
                      these astonishing dimensions offer intriguing capabilities
                      for the detection of extensive air showers. While SKA will
                      play a leading role in high-precision cosmic ray
                      measurements, it may also play a role in gamma-ray
                      astronomy. The particle cascade initiated by a gamma ray
                      impacting on the Earth's atmosphere will emit radio waves,
                      comparable to the emission observed from hadronically
                      induced air showers. The energy threshold of current
                      radio-air-shower experiments of tens to hundreds of PeV has
                      limited those experiments to cosmic-ray science so far. With
                      the interferometric measurement of air showers combining the
                      coherent air-shower signals from thousands of individual
                      antennas, we aim at lowering the energy threshold for the
                      radio detection of air showers to PeV energies. The superior
                      angular resolution of SKA may provide a way to both trigger
                      on gamma-rays and separate them from hadronic cosmic rays.
                      SKA’s field of view of the Galactic Center provides a
                      unique opportunity of obtaining a first detection at PeV
                      energies. This contribution will sketch the challenges of as
                      well as the necessary steps needed for gamma-ray detection
                      with SKA and will highlight the scientific impact.},
      month         = {Jul},
      date          = {2025-07-14},
      organization  = {39th International Cosmic Ray
                       Conference, Geneva (Switzerland), 14
                       Jul 2025 - 24 Jul 2025},
      cin          = {Z-RAD},
      ddc          = {530},
      cid          = {I:(DE-H253)Z-RAD-20210408},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613) /
                      DFG project G:(GEPRIS)531213488 - Zeitlich hochaufgelöste
                      3D-Abbildung der Radioemission von kosmischen Luftschauern
                      mit LOFAR und SKA (531213488)},
      pid          = {G:(DE-HGF)POF4-613 / G:(GEPRIS)531213488},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.22323/1.501.0835},
      url          = {https://bib-pubdb1.desy.de/record/640179},
}