% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @INPROCEEDINGS{Aharonian:593113, author = {Aharonian, F. and Benkhali, F. Ait and Alkan, A. and Aschersleben, J. and Ashkar, H. and Backes, M. and Baktash, A. and Barbosa Martins, V. and Barnacka, A. and Barnard, J. and Batzofin, R. and Becherini, Y. and Beck, G. and Berge, D. and Bernlöhr, K. and Bi, B. and Böttcher, M. and Boisson, C. and Bolmont, J. and de Bony de Lavergne, M. and Borowska, J. and Bouyahiaoui, M. and Bradascio, F. and Breuhaus, M. and Brose, R. and Brown, A. and Brun, F. and Bruno, B. and Bulik, T. and Burger-Scheidlin, C. and Bylund, T. and Cangemi, F. and Caroff, S. and Casanova, S. and Cecil, R. and Celic, J. and Cerruti, M. and Chambery, P. and Chand, T. and Chandra, S. and Chen, A. and Chibueze, J. and Chibueze, O. and Collins, T. and Cotter, G. and Cristofari, P. and Mbarubucyeye, J. Damascene and Davids, I. D. and Davies, J. and de Jonge, L. and Devin, J. and Djannati-Ataï, A. and Dmytriiev, A. and Doroshenko, V. and Dreyer, L. and Du Plessis, L. and Egberts, K. and Einecke, S. and Ernenwein, J.-P. and Fegan, S. and Feijen, K. and de Clairfontaine, G. Fichet and Fontaine, G. and Lott, F. and Füßling, M. and Funk, S. and Gabici, S. and Gallant, Y. A. and Ghafourizadeh, S. and Giavitto, G. and Giunti, L. and Glawion, D. and Glicenstein, J. F. and Glombitza, J. and Goswami, P. and Grolleron, G. and Grondin, M.-H. and Haerer, L. and Hattingh, S. and Haupt, M. and Hermann, G. and Hinton, J. A. and Hofmann, W. and Holch, T. L. and Holler, M. and Horns, D. and Huang, Zhiqiu and Jaitly, Annanay and Jamrozy, M. and Jankowsky, F. and Jardin-Blicq, A. and Joshi, V. and Jung-Richardt, I. and Kasai, E. and Katarzyński, K. and Katjaita, H. and Khangulyan, D. and Khatoon, R. and Khélifi, B. and Klepser, S. and Kluźniak, W. and Komin, Nu. and Konno, R. and Kosack, K. and Kostunin, D. and Kundu, A. and Lamanna, G. and Lang, R. G. and Le Stum, S. and Lefranc, V. and Leitl, F. and Lemière, A. and Lemoine-Goumard, M. and Lenain, J.-P. and Leuschner, F. and Luashvili, A. and Lypova, I. and Mackey, J. and Malyshev, D. and Malyshev, D. and Marandon, V. and Marcowith, A. and Marinos, P. and Martí-Devesa, G. and Marx, R. and Maurin, G. and Mehta, A. and Meintjes, P. J. and Meyer, M. and Mitchell, A. and Moderski, R. and Mohrmann, L. and Montanari, A. and Moore, C. and Moulin, E. and Murach, T. and Nakashima, K. and de Naurois, M. and Ndiyavala, H. and Niemiec, J. and Noel, A. Priyana and O'Brien, P. and Ohm, S. and Olivera-Nieto, L. and de Ona Wilhelmi, E. and Ostrowski, M. and Oukacha, E. and Panny, S. and Panter, M. and Parsons, R. D. and Pensec, U. and Peron, G. and Pita, S. and Poireau, V. and Prokhorov, D. A. and Prokoph, H. and Pühlhofer, G. and Punch, M. and Quirrenbach, A. and Regeard, M. and Reichherzer, P. and Reimer, A. and Reimer, O. and Reis, I. and Remy, Q. and Ren, H. and Renaud, M. and Reville, B. and Rieger, F. and Roellinghoff, G. and Rol, E. and Rowell, G. and Rudak, B. and Ricarte, H. Rueda and Ruiz-Velasco, E. and Sabri, K. and Sahakian, V. and Sailer, S. and Salzmann, H. and Sanchez, D. A. and Santangelo, A. and Sasaki, M. and Schäfer, J. and Schüssler, F. and Schutte, H. M. and Senniappan, M. and Shapopi, J. N. S. and Shilunga, S. and Shiningayamwe, K. and Sol, H. and Spackman, H. and Specovius, A. and Spencer, S. and Stawarz, Ł. and Steenkamp, R. and Stegmann, C. and Steinmassl, S. and Steppa, C. and Streil, K. and Sushch, I. and Suzuki, H. and Takahashi, T. and Tanaka, T. and Tavernier, T. and Taylor, A. M. and Terrier, R. and Thakur, A. and Thiersen, J. H. E. and Thorpe-Morgan, C. and Tluczykont, M. and Tsirou, M. and Tsuji, N. and Tuffs, R. and Uchiyama, Y. and Ullmo, M. and Unbehaun, T. and van der Merwe, P. and van Eldik, C. and van Soelen, B. and Vasileiadis, G. and Vecchi, M. and Veh, J. and Venter, C. and Vink, J. and Völk, H. J. and Vogel, N. and Wach, T. and Wagner, S. J. and Werner, F. and White, R. and Wierzcholska, A. and Wong, Yu Wun and Yassin, H. and Zacharias, M. and Zargaryan, D. and Zdziarski, A. A. and Zech, A. and Zhu, S. J. and Zmija, A. and Zouari, S. and Żywucka, N.}, collaboration = {{HESS Collaboration}}, title = {{S}earching for gamma-ray counterparts of {FRB}s with {H}.{E}.{S}.{S}.}, journal = {Proceedings of Science / International School for Advanced Studies}, volume = {(ICRC2023)}, issn = {1824-8039}, address = {Trieste}, publisher = {SISSA}, reportid = {PUBDB-2023-05297}, pages = {776}, year = {2023}, 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}, month = {Jul}, date = {2023-07-26}, organization = {38th International Cosmic Ray Conference, Nagoya (Japan), 26 Jul 2023 - 3 Aug 2023}, keywords = {luminosity: high (INSPIRE) / HESS (INSPIRE) / burst (INSPIRE) / gamma ray: VHE (INSPIRE) / observatory (INSPIRE) / star (INSPIRE) / neutron star (INSPIRE) / magnetar (INSPIRE) / X-ray (INSPIRE) / galaxy (INSPIRE)}, cin = {$Z_CTA$ / ZEU-HESS}, ddc = {530}, cid = {$I:(DE-H253)Z_CTA-20210408$ / I:(DE-H253)ZEU-HESS-20140213}, pnm = {613 - Matter and Radiation from the Universe (POF4-613)}, pid = {G:(DE-HGF)POF4-613}, experiment = {EXP:(DE-H253)CTA-20150101 / EXP:(DE-H253)HESS-20170101}, typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8}, doi = {10.22323/1.444.0776}, url = {https://bib-pubdb1.desy.de/record/593113}, }