7,754 results on '"Larionova, A."'
Search Results
202. Contagious convergent cumulative cooperation: the dynamic development of the G20, BRICS and SCO
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Kirton, John and Larionova, Marina
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- 2022
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203. Rapid quasi-periodic oscillations in the relativistic jet of BL Lacertae
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Jorstad, S. G., Marscher, A. P., Raiteri, C. M., Villata, M., Weaver, Z. R., Zhang, H., Dong, L., Gómez, J. L., Perel, M. V., Savchenko, S. S., Larionov, V. M., Carosati, D., Chen, W. P., Kurtanidze, O. M., Marchini, A., Matsumoto, K., Mortari, F., Aceti, P., Acosta-Pulido, J. A., Andreeva, T., Apolonio, G., Arena, C., Arkharov, A., Bachev, R., Banfi, M., Bonnoli, G., Borman, G. A., Bozhilov, V., Carnerero, M. I., Damljanovic, G., Ehgamberdiev, S. A., Elsässer, D., Frasca, A., Gabellini, D., Grishina, T. S., Gupta, A. C., Hagen-Thorn, V. A., Hallum, M. K., Hart, M., Hasuda, K., Hemrich, F., Hsiao, H. Y., Ibryamov, S., Irsmambetova, T. R., Ivanov, D. V., Joner, M. D., Kimeridze, G. N., Klimanov, S. A., Knött, J., Kopatskaya, E. N., Kurtanidze, S. O., Kurtenkov, A., Kuutma, T., Larionova, E. G., Leonini, S., Lin, H. C., Lorey, C., Mannheim, K., Marino, G., Minev, M., Mirzaqulov, D. O., Morozova, D. A., Nikiforova, A. A., Nikolashvili, M. G., Ovcharov, E., Papini, R., Pursimo, T., Rahimov, I., Reinhart, D., Sakamoto, T., Salvaggio, F., Semkov, E., Shakhovskoy, D. N., Sigua, L. A., Steineke, R., Stojanovic, M., Strigachev, A., Troitskaya, Y. V., Troitskiy, I. S., Tsai, A., Valcheva, A., Vasilyev, A. A., Vince, O., Waller, L., Zaharieva, E., and Chatterjee, R.
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- 2022
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204. The Mu Rhythm in Current Research: Theoretical and Methodological Aspects
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Larionova, E. V., Garakh, Zh. V., and Zaytseva, Yu. S.
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- 2022
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205. On the Self-Propagating High-Temperature Synthesis of a Ti–Si–C Composite Using Fullerites
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Nikonova, R. M., Larionova, N. S., and Lad’yanov, V. I.
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- 2022
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206. AGILE, Fermi, Swift, and GASP-WEBT multi-wavelength observations of the high-redshift blazar 4C $+$71.07 in outburst
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Vercellone, S., Romano, P., Piano, G., Vittorini, V., Donnarumma, I., Munar-Adrover, P., Raiteri, C. M., Villata, M., Verrecchia, F., Lucarelli, F., Pittori, C., Bulgarelli, A., Fioretti, V., Tavani, M., Acosta-Pulido, J. A., Agudo, I., Arkharov, A. A., Bach, U., Bachev, R., Borman, G. A., Butuzova, M. S., Carnerero, M. I., Casadio, C., Damljanovic, G., D'Ammando, F., Di Paola, A., Doroshenko, V. T., Efimova, N. V., Ehgamberdiev, Sh. A., Giroletti, M., Gómez, J. L., Grishina, T. S., Järvelä, E., Klimanov, S. A., Kopatskaya, E. N., Kurtanidze, O. M., Lähteenmäki, A., Larionov, V. M., Larionova, L. V., Mihov, B., Mirzaqulov, D. O., Molina, S. N., Morozova, D. A., Nazarov, S. V., Orienti, M., Righini, S., Savchenko, S. S., Semkov, E., Slavcheva-Mihova, L., Strigachev, A., Tornikoski, M., Troitskaya, Yu. V., Vince, O., Cattaneo, P. W., Colafrancesco, S., Longo, F., Morselli, A., Paoletti, F., and Parmiggiani, N.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The flat-spectrum radio quasar 4C $+$71.07 is a high-redshift ($z=2.172$), $\gamma$-loud blazar whose optical emission is dominated by the thermal radiation from accretion disc. 4C $+$71.07 has been detected in outburst twice by the AGILE $\gamma$-ray satellite during the period end of October - mid November 2015, when it reached a $\gamma$-ray flux of the order of $F_{\rm E>100\,MeV} = (1.2 \pm 0.3)\times 10^{-6}$ photons cm$^{-2}$ s$^{-1}$ and $F_{\rm E>100\,MeV} = (3.1 \pm 0.6)\times 10^{-6}$ photons cm$^{-2}$ s$^{-1}$, respectively, allowing us to investigate the properties of the jet and of the emission region. We investigated its spectral energy distribution by means of almost simultaneous observations covering the cm, mm, near-infrared, optical, ultra-violet, X-ray and $\gamma$-ray energy bands obtained by the GASP-WEBT Consortium, the Swift and the AGILE and Fermi satellites. The spectral energy distribution of the second $\gamma$-ray flare (the one whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about $4\times10^{47}$ erg s$^{-1}$. During the most prominent $\gamma$-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, large-mass black-hole flat-spectrum radio quasars might be good targets for future $\gamma$-ray satellites such as e-ASTROGAM., Comment: Accepted for publication in A&A. 9 pages, 4 Figures, 3 Tables
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- 2018
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207. The extreme HBL behaviour of Markarian 501 during 2012
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Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Arcaro, C., Babić, A., Banerjee, B., Bangale, P., de Almeida, U. Barres, Barrio, J. A., González, J. Becerra, Bednarek, W., Bernardini, E., Berti, A., Bhattacharyya, W., Blanch, O., Bonnoli, G., Carosi, R., Carosi, A., Chatterjee, A., Colak, S. M., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Cumani, P., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Di Pierro, F., Doert, M., Domínguez, A., Prester, D. Dominis, Doro, M., Glawion, D. Eisenacher, Engelkemeier, M., Ramazani, V. Fallah, Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Fruck, C., Galindo, D., López, R. J. García, Garczarczyk, M., Gaug, M., Giammaria, P., Godinović, N., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Ishio, K., Konno, Y., Kubo, H., Kushida, J., Kuveždić, D., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., Maggio, C., Majumdar, P., Makariev, M., Maneva, G., Manganaro, M., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Menzel, U., Minev, M., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moreno, V., Moretti, E., Nagayoshi, T., Neustroev, V., Niedzwiecki, A., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Paiano, S., Palacio, J., Paneque, D., Paoletti, R., Paredes, J. M., Pedaletti, G., Peresano, M., Perri, L., Persic, M., Moroni, P. G. Prada, Prandini, E., Puljak, I., Garcia, J. R., Reichardt, I., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saito, T., Satalecka, K., Schroeder, S., Schweizer, T., Shore, S. N., Sitarek, J., Šnidarić, I., Sobczynska, D., Stamerra, A., Strzys, M., Surić, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Treves, A., Tsujimoto, S., Vanzo, G., Acosta, M. Vazquez, Vovk, I., Ward, J. E., Will, M., Zarić, D., Arbet-Engels, A., Baack, D., Balbo, M., Biland, A., Blank, M., Bretz, T., Bruegge, K., Bulinski, M., Buss, J., Dmytriiev, A., Dorner, D., Einecke, S., Elsaesser, D., Herbst, T., Hildebrand, D., Kortmann, L., Linhoff, L., Mahlke, M., Mannheim, K., Mueller, S. A., Neise, D., Neronov, A., Noethe, M., Oberkirch, J., Paravac, A., Rhode, W., Schleicher, B., Schulz, F., Sedlaczek, K., Shukla, A., Sliusar, V., Walter, R., Archer, A., Benbow, W., Bird, R., Brose, R., Buckley, J. H., Bugaev, V., Christiansen, J. L., Cui, W., Daniel, M. K., Falcone, A., Feng, Q., Finley, J. P., Gillanders, G. H., Gueta, O., Hanna, D., Hervet, O., Holder, J., Hughes, G., Hütten, M., Humensky, T. B., Johnson, C. A., Kaaret, P., Kar, P., Kelley-Hoskins, N., Kertzman, M., Kieda, D., Krause, M., Krennrich, F., Kumar, S., Lang, M. J., Lin, T. T. Y., Maier, G., McArthur, S., Moriarty, P., Mukherjee, R., O'Brien, S., Ong, R. A., Otte, A. N., Park, N., Petrashyk, A., Pichel, A., Pohl, M., Quinn, J., Ragan, K., Reynolds, P. T., Richards, G. T., Roache, E., Rovero, A. C., Rulten, C., Sadeh, I., Santander, M., Sembroski, G. H., Shahinyan, K., Sushch, I., Tyler, J., Wakely, S. P., Weinstein, A., Wells, R. M., Wilcox, P., Wilhel, A., Williams, D. A., Williamson, T. J, Zitzer, B., Perri, M., Verrecchia, F., Leto, C., Villata, M., Raiteri, C. M., Jorstad, S. G., Larionov, V. M., Blinov, D. A., Grishina, T. S., Kopatskaya, E. N., Larionova, E. G., Nikiforova, A. A., Morozova, D. A., Troitskaya, Yu. V., Troitsky, I. S., Kurtanidze, O. M., Nikolashvili, M. G., Kurtanidze, S. O., Kimeridze, G. N., Chigladze, R. A., Strigachev, A., Sadun, A. C., Moody, J. W., Chen, W. P., Lin, H. C., Acosta-Pulido, J. A., Arévalo, M. J., Carnerero, M. I., González-Morales, P. A., Manilla-Robles, A., Jermak, H., Steele, I., Mundel, C., Benítez, E., Hiriart, D., Smith, P. S., Max-Moerbeck, W., Readhead, A. C. S., Richards, J. L., Hovatta, T., Lähteenmäki, A., Tornikoski, M., Tammi, J., Georganopoulos, M., and Baring, M. G.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
A multiwavelength campaign was organized to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC, FACT and VERITAS Cherenkov telescopes, the instruments on board the Swift and Fermi spacecraft, and the telescopes operated by the GASP-WEBT collaboration. Mrk 501 showed a very high energy (VHE) gamma-ray flux above 0.2 TeV of $\sim$0.5 times the Crab Nebula flux (CU) for most of the campaign. The highest activity occurred on 2012 June 9, when the VHE flux was $\sim$3 CU, and the peak of the high-energy spectral component was found to be at $\sim$2 TeV. This study reports very hard X-ray spectra, and the hardest VHE spectra measured to date for Mrk 501. The fractional variability was found to increase with energy, with the highest variability occurring at VHE, and a significant correlation between the X-ray and VHE bands. The unprecedentedly hard X-ray and VHE spectra measured imply that their low- and high-energy components peaked above 5 keV and 0.5 TeV, respectively, during a large fraction of the observing campaign, and hence that Mrk 501 behaved like an extreme high-frequency- peaked blazar (EHBL) throughout the 2012 observing season. This suggests that being an EHBL may not be a permanent characteristic of a blazar, but rather a state which may change over time. The one-zone synchrotron self-Compton (SSC) scenario can successfully describe the segments of the SED where most energy is emitted, with a significant correlation between the electron energy density and the VHE gamma-ray activity, suggesting that most of the variability may be explained by the injection of high-energy electrons. The one-zone SSC scenario used reproduces the behaviour seen between the measured X-ray and VHE gamma-ray fluxes, and predicts that the correlation becomes stronger with increasing energy of the X-rays., Comment: 25 pages, 9 figures, accepted for publication in A&A. Corresponding authors: Gareth Hughes (gareth.hughes@cfa.harvard.edu), David Paneque (dpaneque@mppmu.mpg.de), Amit Shukla (amit.shukla@astro.uni-wuerzburg.de)
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- 2018
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208. Multi-wavelength characterization of the blazar S5~0716+714 during an unprecedented outburst phase
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MAGIC Collaboration, Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Arcaro, C., Baack, D., Babić, A., Banerjee, B., Bangale, P., de Almeida, U. Barres, Barrio, J. A., González, J. Becerra, Bednarek, W., Bernardini, E., Berse, R. Ch., Berti, A., Bhattacharyya, W., Biland, A., Blanch, O., Bonnoli, G., Carosi, R., Carosi, A., Ceribella, G., Chatterjee, A., Colak, S. M., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Cumani, P., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Di Pierro, F., Domínguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Einecke, S., Elsaesser, D., Ramazani, V. Fallah, Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Fruck, C., Galindo, D., Gallozzi, S., López, R. J. García, Garczarczyk, M., Gaug, M., Giammaria, P., Godinović, N., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Ishio, K., Konno, Y., Kubo, H., Kushida, J., Kuveždić, D., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., Maggio, C., Majumdar, P., Makariev, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Masuda, S., Mazin, D., Mielke, K., Minev, M., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moreno, V., Moretti, E., Nagayoshi, T., Neustroev, V., Niedzwiecki, A., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Paiano, S., Palacio, J., Paneque, D., Paoletti, R., Paredes, J. M., Pedaletti, G., Peresano, M., Persic, M., Moroni, P. G. Prada, Prandini, E., Puljak, I., Garcia, J. R., Reichardt, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saito, T., Satalecka, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Stamerra, A., Strzys, M., Surić, T., Takahashi, M., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Treves, A., Tsujimoto, S., Vanzo, G., Acosta, M. Vazquez, Vovk, I., Ward, J. E., Will, M., Zarić, D., Collaboration, Fermi-LAT, Bastieri, D., Gasparrini, D., Lott, B., Rani, B., Thompson, D. J., Collaborators, MWL, Agudo, I., Angelakis, E., Borman, G. A., Casadio, C., Grishina, T. S., Gurwell, M., Hovatta, T., Itoh, R., Järvelä, E., Jermak, H., Jorstad, S., Kopatskaya, E. N., Kraus, A., Krichbaum, T. P., Kuin, N. P. M., Lähteenmäki, A., Larionov, V. M., Larionova, L. V., Lien, A. Y., Madejski, G., Marscher, A., Myserlis, I., Max-Moerbeck, W., Molina, S. N., Morozova, D. A., Nalewajko, K., Pearson, T. J., Ramakrishnan, V., Readhead, A. C. S., Reeves, R. A., Savchenko, S. S., Steele, I. A., Tornikoski, M., Troitskaya, Yu. V., Troitsky, I., Vasilyev, A. A., and Zensus, J. Anton
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The BL Lac object S5~0716+714, a highly variable blazar, underwent an impressive outburst in January 2015 (Phase A), followed by minor activity in February (Phase B). The MAGIC observations were triggered by the optical flux observed in Phase A, corresponding to the brightest ever reported state of the source in the R-band. The comprehensive dataset collected is investigated in order to shed light on the mechanism of the broadband emission. Multi-wavelength light curves have been studied together with the broadband Spectral Energy Distributions (SEDs). The data set collected spans from radio, optical photometry and polarimetry, X-ray, high-energy (HE, 0.1 GeV < E < 100 GeV) with \textit{Fermi}-LAT to the very-high-energy (VHE, E>100 GeV) with MAGIC. The flaring state of Phase A was detected in all the energy bands, providing for the first time a multi-wavelength sample of simultaneous data from the radio band to the VHE. In the constructed SED the \textit{Swift}-XRT+\textit{NuSTAR} data constrain the transition between the synchrotron and inverse Compton components very accurately, while the second peak is constrained from 0.1~GeV to 600~GeV by \textit{Fermi}+MAGIC data. The broadband SED cannot be described with a one-zone synchrotron self-Compton model as it severely underestimates the optical flux in order to reproduce the X-ray to $\gamma$-ray data. Instead we use a two-zone model. The EVPA shows an unprecedented fast rotation. An estimation of the redshift of the source by combined HE and VHE data provides a value of $z = 0.31 \pm 0.02_{stats} \pm 0.05_{sys}$, confirming the literature value. The data show the VHE emission originating in the entrance and exit of a superluminal knot in and out a recollimation shock in the inner jet. A shock-shock interaction in the jet seems responsible for the observed flares and EVPA swing. This scenario is also consistent with the SED modelling.
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- 2018
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209. The Bright $\gamma$-ray Flare of 3C 279 in June 2015: AGILE Detection and Multifrequency Follow-up Observations
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Pittori, C., Lucarelli, F., Verrecchia, F., Raiteri, C. M., Villata, M., Vittorini, V., Tavani, M., Puccetti, S., Perri, M., Donnarumma, I., Vercellone, S., Acosta-Pulido, J. A., Bachev, R., Benitez, E., Borman, G. A., Carnerero, M. I., Carosati, D., Chen, W. P., Ehgamberdiev, Sh. A., Goded, A., Grishina, T. S., Hiriart, D., Hsiao, H. Y., Jorstad, S. G., Kimeridze, G. N., Kopatskaya, E. N., Kurtanidze, O. M., Kurtanidze, S. O., Larionov, V. M., Larionova, L. V., Marscher, A. P., Mirzaqulov, D. O., Morozova, D. A., Nilsson, K., Samal, M. R., Sigua, L. A., Spassov, B., Strigachev, A., Takalo, L. O., Antonelli, L. A., Bulgarelli, A., Cattaneo, P., Colafrancesco, S., Giommi, P., Longo, F., Morselli, A., and Paoletti, F.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report the AGILE detection and the results of the multifrequency follow-up observations of a bright $\gamma$-ray flare of the blazar 3C 279 in June 2015. We use AGILE-GRID and Fermi-LAT $\gamma$-ray data, together with Swift-XRT, Swift-UVOT, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the $\gamma$-ray flare. The $\gamma$-ray flaring data, compared with as yet unpublished simultaneous optical data which allow to set constraints on the big blue bump disk luminosity, show very high Compton dominance values of $\sim 100$, with a ratio of $\gamma$-ray to optical emission rising by a factor of three in a few hours. The multi-wavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the June 2015 flare are also compared with already published data and non-simultaneous historical 3C 279 archival data., Comment: 13 pages, 5 figures,5 Tables. Accepted for publication in ApJ
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- 2018
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210. Checklist as a Working Tool for the Formation of Digital Literacy of BIM-Specialists in the Multilingual World
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Shalina, Daria, primary, Tikhonov, Vladislav, additional, Stepanova, Natalia, additional, and Larionova, Viola, additional
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- 2023
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211. Luminescent lanthanide-based single-molecule magnets
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Larionova, Joulia, primary, Guari, Yannick, additional, Sene, Saad, additional, and Félix, Gautier, additional
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- 2023
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212. Gamification in Education: A Literature Review
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Daineko, Liudmila V., primary, Goncharova, Natalia V., additional, Zaitseva, Ekaterina V., additional, Larionova, Viola A., additional, and Dyachkova, Irina A., additional
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- 2023
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213. Communications Using Gamification for the Implementation of Urban Projects
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Nalimova, Ekaterina, primary, Larionova, Viola, additional, and Stepanova, Natalia, additional
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- 2023
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214. The Experience of Forming Multilingual Competences in Universities in Russia and Turkey
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Goncharova, Natalia V., primary, Daineko, Liudmila V., additional, Larionova, Viola, additional, and Demir, Çağlar, additional
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- 2023
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215. Modern Approaches to the Management of Children with Mucopolysaccharidosis Type I
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Galina V. Baidakova, Alexander A. Baranov, Irina V. Vakhlova, Nato D. Vashakmadze, Elena Yu. Voskoboeva, Ekaterina Yu. Zakharova, Ludmila M. Kuzenkova, Sergey I. Kutsev, Valentina I. Larionova, Tina V. Lobzhanidze, Ludmila K. Mikhailova, Svetlana V. Mikhailova, Sergey V. Moiseev, Leyla S. Namazova-Baranova, Sergey S. Nikitin, Natalya L. Pechatnikova, Olga A. Polyakova, Alla N. Semyachkina, and Olga V. Udalova
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mucopolysaccharidosis type i ,diagnosis ,treatment ,prognosis ,children ,Pediatrics ,RJ1-570 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
This article presents modern data on epidemiology, etiology, and clinical manifestations of mucopolysaccharidosis (MPS) type I in children. MPS develops due to deficiency of particular lysosomal enzyme which determines the disease type. The article considers in details disease's pathogenesis and classification. Evidence-based approaches to diagnosis (differential diagnosis included) are covered, moreover, special attention is paid to pathogenetic, symptomatic, and surgical treatment of MPS.
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- 2022
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216. Diaries of the Protagonist in the Structure of Autobiographical Prose by A. A. Grigoriev (Based on the Stories 'Man of the Future,' 'My Acquaintance with Vitalin,' 'Ophelia')
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Anna N. Larionova
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a. a. grigoriev ,autobiographical prose ,character ,diary ,story ,trilogy ,inner world ,dreamer ,romantic ,Literature (General) ,PN1-6790 - Abstract
The basis of the trilogy about Vitalin by A. A. Grigoriev is the diary entries of the autobiographical character. The writer consciously refers to this form of narration, since it allows the most complete disclosure of the inner world of the protagonist, conveying his thoughts, feelings, emotions, showing the complexity and inconsistency of his nature. Thanks to fragments of the diaries, the themes of the stories expand: from love experiences to philosophical reflections, reflections on the truth, the meaning of life, and the search for happiness. The protagonist’s diary also influences the chronotope of stories, expanding the space and time of the narrative, introducing a life background, background of events into the work, and at the same time enriching our understanding of the character. The author of the article briefly dwells on the autobiographical elements in the life of Arseny Vitalin, notes his resemblance to the character of the novel by M. Yu. Lermontov — Pechorin. Special attention is paid to the genre originality of Grigoriev’s works, their simultaneous isolation and inclusion in the cycle, trilogy. Besides the article discusses the diary fragment “The Dreamer’s Diary” and its meaning in the text. Psychologically convincingly, the author shows that Vitalin, immersed in love experiences, but unable to share his thoughts with someone close to him, finds an outlet for his pent-up feelings in keeping a diary, on the pages of which he gives free rein to his feelings and actions.
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- 2022
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217. Early-onset oral cancer as a clinical entity: aetiology and pathogenesis
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Kolegova, E.S., Patysheva, M.R., Larionova, I.V., Fedorova, I.K., Kulbakin, D.E., Choinzonov, E.L., and Denisov, E.V.
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- 2022
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218. The character of radionuclide contamination of natural lakes at the territory of the Semipalatinsk test site
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Aidarkhanova, A., Larionova, N., Tleukanova, Zh., Mamyrbaeva, A., Ermakova, R., Svetacheva, Yu., Aktayev, M., and Panitskiy, A.
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- 2022
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219. Peculiarities of radioactive soil contamination in places of underground nuclear tests in the Semipalatinsk test site
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Krivitskiy, P.Ye., Larionova, N.V., Monayenko, V.N., Subbotin, S.B., Chernov, A.A., and Panitskiy, A.V.
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- 2022
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220. Quasi-simultaneous Optical Flux and Polarization Variability of the Binary Super Massive Black Hole Blazar OJ 287 from 2015 to 2023: Detection of an Anticorrelation in Flux and Polarization Variability
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Alok C. Gupta, Pankaj Kushwaha, Mauri J. Valtonen, Sergey S. Savchenko, Svetlana G. Jorstad, Ryo Imazawa, Paul J. Wiita, Minfeng Gu, Alan P. Marscher, Zhongli Zhang, Rumen Bachev, G. A. Borman, Haritma Gaur, T. S. Grishina, V. A. Hagen-Thorn, E. N. Kopatskaya, V. M. Larionov, E. G. Larionova, L. V. Larionova, D. A. Morozova, T. Nakaoka, A. Strigachev, Yulia V. Troitskaya, I. S. Troitsky, M. Uemura, A. A. Vasilyev, Z. R. Weaver, and A. V. Zhovtan
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Blazars ,Active galactic nuclei ,BL Lacertae objects ,Jets ,Optical astronomy ,Astrophysics ,QB460-466 - Abstract
We study the optical flux and polarization variability of the binary black hole blazar OJ 287 using quasi-simultaneous observations from 2015 to 2023 carried out using telescopes in the USA, Japan, Russia, Crimea, and Bulgaria. This is one of the most extensive quasi-simultaneous optical flux and polarization variability studies of OJ 287. OJ 287 showed large amplitude, ∼3.0 mag flux variability, large changes of ∼37% in degree of polarization, and a large swing of ∼215° in the angle of the electric vector of polarization. During the period of observation, several flares in flux were detected. Those flares are correlated with a rapid increase in the degree of polarization and swings in electric vector of polarization angle. A peculiar behavior of anticorrelation between flux and polarization degree, accompanied by a nearly constant polarization angle, was detected from JD 2,458,156 to JD 2,458,292. We briefly discuss some explanations for the flux and polarization variations observed in OJ 287.
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- 2023
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221. Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009
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Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Banerjee, B., Bangale, P., de Almeida, U. Barres, Barrio, J. A., González, J. Becerra, Bednarek, W., Bernardini, E., Berti, A., Biasuzzi, B., Biland, A., Blanch, O., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Buson, S., Carosi, A., Chatterjee, A., Clavero, R., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Wilhelmi, E. de Ona, Di Pierro, F., Doert, M., Domínguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Einecke, S., Glawion, D. Eisenacher, Elsaesser, D., Engelkemeier, M., Ramazani, V. Fallah, Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Galindo, D., López, R. J. García, Garczarczyk, M., Terrats, D. Garrido, Gaug, M., Giammaria, P., Godinović, N., Munoz, A. González, Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hanabata, Y., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Hughes, G., Idec, W., Kodani, K., Konno, Y., Kubo, H., Kushida, J., La Barbera, A., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., López-Coto, R., Majumdar, P., Makariev, M., Mallot, K., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martínez, M., Mazin, D., Menzel, U., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moretti, E., Nakajima, D., Neustroev, V., Niedzwiecki, A., Rosillo, M. Nievas, Nilsson, K., Nishijima, K., Noda, K., Nogués, L., Overkemping, A., Paiano, S., Palacio, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Paredes-Fortuny, X., Pedaletti, G., Peresano, M., Perri, L., Persic, M., Poutanen, J., Moroni, P. G. Prada, Prandini, E., Puljak, I., Reichardt, I., Rhode, W., Ribó, M., Rico, J., Garcia, J. Rodriguez, Saito, T., Satalecka, K., Schröder, S., Schultz, C., Schweizer, T., Shore, S. N., Sillanpää, A., Sitarek, J., Snidaric, I., Sobczynska, D., Stamerra, A., Steinbring, T., Strzys, M., Surić, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Tescaro, D., Teshima, M., Thaele, J., Torres, D. F., Toyama, T., Treves, A., Vanzo, G., Verguilov, V., Vovk, I., Ward, J. E., Will, M., Wu, M. H., Zanin, R., Abeysekara, A. U., Archambault, S., Archer, A., Benbow, W., Bird, R., Buchovecky, M., Buckley, J. H., Bugaev, V., Connolly, M. P., Cui, W., Dickinson, H. J., Falcone, A., Feng, Q., Finley, J. P., Fleischhack, H., Flinders, A., Fortson, L., Gillanders, G. H., Griffin, S., Grube, J., Hütten, M., Hanna, D., Holder, J., Humensky, T. B., Kaaret, P., Kar, P., Kelley-Hoskins, N., Kertzman, M., Kieda, D., Krause, M., Krennrich, F., Lang, M. J., Maier, G., McCann, A., Moriarty, P., Mukherjee, R., Nieto, D., O'Brien, S., Ong, R. A., Otte, N., Park, N., Perkins, J., Pichel, A., Pohl, M., Popkow, A., Pueschel, E., Quinn, J., Ragan, K., Reynolds, P. T., Richards, G. T., Roache, E., Rovero, A. C., Rulten, C., Sadeh, I., Santander, M., Sembroski, G. H., Shahinyan, K., Telezhinsky, I., Tucci, J. V., Tyler, J., Wakely, S. P., Weinstein, A., Wilcox, P., Wilhelm, A., Williams, D. A., Zitzer, B., Razzaque, S., Villata, M., Raiteri, C. M., Aller, H. D., Aller, M. F., Larionov, V. M., Arkharov, A. A., Blinov, D. A., Efimova, N. V., Grishina, T. S., Hagen-Thorn, V. A., Kopatskaya, E. N., Larionova, L. V., Larionova, E. G., Morozova, D. A., Troitsky, I. S., Ligustri, R., Calcidese, P., Berdyugin, A., Kurtanidze, O. M., Nikolashvili, M. G., Kimeridze, G. N., Sigua, L. A., Kurtanidze, S. O., Chigladze, R. A., Chen, W. P., Koptelova, E., Sakamoto, T., Sadun, A. C., Moody, J. W., Pace, C., Pearson III, R., Yatsu, Y., Mori, Y., Carraminyana, A., Carrasco, L., de la Fuente, E., Norris, J. P., Smith, P. S., Wehrle, A., Gurwell, M. A., Zook, Alma, Pagani, C., Perri, M., Capalbi, M., Cesarini, A., Krimm, H. A., Kovalev, Y. Y., Kovalev, Yu. A., Ros, E., Pushkarev, A. B., Lister, M. L., Sokolovsky, K. V., Kadler, M., Piner, G., Lähteenmäki, A., Tornikoski, M., Angelakis, E., Krichbaum, T. P., Nestoras, I., Fuhrmann, L, Zensus, J. A., Cassaro, P., Orlati, A., Maccaferri, G., Leto, P., Giroletti, M., Richards, J. L., Max-Moerbeck, W., and Readhead, A. C. S.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1 which includes, among other instruments, MAGIC, VERITAS, Whipple 10-m, Fermi-LAT, RXTE, Swift, GASP-WEBT and VLBA. We find an increase in the fractional variability with energy, while no significant interband correlations of flux changes are found in the acquired data set. The higher variability in the very high energy (>100 GeV, VHE) gamma-ray emission and the lack of correlation with the X-ray emission indicate that the highest-energy electrons that are responsible for the VHE gamma-rays do not make a dominant contribution to the ~1 keV emission. Alternatively, there could be a very variable component contributing to the VHE gamma-ray emission in addition to that coming from the synchrotron self-Compton (SSC) scenarios. The space of SSC model parameters is probed following a dedicated grid-scan strategy, allowing for a wide range of models to be tested and offering a study of the degeneracy of model-to-data agreement in the individual model parameters. We find that there is some degeneracy in both the one-zone and the two-zone SSC scenarios that were probed, with several combinations of model parameters yielding a similar model-to-data agreement, and some parameters better constrained than others. The SSC model grid-scan shows that the flaring activity around 2009 May 22 cannot be modeled adequately with a one-zone SSC scenario, while it can be suitably described within a two-independent-zone SSC scenario. The observation of an electric vector polarization angle rotation coincident with the gamma-ray flare from 2009 May 1 resembles those reported previously for low frequency peaked blazars, hence suggesting that there are many similarities in the flaring mechanisms of blazars with different jet properties., Comment: 33 pages, 15 figures, accepted for publication in A&A. Corresponding authors: Marlene Doert (marlene.doert@tu-dortmund.de) and David Paneque (dpaneque@mppmu.mpg.de)
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- 2016
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222. Top-down modulation of brain responses in spelling error recognition
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Ekaterina Larionova, Zhanna Garakh, and Olga Martynova
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ERP ,Top-down control ,Orthographic decision ,Reading ,Visual word recognition ,Spelling ,Psychology ,BF1-990 - Abstract
The task being undertaken can influence orthographic, phonological and semantic processes. In linguistic research, two tasks are most often used: a task requiring a decision in relation to the presented word and a passive reading task which does not require a decision regarding the presented word. The results of studies using these different tasks are not always consistent. This study aimed to explore brain responses associated with the process of recognition of spelling errors, as well as the influence of the task on this process. Event-related potentials (ERPs) were recorded in 40 adults during an orthographic decision task to determine correctly spelled words and words written with errors that did not change the phonology and during the passive reading. During spelling recognition, the early stages up to 100 ms after the stimulus were automatic and did not depend on the requirements of the task. The amplitude of the N1 component (90–160 ms) was greater in the orthographic decision task, but did not depend on the correct spelling of the word. Late word recognition after 350–500 ms was task dependent, but spelling effects were similar across the two tasks: misspelled words evoked an increase in the amplitude of the N400 component related to lexical and semantic processing regardless of the task. In addition, the orthographic decision task modulated spelling effects, this was reflected in an increase in the amplitude of the P2 component (180–260 ms) for correctly spelled words compared with misspelled words. Thus, our results show that spelling recognition involves general lexico-semantic processes independent of the task. Simultaneously, the orthographic decision task modulates the spelling-specific processes necessary to quickly detect conflicts between orthographic and phonological representations of words in memory.
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- 2023
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223. Exceptional outburst of the blazar CTA 102 in 2012: The GASP-WEBT campaign and its extension
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Larionov, V. M., Villata, M., Raiteri, C. M., Jorstad, S. G., Marscher, A. P., Agudo, I., Smith, P. S., Acosta-Pulido, J. A., Arévalo, M. J., Arkharov, A. A., Bachev, R., Blinov, D. A., Borisov, G., Borman, G. A., Bozhilov, V., Bueno, A., Carnerero, M. I., Carosati, D., Casadio, C., Chen, W. P., Clemens, D. P., Di Paola, A., Ehgamberdiev, Sh. A., Gómez, J. L., González-Morales, P. A, Griñón-Marín, A., Grishina, T. S., Hagen-Thorn, V. A., Ibryamov, S., Itoh, R., Kopatskaya, E. N., Koptelova, E., Lázaro, C., Larionova, E. G., Larionova, L. V., Manilla-Robles, A., Metodieva, Y., Milanova, Yu. V., Mirzaqulov, D. O., Molina, S. N., Morozova, D. A., Nazarov, S. V., Ovcharov, E., Peneva, S., Ros, J. A., Sadun, A. C., Savchenko, S. S., Semkov, E., Sergeev, S. G., Strigachev, A., Troitskaya, Yu. V., and Troitsky, I. S.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
After several years of quiescence, the blazar CTA 102 underwent an exceptional outburst in 2012 September-October. The flare was tracked from gamma-ray to near-infrared frequencies, including Fermi and Swift data as well as photometric and polarimetric data from several observatories. An intensive GASP-WEBT collaboration campaign in optical and NIR bands, with an addition of previously unpublished archival data and extension through fall 2015, allows comparison of this outburst with the previous activity period of this blazar in 2004-2005. We find remarkable similarity between the optical and gamma-ray behaviour of CTA 102 during the outburst, with a time lag between the two light curves of ~1 hour, indicative of co-spatiality of the optical and gamma-ray emission regions. The relation between the gamma-ray and optical fluxes is consistent with the SSC mechanism, with a quadratic dependence of the SSC gamma-ray flux on the synchrotron optical flux evident in the post-outburst stage. However, the gamma-ray/optical relationship is linear during the outburst; we attribute this to changes in the Doppler factor. A strong harder-when-brighter spectral dependence is seen both the in gamma-ray and optical non-thermal emission. This hardening can be explained by convexity of the UV-NIR spectrum that moves to higher frequencies owing to an increased Doppler shift as the viewing angle decreases during the outburst stage. The overall pattern of Stokes parameter variations agrees with a model of a radiating blob or shock wave that moves along a helical path down the jet., Comment: 11 pages, 14 figures, accepted in MNRAS
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- 2016
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224. Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009
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MAGIC Collaboration, Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Banerjee, B., Bangale, P., de Almeida, U. Barres, Barrio, J. A., González, J. Becerra, Bednarek, W., Bernardini, E., Biasuzzi, B., Biland, A., Blanch, O., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Buson, S., Carosi, A., Chatterjee, A., Clavero, R., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Wilhelmi, E. de Oña, Di Pierro, F., Domínguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Einecke, S., Glawion, D. Eisenacher, Elsaesser, D., Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Galindo, D., López, R. J. García, Garczarczyk, M., Terrats, D. Garrido, Gaug, M., Giammaria, P., Godinović, N., Muñoz, A. González, Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hanabata, Y., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Hughes, G., Idec, W., Kodani, K., Konno, Y., Kubo, H., Kushida, J., La Barbera, A., Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., López-Coto, R., Majumdar, P., Makariev, M., Mallot, K., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martínez, M., Mazin, D., Menzel, U., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moretti, E., Nakajima, D., Neustroev, V., Niedzwiecki, A., Rosillo, M. Nievas, Nilsson, K., Nishijima, K., Noda, K., Nogués, L., Orito, R., Overkemping, A., Paiano, S., Palacio, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Paredes-Fortuny, X., Pedaletti, G., Perri, L., Persic, M., Poutanen, J., Moroni, P. G. Prada, Prandini, E., Puljak, I., Rhode, W., Ribó, M., Rico, J., Garcia, J. Rodriguez, Saito, T., Satalecka, K., Schultz, C., Schweizer, T., Shore, S. N., Sillanpää, A., Sitarek, J., Snidaric, I., Sobczynska, D., Stamerra, A., Steinbring, T., Strzys, M., Takalo, L., Takami, H., Tavecchio, F., Temnikov, P., Terzić, T., Tescaro, D., Teshima, M., Thaele, J., Torres, D. F., Toyama, T., Treves, A., Verguilov, V., Vovk, I., Ward, J. E., Will, M., Wu, M. H., Zanin, R., Blinov, D. A., Chen, W. P., Efimova, N. V., Forné, E., Grishina, T. S., Hovatta, T., Jordan, B., Kimeridze, G. N., Kopatskaya, E. N., Koptelova, E., Kurtanidze, O. M., Kurtanidze, S. O., Lähteenmaäki, A., Larionov, V. M., Larionova, E. G., Larionova, L. V., Ligustri, R., Lin, H. C., McBreen, B., Morozova, D. A., Nikolashvili, M. G., Raiteri, C. M., Ros, J. A., Sadun, A. C., Sigua, L. A., Tornikoski, M., Troitsky, I. S., and Villata, M.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We study the multi-band variability and correlations of the TeV blazar Mrk 421 on year time scales, which can bring additional insight on the processes responsible for its broadband emission. We observed Mrk 421 in the very high energy (VHE) gamma-ray range with the Cherenkov telescope MAGIC-I from March 2007 to June 2009 for a total of 96 hours of effective time after quality cuts. The VHE flux variability is quantified with several methods, including the Bayesian Block algorithm, which is applied to data from Cherenkov telescopes for the first time. The 2.3 year long MAGIC light curve is complemented with data from the Swift/BAT and RXTE/ASM satellites and the KVA, GASP-WEBT, OVRO, and Mets\"ahovi telescopes from February 2007 to July 2009, allowing for an excellent characterisation of the multi-band variability and correlations over year time scales. Mrk 421 was found in different gamma-ray emission states during the 2.3 year long observation period. Flares and different levels of variability in the gamma-ray light curve could be identified with the Bayesian Block algorithm. The same behaviour of a quiet and active emission was found in the X-ray light curves measured by Swift/BAT and the RXTE/ASM, with a direct correlation in time. The behaviour of the optical light curve of GASP-WEBT and the radio light curves by OVRO and Mets\"ahovi are different as they show no coincident features with the higher energetic light curves and a less variable emission. The fractional variability is overall increasing with energy. The comparable variability in the X-ray and VHE bands and their direct correlation during both high- and low-activity periods spanning many months show that the electron populations radiating the X-ray and gamma-ray photons are either the same, as expected in the Synchrotron-Self-Compton mechanism, or at least strongly correlated, as expected in electromagnetic cascades., Comment: Corresponding authors: Ann-Kristin Overkemping (ann-kristin.overkemping@tu-dortmund.de), Marina Manganaro (manganaro@iac.es), Diego Tescaro (diego.tescaro@gmail.com), To be published in Astronomy&Astrophysics (A&A), 12 pages, 9 figures
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- 2016
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225. Polarization angle swings in blazars: The case of 3C 279
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Kiehlmann, S., Savolainen, T., Jorstad, S. G., Sokolovsky, K. V., Schinzel, F. K., Marscher, A. P., Larionov, V. M., Agudo, I., Akitaya, H., Benítez, E., Berdyugin, A., Blinov, D. A., Bochkarev, N. G., Borman, G. A., Burenkov, A. N., Casadio, C., Doroshenko, V. T., Efimova, N. V., Fukazawa, Y., Gómez, J. L., Grishina, T. S., Hagen-Thorn, V. A., Heidt, J., Hiriart, D., Itoh, R., Joshi, M., Kawabata, K. S., Kimeridze, G. N., Kopatskaya, E. N., Korobtsev, I. V., Krajci, T., Kurtanidze, O. M., Kurtanidze, S. O., Larionova, E. G., Larionova, L. V., Lindfors, E., López, J. M., McHardy, I. M., Molina, S. N., Moritani, Y., Morozova, D. A., Nazarov, S. V., Nikolashvili, M. G., Nilsson, K., Pulatova, N. G., Reinthal, R., Sadun, A., Sasada, M., Savchenko, S. S., Sergeev, S. G., Sigua, L. A., Smith, P. S., Sorcia, M., Spiridonova, O. I., Takaki, K., Takalo, L. O., Taylor, B., Troitsky, I. S., Uemura, M., Ugolkova, L. S., Ui, T., Yoshida, M., Zensus, J. A., and Zhdanova, V. E.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Over the past few years, several occasions of large, continuous rotations of the electric vector position angle (EVPA) of linearly polarized optical emission from blazars have been reported. These events are often coincident with high energy gamma-ray flares and they have attracted considerable attention, as they could allow one to probe the magnetic field structure in the gamma-ray emitting region of the jet. The flat-spectrum radio quasar 3C279 is one of the most prominent examples showing this behaviour. Our goal is to study the observed EVPA rotations and to distinguish between a stochastic and a deterministic origin of the polarization variability. We have combined multiple data sets of R-band photometry and optical polarimetry measurements of 3C279, yielding exceptionally well-sampled flux density and polarization curves that cover a period of 2008-2012. Several large EVPA rotations are identified in the data. We introduce a quantitative measure for the EVPA curve smoothness, which is then used to test a set of simple random walk polarization variability models against the data. 3C279 shows different polarization variation characteristics during an optical low-flux state and a flaring state. The polarization variation during the flaring state, especially the smooth approx. 360 degrees rotation of the EVPA in mid-2011, is not consistent with the tested stochastic processes. We conclude that during the two different optical flux states, two different processes govern the polarization variation, possibly a stochastic process during the low-brightness state and a deterministic process during the flaring activity., Comment: 19 pages, 15 figures, 6 tables
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- 2016
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226. Functions of long non-coding RNA ROR in patient-derived glioblastoma cells
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Kovalenko, Tatyana F., Yadav, Bhupender, Anufrieva, Ksenia S., Rubtsov, Yury P., Zatsepin, Timofey S., Shcherbinina, Evgenya Y., Solyus, Ekaterina M., Staroverov, Dmitry B., Larionova, Tatyana D., Latyshev, Yaroslav A., Shakhparonov, Michail I., Pandey, Amit Kumar, and Pavlyukov, Marat S.
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- 2022
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227. Characterization of area radioactive contamination of near-surface soil at the Sary-Uzen site in the Semipalatinsk test site
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Krivitskiy, P.Ye., Larionova, N.V., Baklanova, Yu.V., Aidarkhanov, А.O., and Lukashenko, S.N.
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- 2022
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228. Speciation of 137Cs, 90Sr, 241Am, and 239+240Pu artificial radionuclides in soils at the Semipalatinsk test site
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Kunduzbayeva, A.Ye., Lukashenko, S.N., Kabdyrakova, A.M., Larionova, N.V., Magasheva, R.Yu., and Bakirova, G.A.
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- 2022
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229. Radiotherapy resistance: identifying universal biomarkers for various human cancers
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Larionova, Irina, Rakina, Militsa, Ivanyuk, Elena, Trushchuk, Yulia, Chernyshova, Alena, and Denisov, Evgeny
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- 2022
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230. Problems of anti-tuberculosis therapy in patients on hemodialysis
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O. M. Gordeeva, A. M. Tikhonov, S. N. Andreevskaya, E. E. Larionova, and N. L. Karpina
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противотуберкулезная терапия ,гемодиализ ,лекарственная устойчивость мбт ,нежелательные явления ,Diseases of the respiratory system ,RC705-779 - Abstract
The objective: to determine possibility of prescribing and safety of various anti-tuberculosis drugs and their combinations as part of a therapeutic or preventive course of anti-tuberculosis therapy (ATBT) in patients with end-stage chronic kidney disease (CKD) receiving hemodialysis replacement therapy in the settings with high prevalence of drug resistant strains of Mycobacterium tuberculosis.Subjects and Methods. 42 patients receiving hemodialysis replacement therapy were followed-up by Central Tuberculosis Research Institute: of them, 31 (73.8%) had active tuberculosis and 11 (26.2%) had residual post-tuberculous changes in the respiratory organs. During the follow-up, the nature and severity of adverse reactions to anti-tuberculosis drugs were assessed.Results. In the patients with end-stage CKD suffering from respiratory tuberculosis, drug resistant strains prevailed – 68.2%. Some of adverse events developed when taking anti-tuberculosis drugs were as follows: deterioration of uremia in 20.5% of cases, cardiovascular complications – in 17.9%, and neurotoxic reactions – in 15.4%. Progression of uremia occurred more often in the followed-up patients taking anti-tuberculosis drugs versus hepatotoxic reactions (p = 0.02). When treating tuberculosis patients with end-stage CKD, isoniazid was discontinued due to adverse events in 12.8% of cases and pyrazinamide in 12.8% of cases, other drugs were discontinued less frequently. Compilation of individual regimens of anti-tuberculosis drugs with the consideration of drug susceptibility testing results, contraindications, and concomitant diseases made it possible to provide an adequate anti-tuberculosis therapy for patients with end-stage CKD with tuberculosis infection in 92.9% of cases for a period of more than 6 months.
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- 2022
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231. MSCT semiotics of diabetic osteoarthropathy complicated by chronic osteomyelitis
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Galina V. Diachkova, Anatolii S. Sudnitsyn, Nikolai M. Kliushin, Konstantin A. Diachkov, Tatiana A. Larionova, and Ekaterina V. Khieva
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diabetic neuroosteoarthropathy ,chronic osteomyelitis ,msct ,Orthopedic surgery ,RD701-811 - Abstract
Background Conventional radiography, magnetic resonance imaging, nuclear medicine scintigraphy are the imaging techniques currently in use for the evaluation of diabetic neuroosteoarthropathy (DN) with computed tomography being not commonly employed even for cases complicated by chronic osteomyelitis. The objective was to explore MSCT-semiotics of anatomical and radiomorphological changes in foot bones in patients with DN complicated by chronic osteomyelitis (CO) to determine most common manifestations of CO in diabetic foot. Material and methods Single-centre retrospective study. A series of cases. Preoperative radiological findings, MSCT (multislice computed tomography) were examined in 14 patients with DN complicated by chronic osteomyelitis. Results The patients showed impaired structure of the cancellous bone of various severity depending on the nature and localization of foot bone destruction. Overall bone density was higher in cancellous bone of the distal tibia, talus, calcaneus with the local density ranging within significant limits and was maximum at some points of the subchondral tibia and talus and minimum in the intertrabecular areas of the calcaneus and the distal tibia. MSCT scans showed medial calcinosis of the arteries in 5 (35.7 %) from 14 patients. Conclusion MSCT as one of the most objective method for the qualitative and quantitative assessment of the bone is practical for identifying anatomical and topographic relationships of the foot bones and the ankle joint to facilitate reconstructions in three planes and VRT, which is important for assessing the foot in patients with DN complicated by chronic osteomyelitis. The technique allows measurement of the foot bone density in Hounsfield units determining the severity of osteoporosis, the extent of architectonics impairment to facilitate preoperative planning.
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- 2022
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232. Occupational health risk for workers from basic occupational groups employed at copper and zinc ore mining enterprises: Assessment and management
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E.R. Shaykhlislamova, L.K. Karimova, N.A. Beigul, N.A. Muldasheva, A.Z. Fagamova, I.V. Shapoval, A.D. Volgareva, and E.A. Larionova
- Subjects
occupational risk ,workers ,copper-zinc ores ,ore mining ,workers' health ,hygienic and biomedical aspects ,Medicine - Abstract
A great share of workers employed at polymetallic ores mining have to face harmful working conditions at their workplaces. To provide safe working conditions for them and to preserve their health is a vital task occupational medicine has to tackle. Polymetallic ore mining enterprises employ certain common technological processes; nevertheless, there are specific features depending on ore mining techniques and the mineralogical composition of different ores. These features determine differences both in working conditions and in occupational risks of developing occupational morbidity (OM) and work-related morbidity (WRM). By now, there have been enough studies on peculiarities of occupational health risks for workers employed at sulfide ore mines, copper-nickel ore mines and ferruginous quartzite mines. Considerably less attention has been given to assessing occupational risks for workers dealing with mining and processing copper-zinc ores. We performed complex clinical and hygienic examinations at a major copper-zinc ore mining enterprise located in the Southern Urals. The research results gave grounds for determining a category of working conditions, establishing formation peculiarities and the structure of occupational and work-related diseases among workers from various occupational groups. Occupational risks were assessed considering hygienic and medical-biological indicators. We established the highest occupational health risks for shaft sinkers, followed by drilling unit operators, timberers, excavator drivers, load haul dumper (LHD) operators and underground self-propelled machine (USPM) operators. The research results gave grounds for developing a conceptual model of assessing and managing occupational risks in the branch. The urgency of developing and implementing activities aimed at risk mitigation should be determined depending on how validated a risk is and on its rates established for specific occupational groups.
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- 2022
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233. IMPACT MARKETING CAMPAIGNS DOMINANT ENTITIES TELECOMMUNICATIONS ON THE LEVEL OF COMPETITION IN THE REGION
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Natalia A. Larionova and Elena Yu. Shatskaya
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конкуренция ,доминирующий субъект ,маркетинговые акции ,ценовая полити-ка ,рынок телекоммуникаций ,competition ,the dominant subject ,marketing campaigns ,pricing ,telecommunications market ,Economics as a science ,HB71-74 - Abstract
The paper summarizes the results of the authors of the study on the impact of the established tariffs within the marketing activities of the dominant market subject to the level of competition in the region. Studies have shown that marketing actions (including as a tool for retaining existing and attracting new subscribers) made regional operator of information-communication services is the dominant subject in the target market did not lead to a restriction of competition in the region.
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- 2022
234. TECHNICAL POSSIBILITIES OF TELEVISION AS A MEAN OF CREATING VIRTUALITY
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Elena Nikolaevna Larionova
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телевидение ,телевизионный текст ,виртуальность ,виртуальная реальность ,видеосъемка ,освещение ,монтаж ,tv (television) ,television text ,virtuality ,virtual reality ,videoshooting ,lighting ,editing ,Economics as a science ,HB71-74 - Abstract
This article considers the basic techniques for creating television works (videoshooting, lighting, edit- ing), allowing to form the virtual space and virtual time through television text.
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- 2022
235. Giant foam-like macrophages in advanced ovarian cancer
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M. A. Rakina, E. O. Kazakova, T. S. Sudaskikh, N. V. Bezgodova, A. B. Villert, L. A. Kolomiets, and I. V. Larionova
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ovarian neoplasms ,tumor-associated macrophages ,foam-like cells ,receptors ,scavenger ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Introduction. Ovarian cancer (OC) is the third most common gynecological cancer with the worst prognosis and highest mortality rate. The progression of OC can be accompanied by the detrimental functions of the components of the tumor microenvironment, including tumor-associated macrophages (TAMs).The purpose of the study to analyze distribution and morphological phenotype of TAMs in tumor tissue of patients with high-grade serous ovarian cancer (HGSOC).Material and methods. Formalin fixed paraffin embedded tissue sections were obtained from ovarian cancer patients after tumor resection. The protein expression of general macrophage marker CD68 and M2-like markers CD206, CD163 and stabilin-1, belonging to scavenger receptors, was analysed by immunohistochemical staining in tumor tissue. Histological assessment of TAM distribution was performed by pathologist. Immunofluorescent analysis/confocal microscopy was applied to establish the co-expression of CD68 with the main macrophage scavenger receptors.Results. We were able to find giant CD 68-positive macrophages with foamy cytoplasm in ovarian tumor tissue. The accumulation of these tams was specific only for patients with advanced stage (IIIC and IV stages). The presence of foamlike tams had a statistical tendency to be associated with ovarian cancer progression, including metastasis and recurrence. The distribution of stabilin-1-positive macrophages was matched to CD68 expression in almost all cases, as was shown by IHC. Confocal microscopy confirmed that stabilin-1 was expressed in at least 50 % of giant tams. If analysis of tumor samples also demonstrated co-expression of other scavenger receptors, CD163 and CD36, in foam-like cells. Similar to IHC, in most samples the expression of CD206 in tams of foam-like morphology was limited.Conclusion. For the first time we demonstrated the accumulation of giant macrophages with fluffy foam cytoplasm in the tumor tissue of treated patients with advanced ovarian cancer. Such macrophages express diverse scavenger receptors (stabilin-1, CD163, CD 36), thus indicating a high clearance activity of giant TAMs.
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- 2022
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236. Art technologies in the development of students’ emotional intelligence
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L. I. Larionova and L. N. Azarova
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emotional intelligence ,development of students’ emotional intelligence ,art technologies ,art therapy ,art pedagogy ,university education ,professional training ,Science - Abstract
The article presents an overview of domestic research devoted to the development of students’ emotional intelligence by means of art technologies. The relevance of the problem of developing emotional intelligence in modern students is determined by the objectives of higher education. Despite the serious experience gained in Russia in the use of art in teaching and personal education, the active penetration of art technologies into the education system began to occur relatively recently, which explains the time frame of the review study – 2019–2021. The analysis was performed in December 2021 using the national bibliographic database of scientific citation. The research was conducted using such combinations of keywords as “emotional intelligence”, “development of emotional intelligence of students”, “art therapy”, “pedagogical art therapy”, “art technology”, “art therapy at the university” in Russian for the period of 2019–2021. Out of 902 publications devoted to art therapy, the problem of using art technologies in higher education, the development of emotional intelligence through art technologies, the authors selected 49 publications. The analysis of the selected publications showed that the problem of the development of emotional intelligence arouses increased interest among researchers. However, the development of emotional intelligence in students is not a priority. In the system of professional education, the topic of emotional intelligence is not given enough attention, which is unacceptable and does not meet the requirements for the level of training of modern specialists. In recent studies, the possibilities of using art technologies in the development of students’ emotional intelligence have not been sufficiently disclosed. There is a need for further development of a program for the development of students’ emotional intelligence, presentation and description of art therapy techniques and techniques, their place and role in the development of emotional intelligence. Undoubtedly, building up the evidence base and substantiating methods for verifying the effectiveness of various art technologies will be a promising direction.
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- 2022
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237. The detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state
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MAGIC Collaboration, Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Arcaro, C., Baack, D., Babić, A., Banerjee, B., Bangale, P., de Almeida, U. Barres, Barrio, J. A., Bednarek, W., Bernardini, E., Berse, R. Ch., Berti, A., Bhattacharyya, W., Biland, A., Blanch, O., Bonnoli, G., Carosi, R., Carosi, A., Ceribella, G., Chatterjee, A., Colak, S. M., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Cumani, P., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Di Pierro, F., Domínguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Einecke, S., Elsaesser, D., Ramazani, V. Fallah, Fernández-Barral, A., Fidalgo, D., Fonseca, M. V., Font, L., Fruck, C., Galindo, D., López, R. J. García, Garczarczyk, M., Gaug, M., Giammaria, P., Godinović, N., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Ishio, K., Konno, Y., Kubo, H., Kushida, J., dić, D. Kuvež, Lelas, D., Lindfors, E., Lombardi, S., Longo, F., López, M., Maggio, C., Majumdar, P., Makariev, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Masuda, S., Mazin, D., Mielke, K., Minev, M., Miranda, J. M., Mirzoyan, R., Moralejo, A., Moreno, V., Moretti, E., Nagayoshi, T., Neustroev, V., Niedzwiecki, A., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Paiano, S., Palacio, J., Paneque, D., Paoletti, R., Paredes, J. M., Pedaletti, G., Peresano, M., Persic, M., Moroni, P. G. Prada, Prandini, E., Puljak, I., Garcia, J. R., Reichardt, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saito, T., Satalecka, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Stamerra, A., Strzys, M., Surić, T., Takahashi, M., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Treves, A., Tsujimoto, S., Vanzo, G., Acosta, M. Vazquez, Vovk, I., Ward, J. E., Will, M., Zarić, D., González, J. Becerra, Tanaka, Y., Ojha, R., Finke, J., Lähteenmäki, A., Järvelä, E., Tornikoski, M., Ramakrishnan, V., Hovatta, T., Jorstad, S. G., Marscher, A. P., Larionov, V. M., Borman, G. A., Grishina, T. S., Kopatskaya, E. N., Larionova, L. V., Morozova, D. A., Savchenko, S. S., Troitskaya, Yu. V., Troitsky, I. S., Vasilyev, A. A., Agudo, I., Molina, S. N., Casadio, C., Gurwell, M., Carnerero, M. I., Protasio, C., and Pulido, J. A Acosta
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
The very-high-energy (VHE, $\gtrsim 100$ GeV) $\gamma$-ray MAGIC observations of the blazar S4 0954+65, were triggered by an exceptionally high flux state of emission in the optical. This blazar has a disputed redshift of z=0.368 or z$\geqslant$0.45 and an uncertain classification among blazar subclasses. The exceptional source state described here makes for an excellent opportunity to understand physical processes in the jet of S4 0954+65 and thus contribute to its classification. We investigate the multiwavelength (MWL) light curve and spectral energy distribution (SED) of the S4 0954+65 blazar during an enhanced state in February 2015 and put it in context with possible emission scenarios. We collect photometric data in radio, optical, X-ray, and $\gamma$ ray. We study both the optical polarization and the inner parsec-scale jet behavior with 43 GHz data. Observations with the MAGIC telescopes led to the first detection of S4 0954+65 at VHE. Simultaneous data with Fermi-LAT at high energy $\gamma$ ray\ (HE, 100 MeV < E < 100 GeV) also show a period of increased activity. Imaging at 43 GHz reveals the emergence of a new feature in the radio jet in coincidence with the VHE flare. Simultaneous monitoring of the optical polarization angle reveals a rotation of approximately 100$^\circ$. (...) The broadband spectrum can be modeled with an emission mechanism commonly invoked for flat spectrum radio quasars, i.e. inverse Compton scattering on an external soft photon field from the dust torus, also known as external Compton. The light curve and SED phenomenology is consistent with an interpretation of a blob propagating through a helical structured magnetic field and eventually crossing a standing shock in the jet, a scenario typically applied to flat spectrum radio quasars (FSRQs) and low-frequency peaked BL Lac objects (LBL)., Comment: 15 pages, 7 figures, submitted to A&A
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- 2018
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238. Returning to Chekhov
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Zvinyackovskiy, Vladimir, primary, Larionova, Marina, primary, and Bushkanec, Liya, primary
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- 2022
- Full Text
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239. Structural-phase composition of iron-containing high carbon composites with fullerite and graphite obtained by mechanosynthesis
- Author
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Larionova, N.S., Nikonova, R.M., Ul’yanov, A.L., Lad’yanov, V.I., and Kamaeva, L.V.
- Published
- 2022
- Full Text
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240. Dynamic fragmentation in steel cylindrical shells
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Botvina, L.R. and Larionova, A.V.
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- 2022
- Full Text
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241. Nanoheterostructures based on nanosized Prussian blue and its Analogues: Design, properties and applications
- Author
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Guari, Yannick, Cahu, Maëlle, Félix, Gautier, Sene, Saad, Long, Jérôme, Chopineau, Joël, Devoisselle, Jean-Marie, and Larionova, Joulia
- Published
- 2022
- Full Text
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242. Towards 28 %-efficient Si single-junction solar cells with better passivating POLO junctions and photonic crystals
- Author
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Peibst, R., Rienäcker, M., Larionova, Y., Folchert, N., Haase, F., Hollemann, C., Wolter, S., Krügener, J., Bayerl, P., Bayer, J., Dzinnik, M., Haug, R.J., and Brendel, R.
- Published
- 2022
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- View/download PDF
243. 40Ar-39Ar and Rb-Sr age constraints on the formation of Sukhoi-Log-style orogenic gold deposits of the Bodaibo District (Northern Transbaikalia, Russia)
- Author
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Chugaev, Andrey V., Budyak, Alexander E., Larionova, Yulia O., Chernyshev, Igor V., Travin, Alexei V., Tarasova, Yulia I., Gareev, Bulat I., Batalin, Georgii A., Rassokhina, Irina V., and Oleinikova, Tatyana I.
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- 2022
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244. 24.2% efficient POLO back junction solar cell with an AlOx/SiNy dielectric stack from an industrial‐scale direct plasma‐enhanced chemical vapor deposition system.
- Author
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Min, Byungsul, Mertens, Verena, Larionova, Yevgeniya, Pernau, Thomas, Haverkamp, Helge, Dullweber, Thorsten, Peibst, Robby, and Brendel, Rolf
- Subjects
SURFACE passivation ,CHEMICAL vapor deposition ,SILICON nitride ,CELL junctions ,MANUFACTURING processes ,SILICON nitride films - Abstract
An aluminum oxide (AlOx)/silicon nitride (SiNy) dielectric stack was developed using an industrial plasma‐enhanced chemical vapor deposition (PECVD) system with low‐frequency (LF) plasma source for the surface passivation of undiffused textured p‐type crystalline silicon. The median recombination current density is 4.3 fA cm−2 as determined from photoconductance decay lifetime measurements and numerical device modeling. To the best of our knowledge, this is the first time to present a high‐quality LF‐PECVD AlOx/SiNy passivation stack on undiffused textured p‐type crystalline silicon wafers, which are cleaned with industrial processes using HF, HCl, and O3. The simulation agrees well with the measured effective carrier lifetime if the velocity parameters of 5.6 cm s−1 for holes and 803 cm s−1 for electrons are applied with a fixed negative charge density of −3 × 1012 cm−2. The process integration of developed AlOx/SiNy dielectric stack is successfully demonstrated by fabricating p‐type back junction solar cells featuring a poly‐Si‐based passivating contact at the cell rear side. As the best cell efficiency, we achieve 24.2% with an open‐circuit voltage of 725 mV on a M2‐sized Ga‐doped p‐type Czochralski‐grown Si wafer as independently confirmed by ISFH CalTeC. [ABSTRACT FROM AUTHOR]
- Published
- 2025
- Full Text
- View/download PDF
245. INVESTIGATING THE IMPACT OF ARTIFICIAL INTELLIGENCE ON ECONOMIC SECURITY IN THE EUROPEAN UNION.
- Author
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LARIONOVA, Oleksandra
- Abstract
This article examines the dual impact of artificial intelligence (Al) on the EU's economic security, focusing on its opportunities and threats: While Al contributes to economic growth and stability, it also creates new vulnerabilities. The paper discusses the role of Al in fighting economic crime, improving risk management, and fostering innovation. At the same time, it also highlights the risks of Al misuse in cyberattacks and manipulations, as well as potential losses for businesses. The report's conclusions emphasize the need for international cooperation and national cybersecurity strategies to effectively use Al and overcome potential challenges. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF
246. Effect of Powder Preparation of FeNiCoCrMo 0.5 Al 1.3 High-Entropy Alloy on the Phase Composition and Properties of High-Velocity Oxy-Fuel-Sprayed Coatings.
- Author
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Semikolenov, Anton, Mamaev, Nikolay, Larionova, Tatiana, Shalnova, Svetlana, and Tolochko, Oleg
- Subjects
HIGH-entropy alloys ,MECHANICAL alloying ,PROTECTIVE coatings ,OXIDE coating ,ALLOY powders ,POWDER coating ,METAL spraying - Abstract
In this work, the effect of high-entropy alloy powder preparation on the coatings deposited via high-velocity oxygen fuel sprayings was studied. The powders of FeNiCoCrMo
0.5 Al1.3 composition were prepared by milling and gas atomization. The structures, porosity, phase composition, and microhardness of the coatings produced from mechanically alloyed and gas-atomized powders were compared. The influence of milling parameters on the powder phase composition and morphology was studied. Milling at 600 rpm for 1.5 h allowed the production of mechanically alloyed powder with a homogeneous distribution of Fe, Ni, and Al and thin lamellas enriched with Co, Cr, and Mo. Despite the difference in the feedstock powders' phase compositions, the phase compositions of the coatings deposited from mechanically alloyed and gas-atomized powders are the same consisting of BCC, FCC solutions, and oxide. The amount of FCC solutions and oxide in the coating depends on the size distribution of the sprayed powder. It was found that the phase composition and the properties of the coatings deposited from the mechanically alloyed and gas-atomized powders of similar sizes are similar. [ABSTRACT FROM AUTHOR]- Published
- 2024
- Full Text
- View/download PDF
247. Differential retinoic acid sensitivity of oral and pharyngeal teeth in medaka (Oryzias latipes) supports the importance of pouch–cleft contacts in pharyngeal tooth initiation.
- Author
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Larionova, D. and Huysseune, A.
- Subjects
EPIBLAST ,ORYZIAS latipes ,INCISORS ,TOOTH sensitivity ,RESPONSE inhibition - Abstract
Background: Previous studies have claimed that pharyngeal teeth in medaka (Oryzias latipes) are induced independent of retinoic acid (RA) signaling, unlike in zebrafish (Danio rerio). In zebrafish, pharyngeal tooth formation depends on a proper physical contact between the embryonic endodermal pouch anterior to the site of tooth formation, and the adjacent ectodermal cleft, an RA‐dependent process. Here, we test the hypothesis that a proper pouch–cleft contact is required for pharyngeal tooth formation in embryonic medaka, as it is in zebrafish. We used 4‐[diethylamino]benzaldehyde (DEAB) to pharmacologically inhibit RA production, and thus pouch–cleft contacts, in experiments strictly controlled in time, and analyzed these using high‐resolution imaging. Results: Pharyngeal teeth in medaka were present only when the corresponding anterior pouch had reached the ectoderm (i.e., a physical pouch–cleft contact established), similar to the situation in zebrafish. Oral teeth were present even when the treatment started approximately 4 days before normal oral tooth appearance. Conclusions: RA dependency for pharyngeal tooth formation is not different between zebrafish and medaka. We propose that the differential response to DEAB of oral versus pharyngeal teeth in medaka could be ascribed to the distinct germ layer origin of the epithelia involved in tooth formation in these two regions. Key Findings: Pharyngeal tooth formation in medaka depends on the retinoic acid (RA)‐controlled establishment of physical pouch‐cleft contacts.Retinoic acid sensitivity for pharyngeal tooth formation is conserved across teleost fish.Differential response to RA inhibition of oral versus pharyngeal teeth in medaka could be ascribed to the distinct germ layer origin of the epithelia involved. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF
248. Multifunctional Dy 3+ Complexes with Triphenylmethanolates: Structural Diversity, Luminescence, and Magnetic Relaxation.
- Author
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Félix, Gautier, Tolpygin, Aleksei O., Larquey, Aurore, Gogolev, Ilia A., Nelyubina, Yulia V., Guari, Yannick, Larionova, Joulia, and Trifonov, Alexander A.
- Subjects
SINGLE molecule magnets ,MAGNETIC relaxation ,MAGNETIC properties ,ACTIVATION energy ,DYSPROSIUM - Abstract
The coordination environment of magneto-luminescent Dy
3+ -based Single-Molecule Magnets (SMM) is a crucial factor influencing both magnetic and luminescent properties. In this work, we explore how triphenylmethanolate (Ph3 CO− ), in combination with other ligands, can modulate the structure and, therefore, the magnetic properties of Dy3+ -based SMM. Using triphenylmethanolate in combination with THF and pyridine (Py) as co-ligands, we synthesized a series of mononuclear cis-[Dy(OCPh3 )2 (THF)4 ][BPh4 ]·(2,6-Me2 C5 H3 N) (1), trans-Dy(OCPh3 )3 (THF)2 (2), fac-Dy(OCPh3 )3 (py)3 (3) and dinuclear [(Ph3 CO)Dy(THF){(μ2 –Cl)2 Li(THF)2 }μ2 –Cl]2 (4) complexes where the Dy3+ ion presents five- or six-coordinate geometries. Dinuclear compound 4 exhibits a genuine SMM behavior with a relatively high energy barrier of 421 cm−1 , while mononuclear complexes 1–3 are field-induced SMM. These complexes also present Dy3+ -characteristic luminescence, highlighting their multifunctional character. [ABSTRACT FROM AUTHOR]- Published
- 2024
- Full Text
- View/download PDF
249. Transiently elevated expression of different forms of brain-derived neurotrophic factor in the neonatal medial prefrontal cortex affected anxiety and depressive-like behaviors in adolescence.
- Author
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Lanshakov, Dmitriy, Shaburova, Elizaveta, Sukhareva, Ekaterina, Bulygina, Veta, Drozd, Uliana, Larionova, Irina, Gerashchenko, Tatiana, Shnaider, Tatiana, Denisov, Evgeny V., and Kalinina, Tatyana
- Subjects
BRAIN-derived neurotrophic factor ,NEUROBEHAVIORAL disorders ,HEALTH behavior ,NEURONS ,PREFRONTAL cortex ,ADOLESCENCE - Abstract
Brain-derived neurotrophic factor (BDNF) is a secreted molecule that plays an important role in the survival and growth of nerve cells. BDNF undergoes complex post-translational processing with cellular proteases. Pro- and mature BDNF forms bind to different receptor types in the brain. BDNF is prominent in the neonatal cerebral cortex. The neonatal period is critical for the proper development of the brain and nervous system. Disruptions in these critical periods can have long-lasting effects on behavior and mental health. Individuals who experience adverse effects in the neonatal period have demonstrated a predisposition to depression and other neurobehavioral disorders. In this work we studied the influence of transient expression (P3–P8) elevation of pro-, mature and mutant forms of BDNF that could not be processed with cellular convertases in the neonatal medial prefrontal cortex (mPFC) on anxiety and depressive-like behavior in adolescents. Elevated expression of mature BDNF (LV-BDNF) increased anxiety and depressive-like behavior at P30. Only immobility in the tail suspension test was increased after expression of mutant BDNF (LV-pBDNF mut). Using our RNA-seq data and available online sn-RNAseq results, we investigated transcriptomic changes in the neonatal mPFC at P8 that underlie subsequent behavioral changes. Mature BDNF expression caused an increased transcriptional response in perivascular stromal cells (PSC) with such genes: Ptgds, Slc6a13, Slc22a6, Bnc2, Slc13a4, Aldh1a2. Based on GWAS data, Ptgds is a candidate gene associated with ADHD and bipolar disorder Pujol-Gualdo et al. (2021); Marín-Méndez et al. (2012); Munkholm et al. (2015). LV-pBDNF mut caused a complete opposite set of transcriptional changes in the PSC compared to LV-BDNF. The observed similar behavioral phenotype after expression of mature and mutant forms of BDNF together with the detected genes related to bipolar disorder underpinned that Bdnf could play a substantial role in the pathogenesis of this neurobehavioral disorder. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF
250. Multiband Optical Variability of the Blazar 3C 454.3 on Diverse Timescales
- Author
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Karan Dogra, Alok C. Gupta, C. M. Raiteri, M. Villata, Paul J. Wiita, S. O. Kurtanidze, S. G. Jorstad, R. Bachev, G. Damljanovic, C. Lorey, S. S. Savchenko, O. Vince, M. Abdelkareem, F. J. Aceituno, J. A. Acosta-Pulido, I. Agudo, G. Andreuzzi, S. A. Ata, G. V. Baida, L. Barbieri, D. A. Blinov, G. Bonnoli, G. A. Borman, M. I. Carnerero, D. Carosati, V. Casanova, W. P. Chen, Lang Cui, E. G. Elhosseiny, D. Elsaesser, J. Escudero, M. Feige, K. Gazeas, L. E. Gennadievna, T. S. Grishina, Minfeng Gu, V. A. Hagen-Thorn, F. Hemrich, H. Y. Hsiao, M. Ismail, R. Z. Ivanidze, M. D. Jovanovic, T. M. Kamel, G. N. Kimeridze, E. N. Kopatskaya, D. Kuberek, O. M. Kurtanidze, A. Kurtenkov, V. M. Larionov, L. V. Larionova, M. Liao, H. C. Lin, K. Mannheim, A. Marchini, C. Marinelli, A. P. Marscher, D. Morcuende, D. A. Morozova, S. V. Nazarov, M. G. Nikolashvili, D. Reinhart, J. O. Santos, A. Scherbantin, E. Semkov, E. V. Shishkina, L. A. Sigua, A. K. Singh, A. Sota, R. Steineke, M. Stojanovic, A. Strigachev, A. Takey, Amira A. Tawfeek, I. S. Troitskiy, Y. V. Troitskaya, An-Li Tsai, A. A. Vasilyev, K. Vrontaki, Zhongli Zhang, A. V. Zhovtan, N. Zottmann, and Wenwen Zuo
- Subjects
Active galactic nuclei ,Blazars ,Flat-spectrum radio quasars ,Markov chain Monte Carlo ,Relativistic jets ,Supermassive black holes ,Astrophysics ,QB460-466 - Abstract
Due to its peculiar and highly variable nature, the blazar 3C 454.3 has been extensively monitored by the WEBT team. Here, we present for the first time these long-term optical flux and color variability results using data acquired in B , V , R , and I bands over a time span of about two decades. We include data from WEBT collaborators and public archives such as SMARTS, Steward Observatory, and Zwicky Transient Facility. The data are binned and segmented to study the source over this long term when more regular sampling was available. During our study, the long-term spectral variability reveals a redder-when-brighter trend, which, however, stabilizes at a particular brightness cutoff of ∼14.5 mag in the I band, after which it saturates and evolves into a complex state. This trend indicates increasing dominance of jet emission over accretion disk (AD) emission until jet emission completely dominates. Plots of the variation in spectral index (following F _ν ∝ ν ^− ^α ) reveal a bimodal distribution using a one-day binning. These correlate with two extreme phases of 3C 454.3, an outburst or high-flux state and a quiescent or low-flux state, which are respectively jet- and AD-dominated. We have also conducted intraday variability studies of nine light curves and found that six of them are variable. Discrete correlation function analysis between different pairs of optical wave bands peaks at zero lags, indicating cospatial emission in different optical bands.
- Published
- 2024
- Full Text
- View/download PDF
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