Zobrazeno 1 - 10
of 10 991
pro vyhledávání: '"A. Jelínek"'
Autor:
Tavernier, Thomas, Jurysek, Jakub, Novotný, Vladimir, Heller, Matthieu, Mandat, Dusan, Pech, Miroslav, Araudo, A., Alispach, C. M., Beshley, V., Blazek, J., Borkowski, J., Boula, S., Bulik, T., Cadoux, F., Casanova, S., Christov, A., Chytka, L., Favre, Y., Gieras, T., Hamal, P., Hrabovsky, M., Jelinek, M., Karas, V., Gibaud, L., Lyard, É., Mach, E., Michal, S., Michalowksi, J., Moderski, R., Montaruli, T., Muthyala, S. R., Muraczewski, A., Nalewajski, K., Nagai, A., Neise, D., Niemiec, J., Nikolajuk, M., Palatka, M., Prouza, M., Rajda, P., Schovanek, P., Seweryn, K., Sliusar, V., Stawarz, L., Strobl, J., Swierk, P., Świerblewski, J., Travnicek, P., Ostrowski, M., Vicha, J., Della Volpe, D., Walter, R., Marek, W., Zagdański, A., Ziȩtara, K.
Publikováno v:
PoS ICRC2023 (2023) 741
SST-1M is a prototype of a single-mirror Small Size Telescope developed by a consortium of institutes from Poland, Switzerland and the Czech Republic. With a wide field of view of 9 degrees, SST-1Ms are designed to detect gamma-rays in the energy ran
Externí odkaz:
http://arxiv.org/abs/2409.18639
Autor:
Alispach, C., Araudo, A., Balbo, M., Beshley, V., Biland, A., Blažek, J., Borkowski, J., Bulik, T., Cadoux, F., Casanova, S., Christov, A., Chudoba, J., Chytka, L., Dědič, P., della Volpe, D., Favre, Y., Garczarczyk, M., Gibaud, L., Gieras, T., Hamal, P., Heller, M., Hrabovský, M., Janeček, P., Jelínek, M., Jílek, V., Juryšek, J., Karas, V., Lacave, B., Lyard, E., Mach, E., Mandát, D., Marek, W., Michal, S., Michałowski, J., Moderski, R., Montaruli, T., Muraczewski, A., Muthyala, S., Müller, A. L., Nagai, A., Nalewajski, K., Neise, D., Niemiec, J., Nikołajuk, M., Novotný, V., Ostrowski, M., Palatka, M., Pech, M., Prouza, M., Rajda, P., Schovanek, P., Seweryn, K., Sliusar, V., Stawarz, Ł., Sternberger, R., Stodulska, M., Świerblewski, J., Świerk, P., Štrobl, J., Tavernier, T., Trávníček, P., Pujadas, I. Troyano, Vícha, J., Walter, R., Zietara, K.
The SST-1M is a Small-Sized Telescope (SST) designed to provide a cost-effective and high-performance solution for gamma-ray astrophysics, particularly for energies beyond a few TeV. The goal is to integrate this telescope into an array of similar in
Externí odkaz:
http://arxiv.org/abs/2409.11310
This paper introduces a framework for synthesizing reactively loaded antennas and antenna arrays. The framework comprises two main components: computing the fundamental bound using the semi-definite relaxation and finding a realizable solution via op
Externí odkaz:
http://arxiv.org/abs/2409.06291
This paper introduces a computational approach to identify performance constraints in the time-domain based on optimizing the excitation waveform. The method builds on an optimization algorithm that has been employed for decades to establish fundamen
Externí odkaz:
http://arxiv.org/abs/2409.16293
Autor:
Calvo-Fernández, Aitor, Kumar, Manish, Soler-Polo, Diego, Eiguren, Asier, Blanco-Rey, María, Jelínek, Pavel
The mechanism of Kondo screening in strongly correlated molecules with several unpaired electrons on a metal surface is still under debate. Here, we provide a theoretical framework that rationalizes the emergence of Kondo screening involving several
Externí odkaz:
http://arxiv.org/abs/2405.15958
Autor:
Valtonen, Mauri J., Zola, Staszek, Gupta, Alok C., Kishore, Shubham, Gopakumar, Achamveedu, Jorstad, Svetlana G., Wiita, Paul J., Gu, Minfeng, Nilsson, Kari, Marscher, Alan P., Zhang, Zhongli, Hudec, Rene, Matsumoto, Katsura, Drozdz, Marek, Ogloza, Waldemar, Berdyugin, Andrei V., Reichart, Daniel E., Mugrauer, Markus, Dey, Lankeswar, Pursimo, Tapio, Lehto, Harry J., Ciprini, Stefano, Nakaoka, T., Uemura, M., Imazawa, Ryo, Zejmo, Michal, Kouprianov, Vladimir V., Davidson, Jr., James W., Sadun, Alberto, Strobl, Jan, Weaver, Z. R., Jelinek, Martin
We report the study of a huge optical intraday flare on November 12, 2021, at 2 am UT, in the blazar OJ287. In the binary black hole model it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifreq
Externí odkaz:
http://arxiv.org/abs/2405.08627
Trapping of charge at surface states is a longstanding problem in GaN that hinders a full realization of its potential as a semiconductor for microelectronics. At least part of this charge originates in molecules adsorbed on the GaN surface. Multiple
Externí odkaz:
http://arxiv.org/abs/2405.06471
Autor:
Tajuelo-Castilla, Guillermo, Mendieta-Moreno, Jesús I., Accolla, Mario, Sobrado, Jesús M., Canola, Sofia, Jelínek, Pavel, Ellis, Gary J., Martín-Gago, José Ángel, Santoro, Gonzalo
Ultraviolet (UV) processing in the insterstellar medium (ISM) induces the dehydrogenation of hydrocarbons. Aliphatics, including alkanes, are present in different interstellar environments, being prevalently formed in evolved stars; thus, the dehydro
Externí odkaz:
http://arxiv.org/abs/2403.08452
Autor:
Howil, K., Wyrzykowski, Ł., Kruszyńska, K., Zieliński, P., Bachelet, E., Gromadzki, M., Mikołajczyk, P. J., Kotysz, K., Jabłońska, M., Kaczmarek, Z., Mróz, P., Ihanec, N., Ratajczak, M., Pylypenko, U., Rybicki, K., Sweeney, D., Hodgkin, S. T., Larma, M., Carrasco, J. M., Burgaz, U., Godunova, V., Simon, A., Cusano, F., Jelinek, M., Štrobl, J., Hudec, R., Merc, J., Kučáková, H., Erece, O., Kilic, Y., Olivares, F., Morrell, M., Wicker, M.
Identifying black holes is essential for comprehending the development of stars and uncovering novel principles of physics. Gravitational microlensing provides an exceptional opportunity to examine an undetectable population of black holes in the Mil
Externí odkaz:
http://arxiv.org/abs/2403.09006
Autor:
Fernández, J. F. Agüí, Postigo, A. de Ugarte, Thöne, C. C., Kobayashi, S., Rossi, A., Toma, K., Jelínek, M., Kann, D. A., Covino, S., Wiersema, K., Hartmann, D., Jakobsson, P., Martin-Carrillo, A., Melandri, A., De Pasquale, M., Pugliese, G., Savaglio, S., Starling, R. L. C., Štrobl, J., Della Valle, M., de Wet, S., Zafar, T.
Publikováno v:
A&A 690, A216 (2024)
Long gamma ray bursts (GRBs) are produced by the collapse of some very massive stars, which emit ultra-relativistic jets. When the jets collide with the interstellar medium they decelerate and generate the so-called afterglow emission, which has been
Externí odkaz:
http://arxiv.org/abs/2403.02312