Search Results - "Ghafourizadeh, S"

TeV flaring activity of the AGN PKS 0625-354 in November 2018 by Collaboration, H. E. S. S, Aschersleben, J, Ashkar, H, Backes, M, Baktash, A, Martins, V. Barbosa, Batzofin, R, Becherini, Y, Berge, D, Bernlöhr, K, Bi, B, Böttcher, M, Boisson, C, Bolmont, J, de Lavergne, M. de Bony, Breuhaus, M, Brose, R, Bruno, B, Bulik, T, Bylund, T, Casanova, S, Celic, J, Cerruti, M, Chandra, S, Chen, A, Chibueze, O, Cotter, G, Mbarubucyeye, J. Damascene, Dmytriiev, A, Doroshenko, V, Egberts, K, Einecke, S, Ernenwein, J. -P, Füßling, M, Funk, S, Gabici, S, Ghafourizadeh, S, Giavitto, G, Glombitza, J, Goswami, P, Hinton, J. A, Holler, M, Jamrozy, M, Joshi, V, Jung-Richardt, I, Kasai, E, Khatoon, R, Kh'elifi, B, niak, Kostunin, D, Lang, R. G, Leitl, F, Lemière, A, Lenain, J. -P, Leuschner, F, Luashvili, A, Marx, R, Mehta, A, Meyer, M, Mitchell, A, Moderski, R, Montanari, A, Moulin, E, de Naurois, M, Niemiec, J, O'Brien, P, Ohm, S, Olivera-Nieto, L, Wilhelmi, E. de Ona, Ostrowski, M, Panny, S, Parsons, R. D, Punch, M, Quirrenbach, A, Reichherzer, P, Reimer, A, Reimer, O, Rieger, F, Rudak, B, Sahakian, V, Salzmann, H, Sanchez, D. A, Sasaki, M, Schüssler, F, Schutte, H. M, Shapopi, J. N. S, Specovius, A, L, Steenkamp, R, Streil, K, Sushch, I, van Eldik, C, Vecchi, M, Veh, J, Wagner, S. J, Wierzcholska, A, Zdziarski, A. A, Zech, A, Zouari, S, Żywucka, N

“…Most $\gamma$-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to the…”
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The vanishing of the primary emission region in PKS 1510-089 by Aharonian, F, Benkhali, F. Ait, Aschersleben, J, Ashkar, H, Barnard, J, Berge, D, Bernloehr, K, Bi, B, de Lavergne, M. de Bony, Boettcher, M, Bolmont, J, Borowska, J, Bradascio, F, Brose, R, Brun, F, Bruno, B, Burger-Scheidlin, C, Caroff, S, Cerruti, M, Chand, T, Chen, A, Cotter, G, Davids, I. D, Dmytriiev, A, Doroshenko, V, Egberts, K, Einecke, S, Fegan, S, Fontaine, G, Gabici, S, Giavitto, G, Glawion, D, Glicenstein, J. F, Goswami, P, Grolleron, G, Haerer, L, Holch, T. L, Horns, D, Jamrozy, M, Jankowsky, F, Joshi, V, Jung-Richardt, I, Kasai, E, Katarzyski, K, Klu/'zniak, W, Komin, Nu, Kostunin, D, Lang, R. G, Leitl, F, Lenain, J. -P, Leuschner, F, Luashvili, A, Mackey, J, Marandon, V, Marchegiani, P, Marti-Devesa, G, Marx, R, Mehta, A, Meyer, M, Mitchell, A, Moderski, R, Mohrmann, L, Montanari, A, Niemiec, J, Ohm, S, Panter, M, Peron, G, Prokhorov, D. A, Punch, M, Quirrenbach, A, Reimer, O, Ren, H, Rieger, F, Rudak, B, Ricarte, H. Rueda, Sahakian, V, Salzmann, H, Santangelo, A, Sasaki, M, Schuessler, F, Schutte, H. M, Shapopi, J. N. S, Sol, H, Spencer, S, Stawarz, L, Steenkamp, R, Steppa, C, Sushch, I, Tanaka, T, van Eldik, C, van Soelen, B, Vecchi, M, Veh, J, Wach, T, Wierzcholska, A, Zacharias, M, Zargaryan, D, Zywucka, N, Buckley, D. A. H, Cooper, J

“…In July 2021, PKS 1510-089 exhibited a significant flux drop in the high-energy gamma-ray (by a factor 10) and optical (by a factor 5) bands and remained in…”
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Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations by Collaborations, Fermi-LAT, :, Aharonian, F, Backes, M, Martins, V. Barbosa, Becherini, Y, Berge, D, Bi, B, Bouyahiaoui, M, Breuhaus, M, Brose, R, Brun, F, Bruno, B, Bulik, T, Burger-Scheidlin, C, Bylund, T, Caroff, S, Chand, T, Chandra, S, Chen, A, Chibueze, J, de Bony, M, Egberts, K, Ernenwein, J. -P, de Clairfontaine, G. Fichet, Fontaine, G, Funk, S, Gabici, S, Ghafourizadeh, S, Giavitto, G, Glawion, D, Glicenstein, J. F, Goswami, P, Grondin, M. -H, Haerer, L, Holler, M, Horns, D, Jankowsky, F, Joshi, V, Jung-Richardt, I, Kasai, E, Katarzynński, K, Khélifi, B, Komin, Nu, Kosack, K, Kostunin, D, Lang, R. G, Leitl, F, Lemière, A, Lenain, J. -P, Lohse, T, Luashvili, A, Lypova, I, Mackey, J, Malyshev, D, Marandon, V, Martí-Devesa, G, Marx, R, Meyer, M, Mitchell, A, Moderski, R, Mohrmann, L, Moulin, E, Muller, J, Murach, T, Nakashima, K, Ohm, S, Olivera-Nieto, L, Wilhelmi, E. de Ona, Panter, M, Parsons, R. D, Peron, G, Prokhorov, D. A, Prokoph, H, Pühlhofer, G, Reichherzer, P, Reimer, A, Reimer, O, Reville, B, Rieger, F, Ruiz-Velasco, E, Sanchez, D. A, Sasaki, M, Schüussler, F, Schutte, H. M, Schwanke, U, Shapopi, J. N. S, Sol, H, Suzuki, H, Taylor, A. M, Terrier, R, Thorpe-Morgan, C, Uchiyama, Y, Veh, J, Wagner, S. J, White, R, Wierzcholska, A, Wong, Yu Wun, Zacharias, M, Zargaryan, D

“…ApJ Letters 2023, Volume 950, Number 2 950, L16 Magnetic fields in galaxies and galaxy clusters are believed to be the result of the amplification of…”
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A deep spectromorphological study of the $\gamma$-ray emission surrounding the young massive stellar cluster Westerlund 1 by Aharonian, F, Backes, M, Martins, V. Barbosa, Becherini, Y, Berge, D, Bradascio, F, Brose, R, Brun, F, Bulik, T, Cangemi, F, Caroff, S, Casanova, S, Chand, T, Chandra, S, Chibueze, O, Mbarubucyeye, J. Damascene, Feijen, K, Gabici, S, Gallant, Y. A, Ghafourizadeh, S, Giavitto, G, Giunti, L, Glawion, D, Goswami, P, Grondin, M. -H, Härer, L. K, Haupt, M, Hofmann, W, Holler, M, Horns, D, Jamrozy, M, Joshi, V, Jung-Richardt, I, Katarzyński, K, Khélifi, B, Kosack, K, Kostunin, D, Mezek, G. Kukec, Lang, R. G, Stum, S. Le, Lemière, A, Lemoine-Goumard, M, Lenain, J. -P, Leuschner, F, Lohse, T, Mackey, J, Majumdar, J, Malyshev, D, Marandon, V, Marcowith, A, Marx, R, Maurin, G, Mitchell, A, Mohrmann, L, Montanari, A, Moulin, E, Muller, J, Nakashima, K, de Naurois, M, Nayerhoda, A, Olivera-Nieto, L, Ostrowski, M, Panter, M, Parsons, R. D, Peron, G, Prokhorov, D. A, Pühlhofer, G, Punch, M, Quirrenbach, A, Rauth, R, Rieger, F, Rowell, G, Rudak, B, Sahakian, V, Salzmann, H, Sanchez, D. A, Sasaki, M, Schüssler, F, Schutte, H. M, Schwanke, U, Stawarz, Ł, Sushch, I, Tanaka, T, Tsuji, N, van Soelen, B, Veh, J, Vink, J, Wagner, S. J, White, R, Wierzcholska, A, Zacharias, M, Zargaryan, D, Zdziarski, A. A, Zhu, S. J, Żywucka, N, Blackwell, R, Braiding, C, Burton, M, Cubuk, K, Tothill, N

“…A&A 666, A124 (2022) Young massive stellar clusters are extreme environments and potentially provide the means for efficient particle acceleration. Indeed,…”
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