H.E.S.S. programme searching for VHE gamma rays associated with FRBs

Aharonian F, Archaryya A, Aschersleben J, Ashkar H, Backes M, Barbosa Martins V, Batzofin R, Becherini Y, Berge D, Bernlöhr K, Böttcher M, Boisson C, Bolmont J, de Bony de Lavergne M, Borowska J, Bradascio F, Brose R, Brown A, Brun F, Bruno B, Burger-Scheidlin C, Casanova S, Celic J, Cerruti M, Chand T, Chandra S, Chen A, Chibueze J, Chibueze O, Damascene Mbarubucyeye J, de Assis Scarpin J, Djannati-Ataï A, Djuvsland J, Dmytriiev A, Egberts K, Einecke S, Ernenwein JP, Escañuela Nieves C, Filipovic M, Fontaine G, Funk S, Gabici S, Glicenstein JF, Glombitza J, Grolleron G, Heß B, Hofmann W, Holch TL, Holler M, Horns D, Huang Z, Jaitly A, Jamrozy M, Jankowsky F, Jung-Richardt I, Kasai E, Katarzyński K, Kerszberg D, Khatoon R, Khélifi B, Kluźniak W, Komin N, Kosack K, Kostunin D, Kundu A, Guedes Lang R, Le Stum S, Lemière A, Lemoine-Goumard M, Lenain JP, Luashvili A, Mackey J, Malyshev D, Marandon V, Marx R, Mehta A, Meyer M, Mitchell A, Moderski R, Moghadam MO, Moulin E, de Naurois M, Niemiec J, O'Brien P, Olivera-Nieto L, de Ona Wilhelmi E, Ostrowski M, Panny S, Panter M, Parsons RD, Pensec U, Pita S, Pühlhofer G, Punch M, Quirrenbach A, Ravikularaman S, Regeard M, Reimer O, Ren H, Reville B, Rieger F, Rowell G, Rudak B, Sabri K, Sahakian V, Salzmann H, Santangelo A, Sasaki M, Schäfer J, Schüssler F, Schutte HM, Shapopi JN, Sharma A, Spencer S, Stawarz Ł, Steenkamp R, Steinmassl S, Steppa C, Takahashi T, Tanaka T, Tsirou M, van Eldik C, Vecchi M, Venter C, Wach T, Wagner SJ, Wierzcholska A, Zdziarski AA, Zech A, Żywucka N (2025)


Publication Type: Journal article

Publication year: 2025

Journal

Book Volume: 2025

Article Number: 086

Journal Issue: 7

DOI: 10.1088/1475-7516/2025/07/086

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 1044 erg s-1 and 1048 erg s-1, placing limits on the FRB's region persistent VHE emission and potential FRB afterglow emission across timescales from hours to years.

Authors with CRIS profile

Involved external institutions

Eberhard Karls Universität Tübingen DE Germany (DE) Institute of Research into the Fundamental Laws of the Universe / Institut de recherche sur les lois fondamentales de l'univers (IRFU) FR France (FR) Noordwes-Universiteit / North-West University ZA South Africa (ZA) University of Namibia (UNAM) NA Namibia (NA) Université Paris Cité FR France (FR) Jagiellonian University / Uniwersytet Jagielloński (UJ) PL Poland (PL) Max-Planck-Institut für Kernphysik (MPIK) / Max Planck Institute for Nuclear Physics DE Germany (DE) Dublin Institute for Advanced Studies (DIAS) IE Ireland (IE) University of Southern Denmark / Syddansk Universitet DK Denmark (DK) University of Groningen / Rijksuniversiteit Groningen NL Netherlands (NL) Sorbonne Université FR France (FR) Humboldt-Universität zu Berlin DE Germany (DE) University of Oxford GB United Kingdom (GB) Laboratoire Leprince-Ringuet (LLR) FR France (FR) Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences PL Poland (PL) University of the Witwatersrand (WITS) ZA South Africa (ZA) Université Paris-Saclay FR France (FR) Deutsches Elektronen-Synchrotron DESY DE Germany (DE) Institut national de physique nucléaire et de physique des particules (IN2P3) FR France (FR) Université de Bordeaux FR France (FR) Institute of Nuclear Physics Polish Academy of Sciences / Instytut Fizyki Jądrowej im. Henryka Niewodniczańskiego Polskiej Akademii Nauk PL Poland (PL) Leopold-Franzens-Universität Innsbruck / University of Innsbruck AT Austria (AT) Universität Potsdam DE Germany (DE) University of Adelaide AU Australia (AU) University of Montpellier / Université Montpellier FR France (FR) Yerevan State University / Երեվանի Պետական Համալսարան (YSU) AM Armenia (AM) University of Tokyo JP Japan (JP) Konan University / 甲南大学 JP Japan (JP) Laboratoire Univers et Théories (LUTH) / Laboratory of the Universe and Theories FR France (FR) University of Western Sydney AU Australia (AU) Ruprecht-Karls-Universität Heidelberg DE Germany (DE) Nicolaus Copernicus University (NCU) / Uniwersytet Mikołaja Kopernika w Toruniu (UMK) PL Poland (PL) University of Leicester GB United Kingdom (GB) Universität Hamburg (UHH) DE Germany (DE)

How to cite

APA:

Aharonian, F., Archaryya, A., Aschersleben, J., Ashkar, H., Backes, M., Barbosa Martins, V.,... Żywucka, N. (2025). H.E.S.S. programme searching for VHE gamma rays associated with FRBs. Journal of Cosmology and Astroparticle Physics, 2025(7). https://doi.org/10.1088/1475-7516/2025/07/086

MLA:

Aharonian, F., et al. "H.E.S.S. programme searching for VHE gamma rays associated with FRBs." Journal of Cosmology and Astroparticle Physics 2025.7 (2025).

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