학술논문

Gamma-ray observations of MAXI J1820+070 during the 2018 outburst
Document Type
Working Paper
Author
Abe, H.Abe, S.Acciari, V. A.Aniello, T.Ansoldi, S.Antonelli, L. A.Engels, A. ArbetArcaro, C.Artero, M.Asano, K.Baack, D.Babić, A.Baquero, A.de Almeida, U. BarresBarrio, J. A.Batković, I.Baxter, J.González, J. BecerraBednarek, W.Bernardini, E.Bernardos, M.Berti, A.Besenrieder, J.Bhattacharyya, W.Bigongiari, C.Biland, A.Blanch, O.Bonnoli, G.Bošnjak, Ž.Burelli, I.Busetto, G.Carosi, R.Carretero-Castrillo, M.Ceribella, G.Chai, Y.Chilingarian, A.Cikota, S.Colombo, E.Contreras, J. L.Cortina, J.Covino, S.D'Amico, G.D'Elia, V.Da Vela, P.Dazzi, F.De Angelis, A.De Lotto, B.Del Popolo, A.Delfino, M.Delgado, J.Mendez, C. DelgadoDepaoli, D.Di Pierro, F.Di Venere, L.Prester, D. DominisDonini, A.Dorner, D.Doro, M.Elsaesser, D.Emery, G.Ramazani, V. FallahFariña, L.Fattorini, A.Font, L.Fruck, C.Fukami, S.Fukazawa, Y.López, R. J. GarcíaGarczarczyk, M.Gasparyan, S.Gaug, M.Paiva, J. G. GiesbrechtGiglietto, N.Giordano, F.Gliwny, P.Godinović, N.Grau, R.Green, D.Green, J. G.Hadasch, D.Hahn, A.Hassan, T.Heckmann, L.Herrera, J.Hoang, J.Hrupec, D.Hütten, M.Imazawa, R.Inada, T.Iotov, R.Ishio, K.Martínez, I. JiménezJormanainen, J.Kerszberg, D.Kobayashi, Y.Kubo, H.Kushida, J.Lamastra, A.Lelas, D.Leone, F.Lindfors, E.Linhoff, L.Lombardi, S.Longo, F.López-Coto, R.López-Moya, M.López-Oramas, A.Loporchio, S.Lorini, A.Lyard, E.Fraga, B. Machado de OliveiraMajumdar, P.Makariev, M.Maneva, G.Mang, N.Manganaro, M.Mangano, S.Mannheim, K.Mariotti, M.Martínez, M.Aguilar, A. MasMazin, D.Menchiari, S.Mender, S.Mićanović, S.Miceli, D.Miener, T.Miranda, J. M.Mirzoyan, R.Molina, E.Mondal, H. A.Moralejo, A.Morcuende, D.Moreno, V.Nakamori, T.Nanci, C.Nava, L.Neustroev, V.Rosillo, M. NievasNigro, C.Nilsson, K.Nishijima, K.Ekoume, T. NjohNoda, K.Nozaki, S.Ohtani, Y.Oka, T.Okumura, A.Otero-Santos, J.Paiano, S.Palatiello, M.Paneque, D.Paoletti, R.Paredes, J. M.Pavletić, L.Persic, M.Pihet, M.Pirola, G.Podobnik, F.Moroni, P. G. PradaPrandini, E.Principe, G.Priyadarshi, C.Puljak, I.Rhode, W.Ribó, M.Rico, J.Righi, C.Rugliancich, A.Sahakyan, N.Saito, T.Sakurai, S.Satalecka, K.Saturni, F. G.Schleicher, B.Schmidt, K.Schmuckermaier, F.Schubert, J. L.Schweizer, T.Sitarek, J.Sliusar, V.Sobczynska, D.Spolon, A.Stamerra, A.Strišković, J.Strom, D.Strzys, M.Suda, Y.Surić, T.Tajima, H.Takahashi, M.Takeishi, R.Tavecchio, F.Temnikov, P.Terauchi, K.Terzić, T.Teshima, M.Tosti, L.Truzzi, S.Tutone, A.Ubach, S.van Scherpenberg, J.Acosta, M. VazquezVentura, S.Verguilov, V.Viale, I.Vigorito, C. F.Vitale, V.Vovk, I.Walter, R.Will, M.Wunderlich, C.Yamamoto, T.Zarić, D.Abdalla, H.Aharonian, F.Benkhali, F. AitAngüner, E. O.Ashkar, H.Backes, M.Baghmanyan, V.Martins, V. BarbosaBatzofin, R.Becherini, Y.Berge, D.Bernlöhr, K.Böttcher, M.Boisson, C.Bolmont, J.de Lavergne, M. de BonyBradascio, F.Breuhaus, M.Brose, R.Brun, F.Bulik, T.Bylund, T.Cangemi, F.Caroff, S.Casanova, S.Cerruti, M.Chand, T.Chandra, S.Chen, A.Chibueze, O. U.Cotter, G.Cristofari, P.Mbarubucyeye, J. DamasceneDevin, J.Djannati-Ataï, A.Dmytriiev, A.Egberts, K.Ernenwein, J. -P.Fiasson, A.de Clairfontaine, G. FichetFontaine, G.Füßling, M.Funk, S.Gabici, S.Ghafourizadeh, S.Giavitto, G.Glawion, D.Glicenstein, J. F.Goswami, P.Grolleron, G.Hinton, J. A.Hörbe, M.Hoischen, C.Holch, T. L.Holler, M.Horns, D.Huang, ZhiqiuJamrozy, M.Jankowsky, F.Joshi, V.Jung-Richardt, I.Kasai, E.Katarzyński, K.Katz, U.Khélifi, B.Kluźniak, W.Komin, Nu.Kosack, K.Kostunin, D.Lang, R. G.Stum, S. LeLemière, A.Lemoine-Goumard, M.Lenain, J. -P.Leuschner, F.Lohse, T.Luashvili, A.Lypova, I.Mackey, J.Majumdar, J.Malyshev, D.Marandon, V.Marchegiani, P.Martí-Devesa, G.Marx, R.Maurin, G.Meyer, M.Mitchell, A.Moderski, R.Mohrmann, L.Montanari, A.Moulin, E.Muller, J.Murach, T.Nakashima, K.de Naurois, M.Nayerhoda, A.Niemiec, J.Noel, A. PriyanaO'Brien, P.Ohm, S.Olivera-Nieto, L.Wilhelmi, E. de OnaOstrowski, M.Panny, S.Panter, M.Parsons, R. D.Poireau, V.Prokhorov, D. A.Prokoph, H.Pühlhofer, G.Punch, M.Quirrenbach, A.Reichherzer, P.Reimer, A.Reimer, O.Renaud, M.Rieger, F.Rowell, G.Rudak, B.Ricarte, H. RuedaRuiz-Velasco, E.Sahakian, V.Salzmann, H.Santangelo, A.Sasaki, M.Schäfer, J.Schüssler, F.Schutte, H. M.Schwanke, U.Shapopi, J. N. S.Sol, H.Specovius, A.Spencer, S.Stawarz, Ł.Steenkamp, R.Steinmassl, S.Steppa, C.Sushch, I.Suzuki, H.Takahashi, T.Tanaka, T.Thorpe-Morgan, C.Tluczykont, M.Tomankova, L.Tsuji, N.Uchiyama, Y.van Eldik, C.van Soelen, B.Vecchi, M.Veh, J.Venter, C.Vink, J.Wagner, S. J.White, R.Wierzcholska, A.Wong, Yu WunYusafzai, A.Zacharias, M.Zanin, R.Zargaryan, D.Zdziarski, A. A.Zech, A.Zhu, S. J.Zouari, S.Żywucka, N.Acharyya, A.Adams, C. B.Batista, P.Benbow, W.Capasso, M.Christiansen, J. L.Chromey, A. J.Errando, M.Falcone, A.Feng, Q.Finley, J. P.Foote, G. MFortson, L.Furniss, A.Gent, A.Hanlon, W. FHervet, O.Holder, J.Hona, B.Humensky, T. B.Jin, W.Kaaret, P.Kertzman, M.Kherlakian, M.Kleiner, T. K.Kumar, S.Lang, M. J.Lundy, M.Maier, G.McGrath, C. E.Millis, J.Moriarty, P.Mukherjee, R.O'Brien, S.Ong, R. A.Park, N.Patel, S. R.Pfrang, K.Pohl, M.Pueschel, E.Quinn, J.Ragan, K.Reynolds, P. T.Ribeiro, D.Roache, E.Ryan, J. L.Sadeh, I.Saha, L.Santander, M.Sembroski, G. H.Shang, R.Splettstoesser, M.Tak, D.Tucci, J. V.Weinstein, A.Williams, D. A.Williamson, T. J.Bosch-Ramon, V.Celma, C.Linares, M.Russell, D. M.Sala, G.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
MAXI J1820+070 is a low-mass X-ray binary with a black hole as a compact object. This binary underwent an exceptionally bright X-ray outburst from March to October 2018, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 hours of observations of the MAXI J1820+070 outburst with the H.E.S.S., MAGIC and VERITAS experiments at energies above 200 GeV are presented, together with Fermi-LAT data between 0.1 and 500 GeV, and multiwavelength observations from radio to X-rays. Gamma-ray emission is not detected from MAXI J1820+070, but the obtained upper limits and the multiwavelength data allow us to put meaningful constraints on the source properties under reasonable assumptions regarding the non-thermal particle population and the jet synchrotron spectrum. In particular, it is possible to show that, if a high-energy gamma-ray emitting region is present during the hard state of the source, its predicted flux should be at most a factor of 20 below the obtained Fermi-LAT upper limits, and closer to them for magnetic fields significantly below equipartition. During the state transitions, under the plausible assumption that electrons are accelerated up to ~ 500 GeV, the multiwavelength data and the gamma-ray upper limits lead consistently to the conclusion that a potential high-energy and very-high-energy gamma-ray emitting region should be located at a distance from the black hole ranging between 10^11 and 10^13 cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA.
Comment: 15 pages, 5 figures. Accepted for publication in MNRAS