A

Improved Gamma-Hadron Separation for PeV Photon Searches with IceCube

International Cosmic Ray Conference, pp. 837

Abstract

IceTop, the km$^2$ surface array of the IceCube Neutrino Observatory at the South Pole, is sensitive to air showers of all primary particles, including gamma rays. In particular, in the PeV energy range, the combination of IceTop and IceCube’s deep optical detector provides excellent gamma-hadron separation. Almost all air showers induced by cosmic-ray protons and heavier nuclei in this energy range contain high-energy muons detectable by the deep detector, while most photon-induced air showers do not. Therefore, IceCube’s deep detector can be used to strongly suppress hadronic background in photon searches. Furthermore, the lateral distribution of the air-shower signal in IceTop provides additional gamma-hadron separation. In the PeV energy range, the gamma-hadron separation achieved is better than $10^{-3}$: air-shower events measured with IceCube are suppressed more than $1000$ times stronger than photon-induced showers of the same energy simulated with Sibyll 2.3d. This improved gamma-hadron separation in combination with an extension of the energy range to lower energies provides discovery potential for future searches for PeV photon sources in IceCube’s field of view.

Authors 95

  1. Université Libre de Bruxelles

    Affiliation as printed

    Université Libre de Bruxelles , Science Faculty CP230 , B-1050 Brussels , Belgium

  2. University of California, Berkeley

    Affiliation as printed

    Dept. of Physics , University of California , Berkeley , CA 94720 , USA

  3. Ruhr University Bochum

    Affiliation as printed

    Fakultät für Physik & Astronomie , Ruhr-Universität Bochum , D-44780 Bochum , Germany

  4. Karlsruhe Institute of Technology · The University of Adelaide

    Affiliation as printed

    Department of Physics , University of Adelaide , Adelaide , 5005 , Australia

    Institute for Astroparticle Physics , Karlsruhe Institute of Technology (KIT)

  5. University of Delaware · RWTH Aachen University

    Affiliation as printed

    Bartol Research Institute , Department of Physics and Astronomy , University of Delaware

    III. Physikalisches Institut , RWTH Aachen University , D-52056 Aachen , Germany

  6. Georgia Institute of Technology

    Affiliation as printed

    School of Physics and Center for Relativistic Astrophysics , Georgia Institute of Technology , Atlanta , GA 30332 , USA

  7. Karlsruhe Institute of Technology · The University of Adelaide

    Affiliation as printed

    Department of Physics , University of Adelaide , Adelaide , 5005 , Australia

    Institute for Astroparticle Physics , Karlsruhe Institute of Technology (KIT)

  8. University of Delaware · RWTH Aachen University

    Affiliation as printed

    Bartol Research Institute , Department of Physics and Astronomy , University of Delaware

    III. Physikalisches Institut , RWTH Aachen University , D-52056 Aachen , Germany

  9. Université Libre de Bruxelles

    Affiliation as printed

    Université Libre de Bruxelles , Science Faculty CP230 , B-1050 Brussels , Belgium

  10. University of Delaware · RWTH Aachen University

    Affiliation as printed

    Bartol Research Institute , Department of Physics and Astronomy , University of Delaware

    III. Physikalisches Institut , RWTH Aachen University , D-52056 Aachen , Germany

  11. University of Delaware · RWTH Aachen University

    Affiliation as printed

    Bartol Research Institute , Department of Physics and Astronomy , University of Delaware

    III. Physikalisches Institut , RWTH Aachen University , D-52056 Aachen , Germany

Cited by 0 stored of 0

No patents citing this paper on Lens.org (checked 2026-10-06).

References 0