Autor: Roellinghoff, G. - Prolib Integro

Skocz do pozycji: 1.

Tytuł:: Unveiling extended gamma-ray emission around HESS J1813-178
Autorzy:: Holler, M.
Funk, S.
Renaud, M.
Cecil, R.
Reville, B.
Barnard, J.
Zargaryan, D.
Komin, Nu.
Bulik, T.
Cerruti, M.
Gallant, Y. A.
Noel, Angel
Reimer, A.
Fontaine, G.
Chen, A.
Steenkamp, R.
Mehta, A.
Gabici, S.
Kluźniak, W.
Kostunin, D.
Montanari, A.
Żywucka, N.
Venter, C.
Bi, B.
Lenain, J.-P.
Lemoine-Goumard, M.
Moulin, E.
de Naurois, M.
Leuschner, F.
Wach, T.
Aschersleben, J.
Sushch, I.
Malyshev, D.
Veh, J.
Steinmassl, S.
Suzuki, H.
Goswami, P.
Böttcher, M.
Chand, T.
Giavitto, G.
Einecke, S.
de Ona Wilhelmi, E.
Joshi, V.
Barbosa Martins, V.
Khélifi, B.
Wierzcholska, A.
Ghafourizadeh, S.
Batzofin, R.
Damascene Mbarubucyeye, J.
Moderski, R.
O’Brien, P.
Brose, R.
Bouyahiaoui, M.
Baktash, A.
Jamrozy, Marek
Murach, T.
Specovius, A.
Tsuji, N.
Ohm, S.
Bernlöhr, K.
Becherini, Y.
Leitl, F.
Regeard, M.
Doroshenko, V.
Chibueze, O.
Le Stum, S.
Kosack, K.
Spencer, S.
Holch, T. L.
Takahashi, T.
Berge, D.
Wagner, S. J.
Ren, H.
Marx, R.
Borowska, J.
Ashkar, H.
Parsons, R. D.
Punch, M.
Boisson, C.
Kundu, A.
Roellinghoff, G.
Zacharias, M.
Djannati-Ataï, A.
Niemiec, J.
Mitchell, A.
Panter, M.
Salzmann, H.
Olivera-Nieto, L.
Rudak, B.
Glawion, D.
Hofmann, W.
Marinos, P.
Panny, S.
Füßling, M.
Brun, F.
Cotter, G.
Filipovic, M.
Marandon, V.
Chambery, P.
Breuhaus, M.
Mackey, J.
de Bony de Lavergne, M.
Tanaka, T.
Katarzyński, K.
Zouari, S.
Dmytriiev, A.
Shapopi, J. N. S.
Aharonian, F.
van Eldik, C.
Chibueze, J.
Burger-Scheidlin, C.
Glicenstein, J. F.
Terrier, R.
Feijen, K.
Bolmont, J.
Sasaki, M.
Lang, R. G.
Reimer, O.
Steppa, C.
Lemière, A.
Unbehaun, T.
Reichherzer, P.
Bruno, B.
Ait Benkhali, F.
Sahakian, V.
Ernenwein, J.-P.
Hinton, J. A.
Grondin, M.-H.
Ostrowski, Michał
Vecchi, M.
Casanova, S.
Jung-Richardt, I.
Pühlhofer, G.
Quirrenbach, A.
Prokhorov, D. A.
Backes, M.
Schüssler, F.
Schutte, H. M.
Zdziarski, A. A.
Tluczykont, M.
Grolleron, G.
Jankowsky, F.
Celic, J.
Vink, J.
Klepser, S.
Caroff, S.
Martí-Devesa, G.
Rieger, F.
Mohrmann, L.
Khatoon, R.
Opis:: Context. HESS J1813–178 is a very-high-energy γ-ray source spatially coincident with the young and energetic pulsar PSR J1813–1749 and thought to be associated with its pulsar wind nebula (PWN). Recently, evidence for extended high-energy emission in the vicinity of the pulsar has been revealed in the Fermi Large Area Telescope (LAT) data. This motivates revisiting the HESS J1813–178 region, taking advantage of improved analysis methods and an extended dataset. Aims. Using data taken by the High Energy Stereoscopic System (H.E.S.S.) experiment and the Fermi-LAT, we aim to describe the γ-ray emission in the region with a consistent model, to provide insights into its origin. Methods. We performed a likelihood-based analysis on 32 hours of H.E.S.S. data and 12 yr of Fermi-LAT data and we fitted a spectro-morphological model to the combined datasets. These results allowed us to develop a physical model for the origin of the observed γ-ray emission in the region. Results. In addition to the compact very-high-energy γ-ray emission centred on the pulsar, we find a significant yet previously undetected component along the Galactic plane. With Fermi-LAT data, we confirm extended high-energy emission consistent with the position and elongation of the extended emission observed with H.E.S.S. These results establish a consistent description of the emission in the region from GeV energies to several tens of TeV. Conclusions. This study suggests that HESS J1813–178 is associated with a γ-ray PWN powered by PSR J1813–1749. A possible origin of the extended emission component is inverse Compton emission from electrons and positrons that have escaped the confines of the pulsar and form a halo around the PWN.
Dostawca treści:: Repozytorium Uniwersytetu Jagiellońskiego

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Skocz do pozycji: 2.

Tytuł:: Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis
Autorzy:: Holler, M.
Funk, S.
Cristofari, P.
Renaud, M.
Cecil, R.
Reville, B.
Zargaryan, D.
Komin, Nu.
Bulik, T.
Harding, A.
Cerruti, M.
Gallant, Y. A.
Reimer, A.
Fontaine, G.
Chen, A.
Steenkamp, R.
Mehta, A.
Gabici, S.
Kluźniak, W.
Kostunin, D.
Montanari, A.
Żywucka, N.
Venter, C.
Bi, B.
Lenain, J.-P.
Lemoine-Goumard, M.
Moulin, E.
de Naurois, M.
Leuschner, F.
Wach, T.
Aschersleben, J.
Sushch, I.
Malyshev, D.
Veh, J.
Zech, A.
Glombitza, J.
Steinmassl, S.
Suzuki, H.
Goswami, P.
Böttcher, M.
Chand, T.
Giavitto, G.
Einecke, S.
de Ona Wilhelmi, E.
Joshi, V.
Barbosa Martins, V.
Khélifi, B.
Wierzcholska, A.
Batzofin, R.
Meyer, M.
Moderski, R.
O’Brien, P.
Brose, R.
Specovius, A.
Baktash, A.
Jamrozy, Marek
Murach, T.
Tsuji, N.
Devin, J.
Ohm, S.
Bernlöhr, K.
Becherini, Y.
Leitl, F.
Regeard, M.
Chibueze, O.
Chandra, S.
Le Stum, S.
Kosack, K.
Spencer, S.
Holch, T. L.
Takahashi, T.
Bylund, T.
Berge, D.
Wagner, S. J.
Ren, H.
Marx, R.
Borowska, J.
Ashkar, H.
Peron, G.
Parsons, R. D.
Punch, M.
Horns, D.
Boisson, C.
Kundu, A.
Roellinghoff, G.
Zacharias, M.
Bradascio, F.
Djannati-Ataï, A.
Niemiec, J.
Mitchell, A.
Panter, M.
Salzmann, H.
Kasai, E.
Olivera-Nieto, L.
Fegan, S.
Rudak, B.
Stawarz, Łukasz
Glawion, D.
Hofmann, W.
Marinos, P.
Panny, S.
Füßling, M.
Brun, F.
Cotter, G.
Marandon, V.
Chambery, P.
Breuhaus, M.
Mackey, J.
de Bony de Lavergne, M.
Luashvili, A.
Brown, A.
Tanaka, T.
Katarzyński, K.
Zouari, S.
Dmytriiev, A.
Shapopi, J. N. S.
Aharonian, F.
van Eldik, C.
Chibueze, J.
Burger-Scheidlin, C.
Glicenstein, J. F.
Terrier, R.
Feijen, K.
Bolmont, J.
Sasaki, M.
Lang, R. G.
Reimer, O.
Steppa, C.
Lemière, A.
Unbehaun, T.
Reichherzer, P.
Bruno, B.
Ait Benkhali, F.
Sahakian, V.
Streil, K.
Ernenwein, J.-P.
Hinton, J. A.
Grondin, M.-H.
Ostrowski, Michał
Vecchi, M.
Casanova, S.
Pühlhofer, G.
Quirrenbach, A.
Prokhorov, D. A.
Backes, M.
Schüssler, F.
Schutte, H. M.
Zdziarski, A. A.
Tluczykont, M.
Grolleron, G.
Jankowsky, F.
Celic, J.
Vink, J.
Caroff, S.
Martí-Devesa, G.
Rieger, F.
Haerer, L.
Djuvsland, J.
Filipović, M.
Mohrmann, L.
Khatoon, R.
Opis:: The Crab Nebula is a unique laboratory for studying the acceleration of electrons and positrons through their non-thermal radiation. Observations of very-high-energy γ rays from the Crab Nebula have provided important constraints for modelling its broadband emission. We present the first fully self-consistent analysis of the Crab Nebula’s γ-ray emission between 1 GeV and ∼100 TeV, that is, over five orders of magnitude in energy. Using the open-source software package GAMMAPY, we combined 11.4 yr of data from the Fermi Large Area Telescope and 80 h of High Energy Stereoscopic System (H.E.S.S.) data at the event level and provide a measurement of the spatial extension of the nebula and its energy spectrum. We find evidence for a shrinking of the nebula with increasing γ-ray energy. Furthermore, we fitted several phenomenological models to the measured data, finding that none of them can fully describe the spatial extension and the spectral energy distribution at the same time. Especially the extension measured at TeV energies appears too large when compared to the X-ray emission. Our measurements probe the structure of the magnetic field between the pulsar wind termination shock and the dust torus, and we conclude that the magnetic field strength decreases with increasing distance from the pulsar. We complement our study with a careful assessment of systematic uncertainties.
Dostawca treści:: Repozytorium Uniwersytetu Jagiellońskiego

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Skocz do pozycji: 3.

Tytuł:: Broadband multi-wavelength properties of M87 during the 2018 EHT campaign including a very high energy flaring episode
Autorzy:: Nickel, L.
Vos, J.
Errando, M.
Niinuma, K.
Maldera, S.
Saturni, F. G.
Satapathy, K.
Brissenden, R.
Impellizzeri, C. M. V.
Issaoun, S.
Kubo, H.
Roache, E.
Moriyama, K.
Berenji, B.
Georgiev, B.
Patel, N.
Lindfors, E.
Kaaret, P.
Foote, J.
Leone, F.
Ceribella, G.
Hadasch, D.
Johnson, M. D.
Hahn, A.
Kluźniak, W.
Negro, M.
Godinović, N.
Okumura, A.
Kim, D.-J.
Barres de Almeida, U.
Chan, C.-k.
Biland, A.
Moran, J. M.
Abhishek, A.
Green, D.
Silvestri, G.
de Naurois, M.
Weintroub, J.
Takahashi, M.
Wach, T.
Honma, M.
Mizuno, T.
Zech, A.
Eatough, R. P.
Stamerra, A.
Mereu, I.
Paredes, J. M.
Suson, D. J.
Lombardi, S.
Inoue, M.
Einecke, S.
Nigro, C.
Ryan, J. L.
Chang, D. O.
Nishijima, K.
Millard, M. J.
Jannuzi, B. T.
McGrath, C. E.
Ward-Thompson, D.
Kramer, M.
Roelofs, F.
Gradetzke, T.
Liu, X.
Santangelo, A.
Kettenis, M.
Brose, R.
Fukami, S.
Doro, M.
Hirota, T.
Matthews, L. D.
Ohm, S.
Fröse, S.
Chen, Y.
Liuzzo, E.
Marchili, N.
Ricarte, A.
Duerr, A.
Ravikularaman, S.
Sánchez-Conde, M.
Huang, Zhiqiu
Shao, L.
Font, L.
Lo, W.-P.
Chatterjee, S.
Grenier, I. A.
Antonelli, L. A.
Giordano, F.
Leitl, F.
Rani, B.
Di Pierro, F.
Colombo, E.
Neilsen, J.
Kosack, K.
Holch, T. L.
Navarro Fuentes, S.
Nanci, C.
Haggard, D.
Berge, D.
Wagner, S. J.
Kravchenko, E. V.
Tavecchio, F.
Ramakrishnan, V.
Li, G.
Tsirou, M.
Schloerb, F. P.
Rottmann, H.
Caraveo, P. A.
Boisson, C.
Miener, T.
Toma, K.
Holder, J.
Sgrò, C.
Bradascio, F.
Grau, R.
Bach, U.
Aguasca-Cabot, A.
Kasai, E.
Barrio, J. A.
Contreras, J. L.
Jiménez-Rosales, A.
Fraga-Encinas, R.
Savolainen, T.
Gargano, F.
Bonino, R.
Panny, S.
Arbet Engels, A.
Narayanan, G.
Cotter, G.
Kramer, J. A.
Mizuno, Y.
O’Brien, S.
Nilsson, K.
Mackey, J.
Bautista, A.
Berti, A.
de Bony de Lavergne, M.
Tanaka, T.
Brown, A.
Germani, S.
Cui, Y.-Z.
Benson, B. A.
Falcone, A. D.
Babić, A.
Cerasole, D.
Fariña, L.
Zhao, R.
Lang, R. G.
Özel, F.
Kim, J.
Vassiliev, V. V.
Lamastra, A.
Ball, D.
Chen, M.-T.
Johnson, M. N.
Humensky, T. B.
Ernenwein, J.-P.
Kushida, J.
Nakamura, M.
Prada Moroni, P. G.
Santander, M.
Dazzi, F.
Paoletti, R.
La Bella, N.
Sohn, B. W.
Fuentes, A.
Celic, J.
Terauchi, K.
Myserlis, I.
Stanway, J. S.
Bronzwaer, T.
Cho, I.
Torres, D. F.
Ro, H.
Barrett, J.
Elsaesser, D.
Blanch, O.
Wielgus, M.
Sitarek, J.
Djuvsland, J.
Sánchez-Portal, M.
Khatoon, R.
Funk, S.
Loparco, F.
Reville, B.
Majumdar, P.
Otero-Santos, J.
Chatterjee, K.
Natarajan, I.
Hinrichs, C. E.
Zhao, G.-Y.
Torne, P.
Gaug, M.
Omodei, N.
Castro-Tirado, A. J.
Baloković, M.
Cerruti, M.
Mondal, H. A.
Bruel, P.
Pensec, U.
Ohtani, Y.
lackburn, L.
Tiede, P.
Park, J.
Kramer, C.
Hesper, R.
Mus, A.
Davelaar, J.
Machado de Oliveira Fraga, B.
Pirola, G.
Liu, J.
Ford, N. M.
Ford, H. A.
Small, D.
Dihingia, I. K.
De Lotto, B.
Kumar, S.
Nagai, H.
Kerszberg, D.
Nievas Rosillo, M.
Tazaki, F.
Martí-Vidal, I.
Persic, M.
Saz Parkinson, P. M.
Gasbarra, C.
Splettstoesser, M.
Kobayashi, Y.
Tetarenko, A. J.
Leuschner, F.
Aschersleben, J.
Tutone, A.
Malyshev, D.
Schäfer, J.
De Laurentis, M.
Nikolić, L.
Yamaguchi, P.
Righi, C.
Suzuki, H.
Goswami, P.
Furniss, A.
Keating, G. K.
Prather, B.
Di Tria, R.
Wong, G. N.
Porth, O.
de Ona Wilhelmi, E.
Maneva, G.
Chen, Z.
Baczko, A.-K.
Mariotti, M.
Strzys, M.
Barbosa Martins, V.
Oh, J.
Zensus, J. A.
Krichbaum, T. P.
Wierzcholska, A.
Li, B.
Principe, G.
D’Elia, V.
Batzofin, R.
Sharma, A.
Gold, R.
Yadlapalli, N.
Longo, F.
Manganaro, M.
Bauböck, M.
Kleiner, T. K.
Lovellette, M. N.
Giesbrecht Paiva, J. G.
Kocherlakota, P.
Schmuckermaier, F.
Becherini, Y.
Boyce, H.
Mazziotta, M. N.
Fomalont, E.
Fukazawa, Y.
Martínez, M.
Lobanov, A. P.
Krennrich, F.
Suutarinen, S.
Conway, J. E.
Verna, G.
Bouman, K. L.
Lindqvist, M.
Farah, J.
Le Stum, S.
Xia, B.
Zhang, H.
Carretero-Castrillo, M.
Reis, I.
Herrera Llorente, J.
Menchiari, S.
Sun, H.
Takahashi, T.
Moscibrodzka, M.
Kuss, M.
Anantua, R.
Marx, R.
Psaltis, D.
Borowska, J.
Yan, H.
Morselli, A.
Ashkar, H.
Podobnik, F.
Valverde, J.
Trippe, S.
Lonsdale, C. J.
Zhao, S.-S.
Cavazzuti, E.
Mitchell, A.
Panter, M.
Salzmann, H.
Foschi, M.
Jeter, B.
Stawarz, Łukasz
Busetto, G.
Toscano, T.
Sheridan, C.
Gómez-Ruiz, A. I.
Hassan, T.
D’Amico, G.
Jorstad, S.
Li, Z.
Yuan, Y.-F.
Olivares, H.
PopStefanija, A.
Schonfeld, J.
Katarzyński, K.
van Eldik, C.
Yfantis, A.
López-Moya, M.
Mazin, D.
Carosi, R.
Cheong, W.-Y.
Wang, N.
Takeishi, R.
Domínguez, A.
Dominis Prester, D.
Artero, M.
García, R.
Sahakian, V.
Müller, C.
Streil, K.
López-Coto, R.
Hanlon, W.
Roshanineshat, A.
Aniello, T.
Vazquez Acosta, M.
Dexter, J.
Matsushita, S.
Njoh Ekoume, T.
Dinesh, A.
Jung-Richardt, I.
Tilanus, R. P. J.
Burelli, I.
Emami, R.
Shapopi, J. N. S.
Yu, W.
Dorner, D.
Jiménez Martínez, I.
Sciaccaluga, A.
Schüssler, F.
Vovk, I.
Sakai, N.
Arcaro, C.
Grolleron, G.
Lang, M. J.
Dempsey, J.
Heckmann, L.
Kertzman, M.
Washington, J. E.
Martí-Devesa, G.
Sánchez, S.
Ikeda, S.
Marrone, D. P.
Yuan, F.
Lisakov, M.
MacDonald, N. R.
Sol, H.
Di Lalla, N.
Molero González, M.
Blandford, R. D.
Mizuno, I.
Garczarczyk, M.
Musoke, G.
Holler, M.
Pesce, D. W.
Orlando, E.
Hays, E.
Cecil, R.
Algaba, J. C.
Pen, U.-L.
Lowitz, A. E.
Cristarella Orestano, P.
Hrupec, D.
Fromm, C. M.
Azulay, R.
Conroy, N. S.
Koch, P. M.
Alberdi, A.
Roy, A. L.
Pihet, M.
Moralejo, A.
Young, A.
Da Vela, P.
Batković, I.
Gu, M.
Markoff, S.
Fontaine, G.
Titus, M.
Kuo, C.-Y.
Michail, J.
Chen, A.
Wiik, K.
Neustroev, V.
Lico, R.
Montanari, A.
Sembroski, G. H.
Besenrieder, J.
Desvignes, G.
Lenain, J.-P.
Moulin, E.
Kofuji, Y.
Carosi, A.
Moriarty, P.
Miranda, J. M.
van Langevelde, H. J.
Abe, S.
van Rossum, D. R.
Böttcher, M.
Ruszczyk, C.
Covino, S.
Bower, G. C.
Ripperda, B.
Ong, R. A.
Priyadarshi, C.
Tucci, J. V.
Temnikov, P.
Meyer, M.
Blundell, R.
Koay, J. Y.
Di Venere, L.
Damascene Mbarubucyeye, J.
Moderski, R.
O’Brien, P.
Mannheim, K.
Jones, A. C.
Doeleman, S. S.
Cortina, J.
Turk, M.
Makariev, M.
Huang, C.-W. L.
Prandini, E.
Pohl, M.
Wu, Q.
Heumann, D.
Reynolds, P. T.
Freeman, W. T.
Raymond, A. W.
Franckowiak, A.
Truzzi, S.
Monzani, M. E.
Loinard, L.
Friberg, P.
Giliberti, M.
Mao, J.
Jormanainen, J.
James, D. J.
Molina, E.
Abhir, J.
Gentaz, O.
Okino, H.
Rao, R.
Ribeiro, D.
Crawford, T. M.
Gómez, J. L.
Chael, A.
Deane, R.
Lyard, E.
van Scherpenberg, J.
Sadeh, I.
Ciprini, S.
Maier, G.
Imazawa, R.
Mas-Aguilar, A.
Pita, S.
Liu, Z.
Ubach, S.
Donini, A.
Savchenko, S. S.
Dhruv, V.
Schmidt, K.
Cifuentes, A.
Kundu, A.
Palumbo, D. C. M.
Green, J. G.
Zacharias, M.
Lundy, M.
Sasada, M.
Niemiec, J.
Kawashima, T.
Bonnoli, G.
Acciari, V. A.
Filippos Paraschos, G.
Günther, P.
Will, M.
Glawion, D.
Cutini, S.
Peresano, M.
Feng, Q.
Chai, Y.
Traianou, E.
Hada, K.
Luashvili, A.
Ishio, K.
Sahakyan, N.
Quinn, J.
Paneque, D.
Kerby, S.
Kieda, D.
Saha, L.
Adams, C. B.
Glicenstein, J. F.
Gammie, C. F.
Acharyya, A.
Broguiere, D.
Wajima, K.
Lu, R.-S.
Sasaki, M.
Delfino, M.
Carlstrom, J. E.
Reimer, O.
Steppa, C.
Sosapanta Salas, L. D.
Lemière, A.
Bruno, B.
Bigongiari, C.
Marscher, A. P.
Giroletti, M.
Fortson, L.
Ros, E.
Cameron, R. A.
Ostrowski, Michał
Taylor, A. M.
Vecchi, M.
Lindahl, G.
Jung, T.
Koyama, S.
Casanova, S.
Baxter, J.
Schweizer, T.
Nowak, M. A.
Martínez-Chicharro, M.
Quirrenbach, A.
Foffano, L.
Witzel, G.
Britzen, S.
Fegan, S. J.
Ruiz, I.
Backes, M.
Bošnjak, Ž.
De Angelis, A.
Yamamoto, T.
Schutte, H. M.
Liu, K.
Miceli, D.
Menten, K. M.
Christian, P.
Zhong, W.
Campoy-Ordaz, A.
Terzić, T.
Ragan, K.
Joshi, A. V.
Giglietto, N.
D’Ammando, F.
Fattorini, A.
Walter, R.
Haerer, L.
Teshima, M.
Bandyopadhyay, B.
Bednarek, W.
Agudo, I.
Gurwell, M. A.
Ma, J.
Falcke, H.
de Menezes, R.
Shang, R.
Moghadam, M. O.
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Loporchio, S.
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Mirabal, N.
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Parsons, H.
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Vitale, V.
Wong, S. L.
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López-Oramas, A.
Zdziarski, A. A.
Wharton, R.
Tluczykont, M.
Wondrak, M. F.
Jankowsky, F.
Horan, D.
Zhang, S.
Delgado Mendez, C.
Hervet, O.
Janssen, M.
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Schubert, J. L.
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Wang, J.
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Jiang, W.
Opis:: Context. The nearby elliptical galaxy M87 contains one of only two supermassive black holes whose emission surrounding the event horizon has been imaged by the Event Horizon Telescope (EHT). In 2018, more than two dozen multi-wavelength (MWL) facilities (from radio to γ-ray energies) took part in the second M87 EHT campaign. Aims. The goal of this extensive MWL campaign was to better understand the physics of the accreting black hole M87*, the relationship between the inflow and inner jets, and the high-energy particle acceleration. Understanding the complex astrophysics is also a necessary first step towards performing further tests of general relativity. Methods. The MWL campaign took place in April 2018, overlapping with the EHT M87* observations. We present a new, contemporaneous spectral energy distribution (SED) ranging from radio to very high-energy (VHE) γ-rays as well as details of the individual observations and light curves. We also conducted phenomenological modelling to investigate the basic source properties. Results. We present the first VHE γ-ray flare from M87 detected since 2010. The flux above 350 GeV more than doubled within a period of ≈36 hours. We find that the X-ray flux is enhanced by about a factor of two compared to 2017, while the radio and millimetre core fluxes are consistent between 2017 and 2018. We detect evidence for a monotonically increasing jet position angle that corresponds to variations in the bright spot of the EHT image. Conclusions. Our results show the value of continued MWL monitoring together with precision imaging for addressing the origins of high-energy particle acceleration. While we cannot currently pinpoint the precise location where such acceleration takes place, the new VHE γ-ray flare already presents a challenge to simple one-zone leptonic emission model approaches, and it emphasises the need for combined image and spectral modelling.
Dostawca treści:: Repozytorium Uniwersytetu Jagiellońskiego

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