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Start Over Author "Abe, S" Journal monthly notices of the royal astronomical society
4 results on '"Abe, S"'

1. Performance and first measurements of the MAGIC stellar intensity interferometer

Author

Abe, S, primary, Abhir, J, additional, Acciari, V A, additional, Aguasca-Cabot, A, additional, Agudo, I, additional, Aniello, T, additional, Ansoldi, S, additional, Antonelli, L A, additional, Arbet Engels, A, additional, Arcaro, C, additional, Artero, M, additional, Asano, K, additional, Babić, A, additional, Baquero, A, additional, de Almeida, U Barres, additional, Barrio, J A, additional, Batković, I, additional, Bautista, A, additional, Baxter, J, additional, González, J Becerra, additional, Bernardini, E, additional, Bernardos, M, additional, Bernete, J, additional, Berti, A, additional, Besenrieder, J, additional, Bigongiari, C, additional, Biland, A, additional, Blanch, O, additional, Bonnoli, G, additional, Bošnjak, Ž, additional, Burelli, I, additional, Busetto, G, additional, Campoy-Ordaz, A, additional, Carosi, A, additional, Carosi, R, additional, Carretero-Castrillo, M, additional, Ceribella, G, additional, Chai, Y, additional, Cifuentes, A, additional, Colombo, E, additional, Contreras, J L, additional, Cortina, J, additional, Covino, S, additional, D’Amico, G, additional, D’Elia, V, additional, Da Vela, P, additional, Dazzi, F, additional, De Angelis, A, additional, De Lotto, B, additional, de Menezes, R, additional, Del Popolo, A, additional, Delfino, M, additional, Delgado, J, additional, Mendez, C Delgado, additional, Pierro, F Di, additional, Venere, L Di, additional, Prester, D Dominis, additional, Donini, A, additional, Dorner, D, additional, Doro, M, additional, Elsaesser, D, additional, Emery, G, additional, Escudero, J, additional, Fariña, L, additional, Fattorini, A, additional, Foffano, L, additional, Font, L, additional, Fröse, S, additional, Fukami, S, additional, Fukazawa, Y, additional, López, R J García, additional, Garczarczyk, M, additional, Gasparyan, S, additional, Gaug, M, additional, Paiva, J G Giesbrecht, additional, Giglietto, N, additional, Giordano, F, additional, Gliwny, P, additional, Gradetzke, T, additional, Grau, R, additional, Green, D, additional, Green, J G, additional, Günther, P, additional, Hadasch, D, additional, Hahn, A, additional, Hassan, T, additional, Heckmann, L, additional, Herrera, J, additional, Hrupec, D, additional, Hütten, M, additional, Imazawa, R, additional, Ishio, K, additional, Jiménez Martínez, I, additional, Jormanainen, J, additional, Kayanoki, T, additional, Kerszberg, D, additional, Kluge, G W, additional, Kobayashi, Y, additional, Kouch, P M, additional, Kubo, H, additional, Kushida, J, additional, Láinez, M, additional, Lamastra, A, additional, Leone, F, additional, Lindfors, E, additional, Linhoff, L, additional, Lombardi, S, additional, Longo, F, additional, López-Coto, R, additional, López-Moya, M, additional, López-Oramas, A, additional, Loporchio, S, additional, Lorini, A, additional, Lyard, E, additional, Fraga, B Machado de Oliveira, additional, Majumdar, P, additional, Makariev, M, additional, Maneva, G, additional, Mang, N, additional, Manganaro, M, additional, Mangano, S, additional, Mannheim, K, additional, Mariotti, M, additional, Martínez, M, additional, Martínez-Chicharro, M, additional, Mas-Aguilar, A, additional, Mazin, D, additional, Menchiari, S, additional, Mender, S, additional, Miceli, D, additional, Miener, T, additional, Miranda, J M, additional, Mirzoyan, R, additional, González, M Molero, additional, Molina, E, additional, Mondal, H A, additional, Moralejo, A, additional, Morcuende, D, additional, Nakamori, T, additional, Nanci, C, additional, Neustroev, V, additional, Nickel, L, additional, Rosillo, M Nievas, additional, Nigro, C, additional, Nikolić, L, additional, Nilsson, K, additional, Nishijima, K, additional, Ekoume, T Njoh, additional, Noda, K, additional, Nozaki, S, additional, Ohtani, Y, additional, Okumura, A, additional, Otero-Santos, J, additional, Paiano, S, additional, Palatiello, M, additional, Paneque, D, additional, Paoletti, R, additional, Paredes, J M, additional, Peresano, M, additional, Persic, M, additional, Pihet, M, additional, Pirola, G, additional, Podobnik, F, additional, Moroni, P G Prada, additional, Prandini, E, additional, Principe, G, additional, Priyadarshi, C, additional, Rhode, W, additional, Ribó, M, additional, Rico, J, additional, Righi, C, additional, Sahakyan, N, additional, Saito, T, additional, Satalecka, K, additional, Saturni, F G, additional, Schleicher, B, additional, Schmidt, K, additional, Schmuckermaier, F, additional, Schubert, J L, additional, Schweizer, T, additional, Sciaccaluga, A, additional, Silvestri, G, additional, Sitarek, J, additional, Sliusar, V, additional, Sobczynska, D, additional, Spolon, A, additional, Stamerra, A, additional, Strišković, J, additional, Strom, D, additional, Strzys, M, additional, Suda, Y, additional, Surić, T, additional, Suutarinen, S, additional, Tajima, H, additional, Takahashi, M, additional, Takeishi, R, additional, Temnikov, P, additional, Terauchi, K, additional, Terzić, T, additional, Teshima, M, additional, Truzzi, S, additional, Tutone, A, additional, Ubach, S, additional, van Scherpenberg, J, additional, Acosta, M Vazquez, additional, Ventura, S, additional, Viale, I, additional, Vigorito, C F, additional, Vitale, V, additional, Walter, R, additional, Will, M, additional, Wunderlich, C, additional, Yamamoto, T, additional, Chon, G, additional, Díaz, C, additional, Fiori, M, additional, Lobo, M, additional, Naletto, G, additional, Polo, M, additional, Rodríguez-Vázquez, J J, additional, Saha, P, additional, and Zampieri, L, additional

Published
2024
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2. MAGIC detection of GRB 201216C at z = 1.1

Author

Abe, H, primary, Abe, S, additional, Acciari, V A, additional, Agudo, I, additional, Aniello, T, additional, Ansoldi, S, additional, Antonelli, L A, additional, Engels, A Arbet, additional, Arcaro, C, additional, Artero, M, additional, Asano, K, additional, Baack, D, additional, Babić, A, additional, Baquero, A, additional, de Almeida, U Barres, additional, Barrio, J A, additional, Batković, I, additional, Baxter, J, additional, González, J Becerra, additional, Bednarek, W, additional, Bernardini, E, additional, Bernete, J, additional, Berti, A, additional, Besenrieder, J, additional, Bigongiari, C, additional, Biland, A, additional, Blanch, O, additional, Bonnoli, G, additional, Bošnjak, Ž, additional, Burelli, I, additional, Busetto, G, additional, Campoy-Ordaz, A, additional, Carosi, A, additional, Carosi, R, additional, Carretero-Castrillo, M, additional, Castro-Tirado, A J, additional, Ceribella, G, additional, Chai, Y, additional, Cifuentes, A, additional, Cikota, S, additional, Colombo, E, additional, Contreras, J L, additional, Cortina, J, additional, Covino, S, additional, D’Amico, G, additional, D’Elia, V, additional, Da Vela, P, additional, Dazzi, F, additional, De Angelis, A, additional, De Lotto, B, additional, Del Popolo, A, additional, Delfino, M, additional, Delgado, J, additional, Mendez, C Delgado, additional, Depaoli, D, additional, Di Pierro, F, additional, Di Venere, L, additional, Prester, D Dominis, additional, Donini, A, additional, Dorner, D, additional, Doro, M, additional, Elsaesser, D, additional, Emery, G, additional, Escudero, J, additional, Fari na, L, additional, Fattorini, A, additional, Foffano, L, additional, Font, L, additional, Fukami, S, additional, Fukazawa, Y, additional, López, R J García, additional, Garczarczyk, M, additional, Gasparyan, S, additional, Gaug, M, additional, Paiva, J G Giesbrecht, additional, Giglietto, N, additional, Giordano, F, additional, Gliwny, P, additional, Godinović, N, additional, Grau, R, additional, Green, D, additional, Green, J G, additional, Hadasch, D, additional, Hahn, A, additional, Hassan, T, additional, Heckmann, L, additional, Herrera, J, additional, Hrupec, D, additional, Hütten, M, additional, Imazawa, R, additional, Inada, T, additional, Iotov, R, additional, Ishio, K, additional, Martínez, I Jiménez, additional, Jormanainen, J, additional, Kerszberg, D, additional, Kluge, G W, additional, Kobayashi, Y, additional, Kouch, P M, additional, Kubo, H, additional, Kushida, J, additional, Lezáun, M Láinez, additional, Lamastra, A, additional, Leone, F, additional, Lindfors, E, additional, Linhoff, L, additional, Lombardi, S, additional, Longo, F, additional, López-Coto, R, additional, López-Moya, M, additional, López-Oramas, A, additional, Loporchio, S, additional, Lorini, A, additional, Lyard, E, additional, de Oliveira Fraga, B Machado, additional, Majumdar, P, additional, Makariev, M, additional, Maneva, G, additional, Mang, N, additional, Manganaro, M, additional, Mangano, S, additional, Mannheim, K, additional, Mariotti, M, additional, Martínez, M, additional, Mas-Aguilar, A, additional, Mazin, D, additional, Menchiari, S, additional, Mender, S, additional, Mićanović, S, additional, Miceli, D, additional, Miener, T, additional, Miranda, J M, additional, Mirzoyan, R, additional, González, M Molero, additional, Molina, E, additional, Mondal, H A, additional, Moralejo, A, additional, Morcuende, D, additional, Nanci, C, additional, Nava, L, additional, Neustroev, V, additional, Rosillo, M Nievas, additional, Nigro, C, additional, Nikolić, L, additional, Nilsson, K, additional, Nishijima, K, additional, Ekoume, T Njoh, additional, Noda, K, additional, Nozaki, S, additional, Ohtani, Y, additional, Okumura, A, additional, Otero-Santos, J, additional, Paiano, S, additional, Palatiello, M, additional, Paneque, D, additional, Paoletti, R, additional, Paredes, J M, additional, Pavletić, L, additional, Pavlović, D, additional, Persic, M, additional, Pihet, M, additional, Pirola, G, additional, Podobnik, F, additional, Moroni, P G Prada, additional, Prandini, E, additional, Principe, G, additional, Priyadarshi, C, additional, Rhode, W, additional, Ribó, M, additional, Rico, J, additional, Righi, C, additional, Sahakyan, N, additional, Saito, T, additional, Satalecka, K, additional, Saturni, F G, additional, Schleicher, B, additional, Schmidt, K, additional, Schmuckermaier, F, additional, Schubert, J L, additional, Schweizer, T, additional, Sciaccaluga, A, additional, Sitarek, J, additional, Sliusar, V, additional, Sobczynska, D, additional, Spolon, A, additional, Stamerra, A, additional, Strišković, J, additional, Strom, D, additional, Strzys, M, additional, Suda, Y, additional, Suutarinen, S, additional, Tajima, H, additional, Takahashi, M, additional, Takeishi, R, additional, Tavecchio, F, additional, Temnikov, P, additional, Terauchi, K, additional, Terzić, T, additional, Teshima, M, additional, Tosti, L, additional, Truzzi, S, additional, Tutone, A, additional, Ubach, S, additional, van Scherpenberg, J, additional, Acosta, M Vazquez, additional, Ventura, S, additional, Verguilov, V, additional, Viale, I, additional, Vigorito, C F, additional, Vitale, V, additional, Vovk, I, additional, Walter, R, additional, Will, M, additional, Yamamoto, T, additional, Gomboc, A, additional, Jordana-Mitjans, N, additional, Melandri, A, additional, Mundell, C G, additional, Shrestha, M, additional, and Steele, I A, additional

Published
2023
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3. MAGIC detection of GRB 201216C at z = 1.1.

Author

Abe, H, Abe, S, Acciari, V A, Agudo, I, Aniello, T, Ansoldi, S, Antonelli, L A, Engels, A Arbet, Arcaro, C, Artero, M, Asano, K, Baack, D, Babić, A, Baquero, A, de Almeida, U Barres, Barrio, J A, Batković, I, Baxter, J, González, J Becerra, and Bednarek, W

Subjects
*ELECTROMAGNETIC radiation, *ELECTROMAGNETIC waves, *GAMMA ray bursts, *COSMOLOGICAL distances, *ENERGY bands, *MAGIC
Abstract

Gamma-ray bursts (GRBs) are explosive transient events occurring at cosmological distances, releasing a large amount of energy as electromagnetic radiation over several energy bands. We report the detection of the long GRB 201216C by the MAGIC telescopes. The source is located at z  = 1.1 and thus it is the farthest one detected at very high energies. The emission above 70 GeV of GRB 201216C is modelled together with multiwavelength data within a synchrotron and synchrotron self-Compton (SSC) scenario. We find that SSC can explain the broad-band data well from the optical to the very-high-energy band. For the late-time radio data, a different component is needed to account for the observed emission. Differently from previous GRBs detected in the very-high-energy range, the model for GRB 201216C strongly favours a wind-like medium. The model parameters have values similar to those found in past studies of the afterglows of GRBs detected up to GeV energies. [ABSTRACT FROM AUTHOR]

Published
2024
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4. Gamma-ray observations of MAXI J1820+070 during the 2018 outburst.

Author

Abe, H, Abe, S, Acciari, V A, Aniello, T, Ansoldi, S, Antonelli, L A, Arbet Engels, A, Arcaro, C, Artero, M, Asano, K, Baack, D, Babić, A, Baquero, A, Barres de Almeida, U, Barrio, J A, Batković, I, Baxter, J, Becerra González, J, Bednarek, W, and Bernardini, E

Subjects
*X-ray binaries, *SOLAR radio emission, *BINARY black holes, *MAGNETIC fields
Abstract

MAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h 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 (HE) 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 HE and very-HE gamma-ray emitting region should be located at a distance from the BH ranging between 1011 and 1013 cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA. [ABSTRACT FROM AUTHOR]

Published
2022
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