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@ARTICLE{Aharonian:642329,
      author       = {Aharonian, F. and Archaryya, A. and Aschersleben, J. and
                      Ashkar, H. and Backes, M. and Barbosa Martins, Victor and
                      Batzofin, R. and Becherini, Y. and Berge, D. and Bernlohr,
                      K. and Bottcher, M. and Boisson, C. and Bolmont, J. and de
                      Bony de Lavergne, M. and Borowska, J. and Bradascio, F. and
                      Brose, R. and Brown, A. and Brun, F. and Bruno, B. and
                      Burger-Scheidlin, C. and Casanova, S. and Celic, J. and
                      Cerruti, M. and Chand, T. and Chandra, S. and Chen, A. and
                      Chibueze, J. and Chibueze, O. and Damascene Mbarubucyeye, J.
                      and de Assis Scarpin, J. and Djannati-Atai, A. and
                      Djuvsland, J. and Dmytriiev, A. and Egberts, K. and Einecke,
                      S. and Ernenwein, J.-P. and Escanuela Nieves, C. and
                      Filipovic, M. and Fontaine, G. and Funk, S. and Gabici, S.
                      and Glicenstein, J. F. and Glombitza, J. and Grolleron, G.
                      and Heß, B. and Hofmann, W. and Holch, Tim Lukas and
                      Holler, M. and Horns, D. and Huang, Zhiqiu and Jaitly, A.
                      and Jamrozy, M. and Jankowsky, F. and Jung-Richardt, I. and
                      Kasai, E. and Katarzynski, K. and Kerszberg, D. and Khatoon,
                      R. and Khelifi, B. and Kluzniak, W. and Komin, Nu. and
                      Kosack, K. and Kostunin, D. and Kundu, A. and Lang, R. G.
                      and Le Stum, S. and Lemière, A. and Lemoine-Goumard, M. and
                      Lenain, J.-P. and Luashvili, A. and Mackey, J. and Malyshev,
                      D. and Marandon, V. and Marx, R. and Mehta, A. and Meyer, M.
                      and Mitchell, A. and Moderski, R. and Moghadam, M. O. and
                      Moulin, E. and de Naurois, M. and Niemiec, J. and O'Brien,
                      P. and Olivera-Nieto, L. and de Ona Wilhelmi, Emma Maria and
                      Ostrowski, M. and Panny, S. and Panter, M. and Pensec, U.
                      and Parsons, R. D. and Pita, S. and Puhlhofer, G. and Punch,
                      M. and Quirrenbach, A. and Ravikularaman, S. and Regeard, M.
                      and Reimer, O. and Ren, H. and Reville, B. and Rieger, F.
                      and Rowell, G. and Rudak, B. and Sabri, K. and Sahakian, V.
                      and Salzmann, H. and Santangelo, A. and Sasaki, M. and
                      Schäfer, J. and Schussler, F. and Schutte, H. M. and
                      Shapopi, J. N. S. and Sharma, A. and Spencer, S. and
                      Stawarz, L. and Steenkamp, R. and Steinmassl, S. and Steppa,
                      C. and Takahashi, T. and Tanaka, T. and Tsirou, M. and van
                      Eldik, C. and Vecchi, M. and Venter, C. and Wach, T. and
                      Wagner, S. J. and Wierzcholska, A. and Zdziarski, A. A. and
                      Zech, A. and Zywucka, N.},
      collaboration = {H. E. S. S.{ Collaboration}},
      title        = {{H}.{E}.{S}.{S}. programme searching for {VHE} gamma rays
                      associated with {FRB}s},
      journal      = {Journal of cosmology and astroparticle physics},
      volume       = {07},
      number       = {07},
      issn         = {1475-7508},
      address      = {London},
      publisher    = {IOP},
      reportid     = {PUBDB-2025-05484, arXiv:2507.02143},
      pages        = {086},
      year         = {2025},
      abstract     = {Fast Radio Bursts (FRBs) are highly energetic, extremely
                      short-lived bursts of radio flashes. Despite extensive
                      research, the exact cause of these outbursts remains
                      speculative. The high luminosity, short duration, and high
                      dispersion measure of these events suggest they result from
                      extreme, high-energy extragalactic sources, such as highly
                      magnetized and rapidly spinning neutron stars known as
                      magnetars. The number of detected FRBs, including repeating
                      ones, has grown rapidly in recent years. Except for FRB
                      20200428D, and FRB-like radio burst that is associated to
                      Galactic magnetar SGR 1935+2154, no multi-wavelength
                      counterpart to any FRB has been detected yet. The High
                      Energy Stereoscopic System (H.E.S.S.) telescope has
                      developed a program to follow up FRBs searching for their
                      gamma-ray counterparts, helping to uncover the nature of
                      FRBs and FRB sources.This paper provides an overview of the
                      searches for FRB sources conducted by H.E.S.S., including
                      follow-up observations and simultaneous multi-wavelength
                      campaigns with radio and X-ray observatories. Among the FRB
                      sources observed by H.E.S.S., nine are localized with
                      redshifts ranging between 0.11 and 0.492 from 2015 to 2022.
                      No significant very high energy (VHE) emission was detected
                      during these observations. We report constraints on the VHE
                      luminosity ranging from 10$^{44}$ erg s$^{-1}$ and 10$^{48}$
                      erg s$^{-1}$, placing limits on the FRB's region persistent
                      VHE emission and potential FRB afterglow emission across
                      timescales from hours to years.},
      keywords     = {gamma ray experiments (autogen) / neutron stars (autogen) /
                      radio pulsars (autogen)},
      cin          = {$Z_GA$},
      ddc          = {530},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)HESS-20170101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2507.02143},
      howpublished = {arXiv:2507.02143},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2507.02143;\%\%$},
      doi          = {10.1088/1475-7516/2025/07/086},
      url          = {https://bib-pubdb1.desy.de/record/642329},
}