Zobrazeno 1 - 10
of 284
pro vyhledávání: '"Araudo, AT"'
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
Publikováno v:
IOP Conference Series 2024
Cosmic rays are charged particles that are accelerated to relativistic speeds by astrophysical shocks. Numerical models have been successful in confirming the acceleration process for (quasi-)parallel shocks, which have the magnetic field aligned wit
Externí odkaz:
http://arxiv.org/abs/2407.05847
Astrophysical shocks create cosmic rays by accelerating charged particles to relativistic speeds. However, the relative contribution of various types of shocks to the cosmic ray spectrum is still the subject of ongoing debate. Numerical studies have
Externí odkaz:
http://arxiv.org/abs/2308.12721
Autor:
Jurysek, J., Tavernier, T., Novotný, V., Heller, M., Mandat, D., Pech, M., Alispach, C., Araudo, A., Beshley, V., Blazek, J., Borkowski, J., Boula, S., Bulik, T., Cadoux, F., Casanova, S., Christov, A., Chytka, L., della Volpe, D., Favre, Y., Gibaud, L., Gieras, T., Hamal, P., Hrabovsky, M., Jelínek, M., Karas, V., Lyard, E., Mach, E., Marek, W., Michal, S., Michałowski, J., Moderski, R., Montaruli, T., Muraczewski, A., Muthyala, S. R., Nagai, A., Nalewajski, K., Neise, D., Niemiec, J., Nikołajuk, M., Ostrowski, M., Palatka, M., Prouza, M., Rajda, P., Schovanek, P., Seweryn, K., Sliusar, V., Stawarz, Ł., Świerblewski, J., Świerk, P., Štrobl, J., Vícha, J., Walter, R., Zagdański, A., Zietara, K.
The Single-Mirror Small-Sized Telescope, or SST-1M, was originally developed as a prototype of a small-sized telescope for CTA, designed to form an array for observations of gamma-ray-induced atmospheric showers for energies above 3 TeV. A pair of SS
Externí odkaz:
http://arxiv.org/abs/2307.09799
Autor:
Müller, Ana Laura, Naddaf, Mohammad-Hassan, Zajaček, Michal, Czerny, Bożena, Araudo, Anabella, Karas, Vladimír
The spectra of active galactic nuclei exhibit broad-emission lines that presumably originate in the Broad-Line Region (BLR) with gaseous-dusty clouds in a predominantly Keplerian motion around the central black hole. Signatures of both inflow and out
Externí odkaz:
http://arxiv.org/abs/2204.05361
The termination regions of non-relativistic jets in protostars and supersonic outflows in classical novae are nonthermal emitters. Given the high densities in these systems, radiative shocks are expected to form. However, in the presence of high velo
Externí odkaz:
http://arxiv.org/abs/2201.01696
Autor:
Araudo, A., Carosi, A., Hofmann, W., Iocco, F., Lenain, J. -P., Lindfors, E., Lopez, A., Meyer, M., Morlino, G., Olmi, B., Romano, P., Santander, M., Tibaldo, L., Zanin, R.
Feedback on the ASTRONET Science Vision and Infrastructure Roadmap from the CTA Consortium.
Comment: Submitted as input to the ASTRONET Science Vision and Infrastructure roadmap on behalf of the CTA consortium
Comment: Submitted as input to the ASTRONET Science Vision and Infrastructure roadmap on behalf of the CTA consortium
Externí odkaz:
http://arxiv.org/abs/2106.08952
Autor:
Araudo, A., Morlino, G., Olmi, B., Acero, F., Agudo, I., Adam, R., Batista, R. Alves, Amato, E., Anguner, E. O., Antonelli, L. A., Ascasibar, Y., Balazs, C., Tjus, J. Becker, Bigongiari, C., Bissaldi, E., Bolmont, J., Boisson, C., Bordas, P., Bošnjak, Ž., Brown, A. M., Burton, M., Bucciantini, N., Cangemi, F., Caraveo, P., Cardillo, M., Caroff, S., Casanova, S., Chaty, S., Chernyakova, M., Coelho, J. G., Conte, F., Cotter, G., Crestan, S., D'Aì, A., Pino, E. M. de Gouveia Dal, Delgado, C., della Volpe, D., de Martino, D., Djannati-Ataï, A., Anjos, R. C. Dos, Dwarkadas, V., Emery, G., Fedorova, E., Filipovic, M. D., Fornieri, O., Galanti, G., Gasparrini, D., Ghirlanda, G., Giuliani, A., Goldoni, P., Granot, J., Grasso, D., Wilhelmi, E. de Oña, Khélifi, B., Heller, M., Horan, D., Hnatyk, B., Hnatyk, R., Inoue, S., Jamrozy, M., Komin, N., Lamastra, A., La Palombara, N., Lenain, J. -P., Liodakis, I., Lombardi, S., Longo, F., Lòpez-Oramas, A., Lòpez-Moya, M., Lucarelli, F., Luque-Escamilla, P. L., Majumdar, P., Marcowith, A., Martì, J., Martinez, M., Mazin, D., Menchiari, S., Mohrmann, L., Montaruli, T., Morselli, A., Mundell, C. G., Murach, T., Nagai, A., Nayerhoda, A., Niemiec, J., Nikolajuk, M., Ong, R. A., Paredes, J. M., Pareschi, G., Pohl, M., Pühlhofer, G., Punch, M., Reimer, O., Ribò, M., Rieger, F., Rodriguez, G., Rowell, G., Romano, P., Roncadelli, M., Romeo, G., Rudak, B., Greus, F. Salesa, Saturni, F. G., Sawangwit, U., Schüssler, F., Sergijenko, O., Sol, H., Stamerra, A., Stolarczyk, T., Tagliaferri, G., Tavecchio, F., Testa, V., Tibaldo, L., Viana, A., Vercellone, S., Ventura, S., Vink, J., Vorobiov, S., Vitale, V., Sadeh, I., Sharma, P., Shellard, R. C., Suomijärvi, T., Wierzcholska, A.
This white paper briefly summarizes the importance of the study of relativistic cosmic rays, both as a constituent of our Universe, and through their impact on stellar and galactic evolution. The focus is on what can be learned over the coming decade
Externí odkaz:
http://arxiv.org/abs/2106.03599
Synchrotron radio emission from non-relativistic jets powered by massive protostars has been reported, indicating the presence of relativistic electrons and magnetic fields of strength ~0.3-5 mG. We study diffusive shock acceleration and magnetic fie
Externí odkaz:
http://arxiv.org/abs/2102.11583