Zobrazeno 1 - 10
of 36
pro vyhledávání: '"A M Krassilchtchikov"'
Autor:
E. E. Kholupenko, D. V. Badmaev, A. S. Antonov, A. A. Bogdanov, A. M. Krassilchtchikov, D. O. Kuleshov, Yu. V. Tuboltsev, E. M. Khilkevich, Yu. V. Chichagov
Publikováno v:
Technical Physics. 67:80-103
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3e33e63677304ad4c06c0fb3eaebdeb2
https://doi.org/10.1134/s106378422201008x
https://doi.org/10.1134/s106378422201008x
Autor:
E. V. Sherstnev, P. N. Aruev, A. V. Nikolaev, D. Yu. Petrov, S. V. Bobashev, A. M. Krassilchtchikov
Publikováno v:
Instruments and Experimental Techniques. 64:93-96
An improved architecture of a hybrid matrix detector that operates in the vacuum ultraviolet-hard X-ray range in the 32 × 32 format for high-speed registration of the radiation profile of high-temperature plasma with photon energies of (Eph = 1–10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28f18cfb977cd7cff23eaed97a7ecaf3
https://doi.org/10.1134/s0020441220060147
https://doi.org/10.1134/s0020441220060147
Autor:
Yu. V. Tubol’tsev, E. E. Kholupenko, D. O. Kuleshov, D. V. Badmaev, Yu. V. Chichagov, A. S. Antonov, Andrey Bogdanov, E. M. Khil’kevich, A. M. Krassilchtchikov
Publikováno v:
Technical Physics. 65:886-895
Source and noise signals in a new camera of the TAIGA-IACT Cherenkov γ-ray telescope based on silicon photomultipliers (SiPM) have been simulated. It is shown that application of modern silicon photomultipliers as detecting elements of TAIGA-IACT (i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b193496df2b70ba0bd818806e1a90a6
https://doi.org/10.1134/s1063784220060158
https://doi.org/10.1134/s1063784220060158
Aims: LS 5039 is an enigmatic high-mass gamma-ray binary which hosts a powerful O6.5V companion, but the nature of the compact object is still to be established using multi-wavelength observations. Methods: We analyzed phase-resolved multi-instrument
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::378ebe6b648144133090873bd6702c47
Autor:
F. A. Aharonyan, G. I. Vasiliev, A. V. Nikolaev, E. E. Kholupenko, P. N. Aruev, V. V. Zabrodskii, Andrei M. Bykov, A. M. Krassilchtchikov
Publikováno v:
Technical Physics. 63:1603-1614
Cherenkov emission of extensive air showers (EAS) from cosmic gamma rays and cosmic-ray protons has been modelled. Spectral density of such emission in the 240–700 nm band has been determined for 3 GeV–10 TeV primaries of both sorts. It has been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d253818149ba21382753be74fabc5ea7
https://doi.org/10.1134/s1063784218110154
https://doi.org/10.1134/s1063784218110154
Autor:
A. M. Krassilchtchikov, K. P. Levenfish, Andrei M. Bykov, Yu. A. Kropotina, A. V. Kozlova, Sergei Blinnikov
Publikováno v:
Physics of Atomic Nuclei. 81:139-145
A hydrodynamical description of supernova remnants is based on the approximation of locally equilibrium particle distributions. Shock waves in supernova remnants at various stages of ejecta propagation are collisionless and form nonequilibrium partic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cc5adc2df7988cc6a4fdd7bf329fdf41
https://doi.org/10.1134/s1063778818010155
https://doi.org/10.1134/s1063778818010155
Publikováno v:
Journal of Physics: Conference Series. 2103:012026
The design and scheme of signal readout from silicon photomultipliers OnSemi MicroFJ-60035 used as sensitive elements (pixels) of a new detector cluster for the camera of the Cherenkov gamma-ray telescope TAIGA-IACT are developed. The design of the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82244e24945db60c11ec0ec8abcdcd55
https://doi.org/10.1088/1742-6596/2103/1/012026
https://doi.org/10.1088/1742-6596/2103/1/012026
Publikováno v:
Journal of Physics: Conference Series. 2103:012020
We show that even the slow (subsonic) motion of pulsar wind nebulae (PWNe) relative to an ambient matter has a significant impact on their observables. The motion changes the appearance of nebulae on X-ray images, comparing to what would be observed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0070ebcba60a89f9d2fcc18c8c478e3
https://doi.org/10.1088/1742-6596/2103/1/012020
https://doi.org/10.1088/1742-6596/2103/1/012020
Autor:
D O Kuleshov, V A Simonyan, A A Bogdanov, E E Kholupenko, Yu V Tuboltsev, Yu V Chichagov, A M Krassilchtchikov
Publikováno v:
Journal of Physics: Conference Series. 2103:012036
This study was devoted to measurements of the UV-range photon detection efficiency (PDE) of OnSemi MicroFJ SiPM detectors use together with custom UV filters and of the transmission coefficient of these filters at 277 nm. The final goal of these meas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::07de0559eeb569b1fa1cf6f99fdbdbc9
https://doi.org/10.1088/1742-6596/2103/1/012036
https://doi.org/10.1088/1742-6596/2103/1/012036
Publikováno v:
Journal of Physics: Conference Series. 2103:012006
Observations of hard X-ray emission from the Vela pulsar wind nebula (PWN) with the ISGRI camera aboard INTEGRAL gamma-ray observatory have been analysed with the aim to search for possible flux variability on scales from weeks to years, which could
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5f9b2003ce509626f1f23d8926c12d62
https://doi.org/10.1088/1742-6596/2103/1/012006
https://doi.org/10.1088/1742-6596/2103/1/012006