Zobrazeno 1 - 10
of 225
pro vyhledávání: '"Bakaldin, A"'
Autor:
Topchiev, N. P., Galper, A. M., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Bakaldin, A. V., Cherniy, R. A., Chernysheva, I. V., Gudkova, E. N., Gusakov, Yu. V., Dalkarov, O. D., Egorov, A. E., Kheymits, M. D., Korotkov, M. G., Leonov, A. A., Malinin, A. G., Mikhailov, V. V., Mikhailova, A. V., Minaev, P. Yu., Pappe, N. Yu., Razumeyko, M. V., Runtso, M. F., Stozhkov, Yu. I., Suchkov, S. I., Yurkin, Yu. T.
The future space-based GAMMA-400 gamma-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years to observe Galactic plane, Galactic Center, Fermi Bubbles, Crab, Vela, Cygnus X, Geminga, Sun, a
Externí odkaz:
http://arxiv.org/abs/2108.12609
Capabilities of the GAMMA-400 gamma-ray telescope to detect gamma-ray bursts from lateral directions
Autor:
Leonov, A A, Galper, A M, Topchiev, N P, Arkhangelskaja, I V, Arkhangelskiy, A I, Bakaldin, A V, Chernysheva, I V, Dalkarov, O D, Egorov, A E, Kheymits, M D, Korotkov, M G, Malinin, A G, Mayorov, A G, Mikhailov, V V, Mikhailova, A V, Minaev, P Yu, Pappe, N Yu, Picozza, P, Sparvoli, R, Stozhkov, Yu I, Suchkov, S I, Yurkin, Yu T
The currently developing space-based gamma-ray telescope GAMMA-400 will measure the gamma-ray and electron + positron fluxes using the main top-down aperture in the energy range from ~20 MeV to several TeV in a highly elliptic orbit (without shading
Externí odkaz:
http://arxiv.org/abs/2103.07161
Autor:
Topchiev, N.P., Galper, A.M., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Cherniy, R.A., Chernysheva, I.V., Gudkova, E.N., Gusakov, Yu.V., Dalkarov, O.D., Egorov, A.E., Kheymits, M.D., Korotkov, M.G., Leonov, A.A., Malinin, A.G., Mikhailov, V.V., Mikhailova, A.V., Minaev, P.Yu., Pappe, N.Yu., Razumeyko, M.V., Runtso, M.F., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T.
Publikováno v:
In Advances in Space Research 1 November 2022 70(9):2773-2793
Autor:
Bakaldin, A. V., Bobkov, S. G., Serdin, O. V., Gorbunov, M. S., Arkhangelskiy, A. I., Leonov, A. A., Topchiev, N. P.
The future GAMMA-400 space mission is aimed for the study of gamma rays in the energy range from ~20 MeV up to ~1 TeV. The observations will carry out with GAMMA-400 gamma-ray telescope installed on-board the Russian Space Observatory. We present the
Externí odkaz:
http://arxiv.org/abs/1707.04883
Autor:
Topchiev, N. P., Galper, A. M., Bonvicini, V., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Bakaldin, A. V., Bobkov, S. G., Dalkarov, O. D., Egorov, A. E., Gusakov, Yu. V., Hnatyk, B. I., Kadilin, V. V., Kheymits, M. D., Korepanov, V. E., Leonov, A. A., Mikhailov, V. V., Moiseev, A. A., Moskalenko, I. V., Naumov, P. Yu., Picozza, P., Runtso, M. F., Serdin, O. V., Sparvoli, R., Spillantini, P., Stozhkov, Yu. I., Suchkov, S. I., Taraskin, A. A., Yurkin, Yu. T., Zverev, V. G.
Extraterrestrial gamma-ray astronomy is now a source of new knowledge in the fields of astrophysics, cosmic-ray physics, and the nature of dark matter. The next absolutely necessary step in the development of extraterrestrial high-energy gamma-ray as
Externí odkaz:
http://arxiv.org/abs/1707.04882
Autor:
Leonov, A. A., Galper, A. M., Topchiev, N. P., Bonvicini, V., Adriani, O., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Bakaldin, A. V., Bobkov, S. G., Boezio, M., Dalkarov, O. D., Egorov, A. E., Glushkov, N. A., Gorbunov, M. S., Gusakov, Yu. V., Hnatyk, B. I., Kadilin, V. V., Kaplin, V. A., Kheymits, M. D., Korepanov, V. E., Longo, F., Mikhailov, V. V., Mocchiutti, E., Moiseev, A. A., Moskalenko, I. V., Naumov, P. Yu., Picozza, P., Runtso, M. F., Serdin, O. V., Sparvoli, R., Spillantini, P., Stozhkov, Yu. I., Suchkov, S. I., Taraskin, A. A., Tavani, M., Yurkin, Yu. T., Zverev, V. G.
The main goal for the GAMMA-400 gamma-ray telescope mission is to perform a sensitive search for signatures of dark matter particles in high-energy gamma-ray emission. Measurements will also concern the following scientific goals: detailed study of t
Externí odkaz:
http://arxiv.org/abs/1612.08877
Capabilities of the GAMMA-400 gamma-ray telescope to detect gamma-ray bursts from lateral directions
Autor:
Leonov, A.A., Galper, A.M., Topchiev, N.P., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Chernysheva, I.V., Dalkarov, O.D., Egorov, A.E., Kheymits, M.D., Korotkov, M.G., Malinin, A.G., Mayorov, A.G., Mikhailov, V.V., Mikhailova, A.V., Yu Minaev, P., Yu Pappe, N., Picozza, P., Sparvoli, R., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T.
Publikováno v:
In Advances in Space Research 1 January 2022 69(1):514-530
Autor:
Sergey I. Suchkov, Irina V. Arkhangelskaja, Andrey I. Arkhangelskiy, Aleksey V. Bakaldin, Irina V. Chernysheva, Arkady M. Galper, Oleg D. Dalkarov, Andrey E. Egorov, Maxim D. Kheymits, Mikhail G. Korotkov, Aleksey A. Leonov, Svetlana A. Leonova, Alexandr G. Malinin, Vladimir V. Mikhailov, Pavel Yu Minaev, Nikolay Yu. Pappe, Mikhail V. Razumeyko, Nikolay P. Topchiev, Yuri T. Yurkin
Publikováno v:
Universe, Vol 9, Iss 8, p 369 (2023)
The upcoming GAMMA-400 experiment will be implemented aboard the Russian astrophysical space observatory, which will be operating in a highly elliptical orbit over a period of 7 years to provide new data on gamma-ray emissions and cosmic-ray electron
Externí odkaz:
https://doaj.org/article/318dcead5e3d4df798ed4ae0545a63d2
Autor:
Topchiev, N. P., Galper, A. M., Bonvicini, V., Adriani, O., Aptekar, R. L., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Bakaldin, A. V., Bergstrom, L., Berti, E., Bigongiari, G., Bobkov, S. G., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bottai, S., Castellini, G., Cattaneo, P. W., Cumani, P., Dalkarov, O. D., Dedenko, G. L., De Donato, C., Dogiel, V. A., Finetti, N., Gascon, D., Gorbunov, M. S., Gusakov, Yu. V., Hnatyk, B. I., Kadilin, V. V., Kaplin, V. A., Kaplun, A. A., Kheymits, M. D., Korepanov, V. E., Larsson, J., Leonov, A. A., Loginov, V. A., Longo, F., Maestro, P., Marrocchesi, P. S., Martinez, M., Menshenin, A. L., Mikhailov, V. V., Mocchiutti, E., Moiseev, A. A., Mori, N., Moskalenko, I. V., Naumov, P. Yu., Papini, P., Paredes, J. M., Pearce, M., Picozza, P., Rappoldi, A., Ricciarini, S., Runtso, M. F., Ryde, F., Serdin, O. V., Sparvoli, R., Spillantini, P., Stozhkov, Yu. I., Suchkov, S. I., Taraskin, A. A., Tavani, M., Tiberio, A., Tyurin, E. M., Ulanov, M. V., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Ward, J. E., Yurkin, Yu. T., Zampa, N., Zirakashvili, V. N., Zverev, V. G.
The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Gal
Externí odkaz:
http://arxiv.org/abs/1507.06246
Autor:
Leonov, A.A., Galper, A.M., Topchiev, N.P., Bakaldin, A.V., Dalkarov, O.D., Dzhivelikyan, E.A., Egorov, A.E., Kheymits, M.D., Mikhailov, V.V., Picozza, P., Sparvoli, R., Suchkov, S.I., Yurkin, Yu.T., Zverev, V.G.
Publikováno v:
In Advances in Space Research 15 May 2019 63(10):3420-3427