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@ARTICLE{Corstanje:625908,
      author       = {Corstanje, A. and Buitink, S. and Bouma, Sjoerd and Desmet,
                      M. and Huege, T. and Laub, P. and Mulrey, K. and Nelles,
                      Anna and Scholten, O. and Terveer, K. and Watanabe, K.},
      title        = {{A} {LOFAR}-style reconstruction of cosmic-ray air showers
                      with {SKA}-{L}ow},
      journal      = {Physical review / D},
      volume       = {112},
      number       = {2},
      issn         = {2470-0010},
      address      = {Ridge, NY},
      publisher    = {American Physical Society},
      reportid     = {PUBDB-2025-01233, arXiv:2504.16873},
      pages        = {023017},
      year         = {2025},
      note         = {14 pages, 10 figures. Accepted for publication in Phys.
                      Rev. D},
      abstract     = {Cosmic-ray air shower detection with the low-frequency part
                      of the Square Kilometre Array (SKA) radio telescope is
                      envisioned to yield very high precision measurements of the
                      particle composition of cosmic rays between 1016 and 1018
                      eV. This is made possible by the extreme antenna density of
                      the core of SKA-Low, surpassing the current most dense radio
                      air shower observatory LOFAR by over an order of magnitude.
                      In order to make these measurements, the technical
                      implementation of this observation mode and the development
                      of reconstruction methods have to happen hand in hand. As a
                      first lower limit of what is obtainable, we apply the
                      current most precise reconstruction methods as used at LOFAR
                      to a first complete simulation of air shower signals for the
                      SKA-Low array. We describe this simulation setup and discuss
                      the obtainable accuracy and resolution. A special focus is
                      put on effects of the dynamic range of the system,
                      beam-forming methods to lower the energy threshold, as well
                      as the limits to the mass composition accuracy given by
                      statistical and systematic uncertainties.},
      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},
      eprint       = {2504.16873},
      howpublished = {arXiv:2504.16873},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2504.16873;\%\%$},
      doi          = {10.1103/l8mt-994v},
      url          = {https://bib-pubdb1.desy.de/record/625908},
}