Zobrazeno 1 - 10
of 799
pro vyhledávání: '"Moskvitin, A."'
Autor:
Vlasyuk, V. V., Sotnikova, Yu. V., Volvach, A. E., Spiridonova, O. I., Stolyarov, V. A., Mikhailov, A. G., Kovalev, Yu. A., Kovalev, Y. Y., Khabibullina, M. L., Kharinov, M. A., Yang, L., Mingaliev, M. G., Semenova, T. A., Zhekanis, P. G., Mufakharov, T. V., Udovitskiy, R. Yu., Kudryashova, A. A., Volvach, L. N., Erkenov, A. K., Moskvitin, A. S., Emelianov, E. V., Fatkhullin, T. A., Tsybulev, P. G., Nizhelsky, N. A., Zhekanis, G. V., Kravchenko, E. V.
We present an optical-to-radio study of the BL Lac object S4 0954+658 observations during 1998-2023. The measurements were obtained with the SAO RAS Zeiss-1000 1-m and AS-500/2 0.5-m telescopes in 2003-2023, with the RATAN-600 radio telescope at 1.25
Externí odkaz:
http://arxiv.org/abs/2401.03992
Autor:
Belkin, S., Pozanenko, A. S., Minaev, P. Y., Pankov, N. S., Volnova, A. A., Rossi, A., Stratta, G., Benetti, S., Palazzi, E., Moskvitin, A. S., Burhonov, O., Rumyantsev, V. V., Klunko, E. V., Inasaridze, R. Ya., Reva, I. V., Kim, V., Jelinek, M., Kann, D. A., Volvach, A. E., Volvach, L. N., Xu, D., Zhu, Z., Fu, S., Mkrtchyan, A. A.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 4, February 2024, Pages 11507-11520
We present full photometric coverage and spectroscopic data for soft GRB 201015A with a redshift z = 0.426. Our data spans a time range of 85 days following the detection of GRB. These observations revealed an underlying supernova SN 201015A with a m
Externí odkaz:
http://arxiv.org/abs/2401.03579
Autor:
Pankov, N. S., Pozanenko, A. S., Minaev, P. Yu., Belkin, S. O., Volnova, A. A., Reva, I. V., Serebryanskiy, A. V., Krugov, M. A., Naroenkov, S. A., Novichonok, A. O., Zhornichenko, A. A., Rumyantsev, V. V., Antonyuk, K. A., Egamberdiev, Sh. A., Burkhonov, O. A., Klunko, E. V., Moskvitin, A. S., Molotov, I. E., Inasaridze, R. Ya.
Publikováno v:
Astron. Lett. 49 (2023)
We present the results of our analysis of multiwavelength observations for the long gamma-ray burst GRB 200829A. The burst redshift $z \approx 1.29 \pm 0.04$ has been determined photometrically at the afterglow phase. In gamma rays the event is one o
Externí odkaz:
http://arxiv.org/abs/2308.02090
Autor:
Moskvitin, V. M., Semenova, N.
Publikováno v:
Russian journal of nonlinear dynamics 2023
In recent years, more and more researchers in the field of neural networks are interested in creating hardware implementations where neurons and the connection between them are realized physically. The physical implementation of ANN fundamentally cha
Externí odkaz:
http://arxiv.org/abs/2303.13262
Publikováno v:
Electrical engineering & Electromechanics, Vol 2024, Iss 1, Pp 61-68 (2024)
Introduction. One of the main driving factors of the demand for cable and conductor products is the modern trend of urbanization, which leads to an increase in cities with significantly increased requirements for electrical networks of transportation
Externí odkaz:
https://doaj.org/article/311153cec9ab4a8e86fd4e6b6790526b
Autor:
Gupta, Rahul, Gupta, S., Chattopadhyay, T., Lipunov, V., Castro-Tirado, A. J., Bhattacharya, D., Pandey, S. B., Oates, S. R., Kumar, Amit, Hu, Y. -D., Valeev, A. F., Minaev, P. Yu., Kumar, H., Vinko, J., Dimple, Sharma, V., Aryan, A., Castellón, A., Gabovich, A., Moskvitin, A., Ordasi, A., Pál, A., Pozanenko, A., Zhang, B. -B., Kumar, B., Svinkin, D., Saraogi, D., Vlasenko, D., Fernández-García, E., Gorbovskoy, E., Anupama, G. C., Misra, K., Sárneczky, K., Kriskovics, L., Castro-Tirado, M. Á., Caballero-García, M. D., Tiurina, N., Balanutsa, P., Lopez, R. R., Sánchez-Ramírez, R., Szakáts, R., Belkin, S., Guziy, S., Iyyani, S., Tiwari, S. N., Vadawale, Santosh V., Sun, T., Bhalerao, V., Kornilov, V., Sokolov, V. V.
Multi-pulsed GRB 190530A, detected by the GBM and LAT onboard \fermi, is the sixth most fluent GBM burst detected so far. This paper presents the timing, spectral, and polarimetric analysis of the prompt emission observed using \AstroSat and \fermi t
Externí odkaz:
http://arxiv.org/abs/2201.01167
Autor:
Pandey, S. B., Kumar, Amit, Kumar, Brajesh, Anupama, G. C., Srivastav, S., Sahu, D. K., Vinko, J., Aryan, A., Pastorello, A., Benetti, S., Tomasella, L., Singh, Avinash, Moskvitin, A. S., Sokolov, V. V., Gupta, R., Misra, K., Ochner, P., Valenti, S.
Optical, near-infrared (NIR) photometric and spectroscopic studies, along with the optical imaging polarimetric results for SN 2012au, are presented in this article to constrain the nature of the progenitor and other properties. Well-calibrated multi
Externí odkaz:
http://arxiv.org/abs/2106.15856
Publikováno v:
Известия высших учебных заведений: Прикладная нелинейная динамика, Vol 31, Iss 4, Pp 484-500 (2023)
The purpose of this study is to establish the features of noise propagation and accumulation in a recurrent neural network using a simplified echo network as an example. In this work, we studied the influence of activation function of artificial neur
Externí odkaz:
https://doaj.org/article/d9eafe98650647a0948843c36e64dc0c
Autor:
Balakina, Elena A., Pruzhinskaya, Maria V., Moskvitin, Alexander S., Blinnikov, Sergei I., Wang, Xiaofeng, Xiang, Danfeng, Lin, Han, Rui, Liming, Wang, Huijuan
In this work we present the photometric and spectroscopic observations of Type IIb Supernova 2017gpn. This supernova was discovered in the error-box of LIGO/Virgo G299232 gravitational-wave event. We obtained the light curves in B and R passbands and
Externí odkaz:
http://arxiv.org/abs/2008.07934
Autor:
Hu, Y. -D., Oates, S. R., Lipunov, V. M., Zhang, B. -B., Castro-Tirado, A. J., Jeong, S., Sánchez-Ramírez, R., Tello, J. C., Cunniffe, R., Gorbovskoy, E., Caballero-García, M. D., Pandey, S. B., Kornilov, V. G., Tyurina, N. V., Kuznetsov, A. S., Balanutsa, P. V., Gress, O. A., Gorbunov, I., Vlasenko, D. M., Vladimirov, V. V., Budnev, N. M., Balakin, F., Ershova, O., Krushinski, V. V., Gabovich, A. V., Yurkov, V. V., Gorosabel, J., Moskvitin, A. S., Burenin, R. A., Sokolov, V. V., Delgado, I., Guziy, S., Fernandez-García, E. J., Park, I. H.
Publikováno v:
A&A 632, A100 (2019)
We investigate the long GRB140629A through multiwavelength observations, which cover optical, infrared and X-rays between 40s and 3yr after the burst, to derive the properties of the dominant jet and its host galaxy. Polarisation observations by the
Externí odkaz:
http://arxiv.org/abs/1910.10747