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Searching for gamma-ray counterparts of FRBs with H.E.S.S.
Aharonian, F. ; Benkhali, F. A. ; Alkan, A. ; Aschersleben, J. ; Ashkar, H. ; Backes, M. ; Baktash, A. ; Barbosa Martins, V.DESY* ; Barnacka, A. ; Barnard, J. ; Batzofin, R. ; Becherini, Y. ; Beck, G. ; Berge, D.DESY* ; Bernlöhr, K. ; Bi, B. ; Böttcher, M. ; Boisson, C. ; Bolmont, J. ; de Bony de Lavergne, M. ; Borowska, J. ; Bouyahiaoui, M. ; Bradascio, F. ; Breuhaus, M. ; Brose, R. ; Brown, A. ; Brun, F. ; Bruno, B. ; Bulik, T. ; Burger-Scheidlin, C. ; Bylund, T. ; Cangemi, F. ; Caroff, S. ; Casanova, S. ; Cecil, R. ; Celic, J. ; Cerruti, M. ; Chambery, P. ; Chand, T. ; Chandra, S. ; Chen, A. ; Chibueze, J. ; Chibueze, O. ; Collins, T. ; Cotter, G. ; Cristofari, P. ; Mbarubucyeye, J. D.DESY* ; Davids, I. D. ; Davies, J. ; de Jonge, L. ; Devin, J. ; Djannati-Ataï, A. ; Dmytriiev, A. ; Doroshenko, V. ; Dreyer, L. ; Du Plessis, L. ; Egberts, K. ; Einecke, S. ; Ernenwein, J.-P. ; Fegan, S. ; Feijen, K. ; de Clairfontaine, G. F. ; Fontaine, G. ; Lott, F. ; Füßling, M.Extern* ; Funk, S. ; Gabici, S. ; Gallant, Y. A. ; Ghafourizadeh, S. ; Giavitto, G.DESY* ; Giunti, L. ; Glawion, D. ; Glicenstein, J. F. ; Glombitza, J. ; Goswami, P. ; Grolleron, G. ; Grondin, M.-H. ; Haerer, L. ; Hattingh, S. ; Haupt, M.DESY* ; Hermann, G. ; Hinton, J. A. ; Hofmann, W. ; Holch, T. L.DESY* ; Holler, M. ; Horns, D. ; Huang, Z. ; Jaitly, A. (Corresponding author)Extern*DESY* ; Jamrozy, M. ; Jankowsky, F. ; Jardin-Blicq, A. ; Joshi, V. ; Jung-Richardt, I. ; Kasai, E. ; Katarzyński, K. ; Katjaita, H. ; Khangulyan, D. ; Khatoon, R. ; Khélifi, B. ; Klepser, S.DESY* ; Kluźniak, W. ; Komin, N. ; Konno, R. ; Kosack, K. ; Kostunin, D.DESY* ; Kundu, A. ; Lamanna, G. ; Lang, R. G. ; Le Stum, S. ; Lefranc, V. ; Leitl, F. ; Lemière, A. ; Lemoine-Goumard, M. ; Lenain, J.-P. ; Leuschner, F. ; Luashvili, A. ; Lypova, I. ; Mackey, J. ; Malyshev, D. ; Malyshev, D. ; Marandon, V. ; Marcowith, A. ; Marinos, P. ; Martí-Devesa, G. ; Marx, R. ; Maurin, G. ; Mehta, A. ; Meintjes, P. J. ; Meyer, M. ; Mitchell, A. ; Moderski, R. ; Mohrmann, L. ; Montanari, A. ; Moore, C. ; Moulin, E. ; Murach, T.DESY* ; Nakashima, K. ; de Naurois, M. ; Ndiyavala, H. ; Niemiec, J. ; Noel, A. P. ; O'Brien, P. ; Ohm, S.DESY* ; Olivera-Nieto, L. ; de Ona Wilhelmi, E.Extern*DESY* ; Ostrowski, M. ; Oukacha, E. ; Panny, S. ; Panter, M. ; Parsons, R. D. ; Pensec, U. ; Peron, G. ; Pita, S. ; Poireau, V. ; Prokhorov, D. A. ; Prokoph, H.DESY* ; Pühlhofer, G. ; Punch, M. ; Quirrenbach, A. ; Regeard, M. ; Reichherzer, P. ; Reimer, A. ; Reimer, O. ; Reis, I. ; Remy, Q. ; Ren, H. ; Renaud, M. ; Reville, B. ; Rieger, F. ; Roellinghoff, G. ; Rol, E. ; Rowell, G. ; Rudak, B. ; Ricarte, H. R. ; Ruiz-Velasco, E. ; Sabri, K. ; Sahakian, V. ; Sailer, S. ; Salzmann, H. ; Sanchez, D. A. ; Santangelo, A. ; Sasaki, M. ; Schäfer, J. ; Schüssler, F. ; Schutte, H. M. ; Senniappan, M. ; Shapopi, J. N. S. ; Shilunga, S. ; Shiningayamwe, K. ; Sol, H. ; Spackman, H. ; Specovius, A. ; Spencer, S. ; Stawarz, Ł. ; Steenkamp, R. ; Stegmann, C.DESY* ; Steinmassl, S. ; Steppa, C. ; Streil, K. ; Sushch, I. ; Suzuki, H. ; Takahashi, T. ; Tanaka, T. ; Tavernier, T. ; Taylor, A. M.DESY* ; Terrier, R. ; Thakur, A. ; Thiersen, J. H. E. ; Thorpe-Morgan, C. ; Tluczykont, M. ; Tsirou, M.DESY* ; Tsuji, N. ; Tuffs, R. ; Uchiyama, Y. ; Ullmo, M. ; Unbehaun, T. ; van der Merwe, P. ; van Eldik, C. ; van Soelen, B. ; Vasileiadis, G. ; Vecchi, M. ; Veh, J. ; Venter, C. ; Vink, J. ; Völk, H. J. ; Vogel, N. ; Wach, T. ; Wagner, S. J. ; Werner, F. ; White, R. ; Wierzcholska, A. ; Wong, Y. W. ; Yassin, H. ; Zacharias, M. ; Zargaryan, D. ; Zdziarski, A. A. ; Zech, A. ; Zhu, S. J.DESY* ; Zmija, A. ; Zouari, S. ; Żywucka, N. ; HESS Collaboration (Collaboration author)
2023
SISSA
Trieste
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Please use a persistent id in citations: doi:10.22323/1.444.0776 doi:10.3204/PUBDB-2023-05297
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 a mystery. One of themost accredited models suggests that they originate from highly magnetized and rapidly spinningneutron stars known as magnetars. The high luminosity, short duration, and high dispersionmeasure of these events suggest they result from extreme, high-energy astrophysical processesof extragalactic origin. The number of detected FRBs, including repeating ones, has grownrapidly in recent years. Except for FRB20200428, that is associated to the galactic magnetar SGR1925+2154, no multi-wavelength counterparts to any FRB has been detected yet. The HighEnergy Stereoscopic System (H.E.S.S.) telescope has developed a program to uncover the natureof these mysterious events by searching for their gamma-ray counterparts. This contributionprovides an overview of the searches for FRB sources conducted by H.E.S.S., including follow-upobservations and simultaneous multi-wavelength campaigns with radio and X-ray observatories
Keyword(s): luminosity: high ; HESS ; burst ; gamma ray: VHE ; observatory ; star ; neutron star ; magnetar ; X-ray ; galaxy
Contributing Institute(s):
- Cherenkov Telescope Array (Z_CTA)
- High Energy Steroscopic System (ZEU-HESS)
Research Program(s):
- 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
Experiment(s):
- Cherenkov Telescope Array
- High Energy Stereoscopic System
Appears in the scientific report
2023
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