Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Sergijenko, O."'
Autor:
Cangemi, F., Hovatta, T., Lindfors, E., Cerruti, M., Becerra-Gonzalez, J., Biteau, J., Boisson, C., Böttcher, M., de Gouveia Dal Pino, E., Dorner, D., Grolleron, G., Lenain, J.-P., Manganaro, M., Max-Moerbeck, W., Morris, P., Nilsson, K., Reis, L. Passos, Romano, P., Sergijenko, O., Tavecchio, F., Vercellone, S., Wagner, S., Zacharias, M., Cherenkov Telescope Array Collaboration
Relativistic jets launched by Active Galactic Nuclei are among the most powerful particle accelerators in the Universe. The emission over the entire electromagnetic spectrum of these relativistic jets can be extremely variable with scales of variabil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::64d2de3ca586e38c1cae30e162ced13a
Autor:
Cangemi, F., Hovatta, T., Grolleron, G., Lenain, J.-P., Manganaro, M., Max-Moerbeck, W., Morris, P., Nilsson, K., Reis, L. Passos, Romano, P., Sergijenko, O., Tavecchio, F., Lindfors, E., Vercellone, S., Wagner, S., Zacharias, M., Cherenkov Telescope Array Collaboration, Cerruti, M., Becerra-Gonzalez, J., Biteau, J., Boisson, C., Böttcher, M., de Gouveia Dal Pino, E., Dorner, D.
Publikováno v:
7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy
7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy, Jul 2022, Barcelona, Spain
7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy, Jul 2022, Barcelona, Spain
Relativistic jets launched by Active Galactic Nuclei are among the most powerful particle accelerators in the Universe. The emission over the entire electromagnetic spectrum of these relativistic jets can be extremely variable with scales of variabil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4875ae190f6b235a2efd55760bb05184
https://bib-pubdb1.desy.de/record/585386
https://bib-pubdb1.desy.de/record/585386
Autor:
Iocco, F., Meyer, M., Doro, M., Hofmann, W., P��rez-Romero, J., Zaharijas, G., Aguirre-Santaella, A., Amato, E., Anguner, E. O., Antonelli, L. A., Ascasibar, Y., Bal��zs, C., Beck, G., Bigongiari, C., Bolmont, J., Bringmann, T., Brown, A. M., Burton, M. G., Chaty, M. Cardillo S., Cotter, G., della Volpe, D., Djannati-Ata��, A., Eckner, C., Emery, G., Fedorova, E., Filipovic, M. D., Galanti, G., Gammaldi, V., Pino, E. M. de Gouveia Dal, Granot, J., Green, J. G., Hayashi, K., Hern��ndez-Cadena, S., Hiroshima, N., Hnatyk, B., Horan, D., H��tten, M., Jamrozy, M., Kohri, K., Lamastra, A., Lenain, J. -P., Lindfors, E., Liodakis, I., Lombardi, S., Longo, F., Lucarelli, F., Martinez, M., Mart��nez-Huerta, H., Mazin, D., Moralejo, A., Morselli, A., Mundell, C. G., Ong, R. A., Poireau, V., Reimer, O., Rico, J., Romeo, G., Romano, P., Rowell, G., Sadeh, I., S��nchez-Conde, M. A., Saturni, F. G., Sergijenko, O., Sol, H., Stamerra, A., Stolarczyk, Th., Tavecchio, F., Vercellone, S., Testa, V., Tibaldo, L., Vecchi, M., Viana, A., Vitale, V., Zhdanov, V.
Astrophysical observations provide strong evidence that more than 80% of all matter in the Universe is in the form of dark matter (DM). Two leading candidates of particles beyond the Standard Model that could constitute all or a fraction of the DM co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74e968f813045b9587184dd1efdfdb04
https://hal.science/hal-03267320
https://hal.science/hal-03267320
Autor:
Boisson, C., Brown, A. M., Burtovoi, A., Cerruti, M., Chernyakova, M., Hassan, T., Lenain, J.-P., Manganaro, M., Romano, P., Sol, H., Tavecchio, F., Vercellone, S., Zampieri, L., Zanin, R., Zech, A., Agudo, I., Alves Batista, R., Anguner, E. O., Antonelli, L. A., Backes, M., Balazs, C., Becerra Gonz��lez, J., Bigongiari, C., Bissaldi, E., Bolmont, J., Bordas, P., Bo��njak, ��., B��ttcher, M., Burton, M., Cangemi, F., Caraveo, P., Cardillo, M., Caroff, S., Carosi, A., Casanova, S., Chaty, S., Contreras, J. L., Coelho, J. G., Cotter, G., D'A��, A., D'Ammando, F., de Gouveia Dal Pino, E. M., de Martino, D., Delgado, C., della Volpe, D., Djannati-Ata��, A., Anjos, R. C. Dos, Wilhelmi, E. de O��a, Dwarkadas, V., Emery, G., Fedorova, E., Fegan, S., Filipovic, M. D., Galanti, G., Gasparrini, D., Ghirlanda, G., Goldoni, P., Granot, J., Green, J. G., Heller, M., Hnatyk, B., Hnatyk, R., Horan, D., Hovatta, T., Inoue, S., Jamrozy, M., Kh��lifi, B., Komin, N., Kohri, K., Lamastra, A., La Palombara, N., Lindfors, E., Liodakis, I., Lombardi, S., Longo, F., Lucarelli, F., Luque-Escamilla, P. L., Marti, J., Martinez, M., Mazin, D., Mbarubucyeye, J. D., Menchiari, S., Mohrmann, L., Montaruli, T., Moralejo Olaizola, A., Morcuende, D., Morlino, G., Morselli, A., Mundell, C. G., Murach, T., Nagai, A., Nayerhoda, A., Niemiec, J., Nikolajuk, M., Olmi, B., Orienti, M., Paredes, J. M., Pareschi, G., Pe'er, A., P��hlhofer, G., Punch, M., Reimer, O., Rib��, M., Rieger, F., Rodriguez, G., Rodriguez, J., Romeo, G., Roncadelli, M., Rowell, G., Rudak, B., Sadeh, I., Salesa Greus, F., Sawangwit, U., Sch��ssler, F., Sergijenko, O., Shellard, R. C., Saturni, F. G., Stamerra, A., Stolarczyk, Th., Tagliaferri, G., Testa, V., Tibaldo, L., Ventura, S., Viana, A., Vink, J., Vitale, V., Vorobiov, S., Wierzcholska, A., Zacharias, M., Zavrtanik, D.
The physics of the non-thermal Universe provides information on the acceleration mechanisms in extreme environments, such as black holes and relativistic jets, neutron stars, supernovae or clusters of galaxies. In the presence of magnetic fields, par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4d58b6d26e29c64e1be7c1e23b78d42f
Autor:
Boisson, C., Brown, A. M., Tavecchio, F., Punch, M., Reimer, O., Ribó, M., Rieger, F., Rodriguez, G., Rodriguez, J., Romeo, G., Roncadelli, M., Rowell, G., Rudak, B., Vercellone, S., Sadeh, I., Salesa Greus, F., Sawangwit, U., Schüssler, F., Sergijenko, O., Shellard, R. C., Saturni, F. G., Stamerra, A., Stolarczyk, Th., Tagliaferri, G., Zampieri, L., Testa, V., Tibaldo, L., Ventura, S., Viana, A., Vink, J., Vitale, V., Vorobiov, S., Wierzcholska, A., Zacharias, M., Zavrtanik, D., Zanin, R., CTA Collaboration, Zech, A., Agudo, I., Alves Batista, R., Anguner, E. O., Antonelli, L. A., Backes, M., Burtovoi, A., Balazs, C., Becerra González, J., Bigongiari, C., Bissaldi, E., Bolmont, J., Bordas, P., Bošnjak, Ž., Böttcher, M., Burton, M., Cangemi, F., Cerruti, M., Caraveo, P., Cardillo, M., Caroff, S., Carosi, A., Casanova, S., Chaty, S., Contreras, J. L., Coelho, J. G., Cotter, G., D'Aì, A., Chernyakova, M., D'Ammando, F., de Gouveia Dal Pino, E. M., de Martino, D., Delgado, C., della Volpe, D., Djannati-Ataï, A., Anjos, R. C. Dos, Wilhelmi, E. de Oña, Dwarkadas, V., Emery, G., Hassan, T., Fedorova, E., Fegan, S., Filipovic, M. D., Galanti, G., Gasparrini, D., Ghirlanda, G., Goldoni, P., Granot, J., Green, J. G., Heller, M., Lenain, J.-P., Hnatyk, B., Hnatyk, R., Horan, D., Hovatta, T., Inoue, S., Jamrozy, M., Khélifi, B., Komin, N., Kohri, K., Lamastra, A., Manganaro, M., La Palombara, N., Lindfors, E., Liodakis, I., Lombardi, S., Longo, F., Lucarelli, F., Luque-Escamilla, P. L., Marti, J., Martinez, M., Mazin, D., Romano, P., Mbarubucyeye, J. D., Menchiari, S., Mohrmann, L., Montaruli, T., Moralejo Olaizola, A., Morcuende, D., Morlino, G., Morselli, A., Mundell, C. G., Murach, T., Sol, H., Nagai, A., Nayerhoda, A., Niemiec, J., Nikolajuk, M., Olmi, B., Orienti, M., Paredes, J. M., Pareschi, G., Pe'er, A., Pühlhofer, G.
Publikováno v:
INSPIRE-HEP
The physics of the non-thermal Universe provides information on the acceleration mechanisms in extreme environments, such as black holes and relativistic jets, neutron stars, supernovae or clusters of galaxies. In the presence of magnetic fields, par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9ba9ab317b71cd57bbf376dd2e47269
http://inspirehep.net/record/1868026
http://inspirehep.net/record/1868026