Zobrazeno 1 - 10
of 273
pro vyhledávání: '"A. Porelli"'
Autor:
Berlea, Vlad Dumitru, Asif, Arooj, Barschke, Merlin F., Berge, David, Crespo, Juan Maria Haces, Giavitto, Gianluca, Kumar, Shashank, Porelli, Andrea, de Simone, Nicola, Watson, Jason, Worm, Steven, Zappon, Francesco, Birman, Adi, Alfassi, Shay, Feningstein, Amos, Waxman, Eli, Netzer, Udi, Liran, Tuvia, Lapid, Ofer, Algranatti, Viktor M., Schvartzvald, Yossi
ULTRASAT (ULtra-violet TRansient Astronomy SATellite) is a wide-angle space telescope that will perform a deep time-resolved all-sky survey in the near-ultraviolet (NUV) spectrum. The science objectives are the detection of counterparts to short-live
Externí odkaz:
http://arxiv.org/abs/2407.03789
Autor:
M. Tluczykont, M. Brückner, N. Budnev, O. Chvalaev, A. Dyachok, S. Epimakhov, O. Gress, D. Hampf, D. Horns, A. Ivanova, N. Kalmykov, E. Konstantinov, E. Korosteleva, V. Kozin, M. Kunnas, L. Kuzmichev, B. Lubsandorzhiev, R. Mirgazov, R. Monkhoev, R. Nachtigall, M. Panasyuk, A. Pakhorukov, V. Poleschuk, A. Porelli, V. Prosin, V. Ptuskin, G. I. Rubtsov, P. S. Satunin, Yu. Semeney, D. Spitschan, A. Skukhin, L. Sveshnikova, R. Wischnewski, A. Zagorodnikov, V. Zirakashvili
Publikováno v:
Acta Polytechnica CTU Proceedings, Vol 1, Iss 1, Pp 283-287 (2014)
A central question of Astroparticle Physics, the origin of cosmic rays, still remains unsolved. HiSCORE (Hundred*i Square-km Cosmic ORigin Explorer) is a concept for a large-area wide-angle non-imaging air shower detector, addressing this question by
Externí odkaz:
https://doaj.org/article/a903734ee1b548eeaf173c881408bb0f
Autor:
Blank, M., Tluczykont, M., Porelli, A., Mirzoyan, R., Wischnewski, R., Awad, A. K., Brueckner, M.
The Tunka Advanced Instrument for Gamma- and cosmic-ray Astronomy (TAIGA) is a multicomponent experiment for the measurement of TeV to PeV gamma- and cosmic rays. Our goal is to establish a novel hybrid direct air shower technique, sufficient to acce
Externí odkaz:
http://arxiv.org/abs/2301.11002
Autor:
Ben-Ami, Sagi, Shvartzvald, Yossi, Waxman, Eli, Netzer, Udi, Yaniv, Yoram, Algranatti, Viktor M., Gal-Yam, Avishay, Lapid, Ofer, Ofek, Eran, Topaz, Jeremy, Arcavi, Iair, Asif, Arooj, Azaria, Shlomi, Bahalul, Eran, Barschke, Merlin F., Bastian-Querner, Benjamin, Berge, David, Berlea, Vlad D., Buhler, Rolf, Dittmar, Louise, Gelman, Anatoly, Giavitto, Gianluca, Guttman, Or, Crespo, Juan M. Haces, Heilbrunn, Daniel, Kachergincky, Arik, Kaipachery, Nirmal, Kowalski, Marek, Kulkarni, Shrinivasrao R., Kumar, Shashank, Kusters, Daniel, Liran, Tuvia, Miron-Salomon, Yonit, Mor, Zohar, Nir, Aharon, Nitzan, Gadi, Philipp, Sebastian, Porelli, Andrea, Sagiv, Ilan, Schliwinski, Julian, Sprecher, Tuvia, De Simone, Nicola, Stern, Nir, Stone, Nicholas C., Trakhtenbrot, Benny, Vasilev, Mikhail, Watson, Jason J., Zappon, Francesco
The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is a space-borne near UV telescope with an unprecedented large field of view (200 sq. deg.). The mission, led by the Weizmann Institute of Science and the Israel Space Agency in collaboration w
Externí odkaz:
http://arxiv.org/abs/2208.00159
Autor:
Berlea, Vlad D., Asif, Arooj, Barschke, Merlin F., Berge, David, Crespo, Juan Maria Haces, Giavitto, Gianluca, Kumar, Shashank, Porelli, Andrea, Simone, Nicola de, Watson, Jason, Worm, Steven, Zappon, Francesco, Birman, Adi, Alfassi, Shay, Fenigstein, Amos, Waxman, Eli, Netzer, Udi, Liran, Tuvia, Lapid, Ofer, Algranatti, Viktor M., Shvartzvald, Yossi
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A November 2024 1068
Autor:
Panov, A. D., Astapov, I. I., Awad, A. K., Beskin, G. M., Bezyazeekov, P. A., Blank, M., Bonvech, E. A., Borodin, A. N., Bruckner, M., Budnev, N. M., Bulan, A. V., Chernov, D. V., Chiavassa, A., Dyachok, A. N., Gafarov, A. R., Garmash, A. Yu., Grebenyuk, V. M., Gress, O. A., Gress, T. I., Grinyuk, A. A., Grishin, O. G., Horns, D., Ivanova, A. L., Kalmykov, N. N., Kindin, V. V., Kiryuhin, S. N., Kokoulin, R. P., Kompaniets, K. G., Korosteleva, E. E., Kozhin, V. A., Kravchenko, E. A., Krivopalova, A. A., Kuzmichev, L. A., Kryukov, A. P., Lagutin, A. A., Lavrova, M. V., Lemeshev, Yu., Lubsandorzhiev, B. K., Lubsandorzhiev, N. B., Lukanov, A. D., Mirgazov, R. R., Mirzoyan, R., Monkhoev, R. D., Osipova, E. A., Pakhorukov, A. L., Pan, A., Pankov, L. V., Petrukhin, A. A., Podgrudkov, D. A., Poleschuk, V. A., Popova, E. G., Porelli, A., Postnikov, E. B., Prosin, V. V., Ptuskin, V. S., Pushnin, A. A., Raikin, R. I., Razumov, A., Rjabov, E., Rubtsov, G. I., Sagan, Y. I., Samoliga, V. S., Sidorenkov, A. Yu., Silaev, A. A., Skurikhin, A. V., Satyshev, I., Sokolov, A. V., Suvorkin, Y., Sveshnikova, L. G., Tabolenko, V. A., Tanaev, A. B., Tarashansky, B. A., Ternovoy, M., Tkachev, L. G., Tluczykont, M., Ushakov, N., Vaidyanathan, A., Volchugov, P. A., Volkov, N. V., Voronin, D., Wischnewski, R., Yashin, I. I., Zagorodnikov, A. V., Zhurov, D. P.
Publikováno v:
Physics of Atomic Nuclei volume 84, pages 1037-1044 (2021)
A wide-angle Cerenkov array TAIGA-HiSCORE (FOV $\sim$0.6 sr), was originally created as a part of TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. Array now consist on nearly 100 optical stations on the area of 1 km$^2$.
Externí odkaz:
http://arxiv.org/abs/2109.09637
Autor:
Kostunin, D., Astapov, I., Bezyazeekov, P., Borodin, A., Budnev, N., Brückner, M., Chiavassa, A., Dyachok, A., Fedorov, O., Gafarov, A., Garmash, A., Grebenyuk, V., Gress, O., Gress, T., Grishin, O., Grinyuk, A., Haungs, A., Horns, D., Huege, T., Ivanova, A., Kalmykov, N., Kazarina, Y., Kindin, V., Kirilenko, P., Kiryuhin, S., Kleifges, M., Kokoulin, R., Kompaniets, K., Korosteleva, E., Kozhin, V., Kravchenko, E., Kuzmichev, A. Kryukov L., Lemeshev, Yu., Lagutin, A., Lenok, V., Lubsandorzhiev, B., Lubsandorzhiev, N., Marshalkina, T., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Osipova, E., Pakhorukov, A., Pan, A., Panasyuk, M., Pankov, L., Petrukhin, A., Poleschuk, V., Popescu, M., Popova, E., Porelli, A., Postnikov, E., Prosin, V., Ptuskin, V., Pushnin, A., Raikin, R., Ryabov, E., Rubtsov, G., Sagan, Y., Sabirov, B., Samoliga, V., Semeney, Yu., Schröder, F. G., Silaev, A., Sidorenkov, A., Skurikhin, A., Slunecka, V., Sokolov, A., Spiering, C., Sveshnikova, L., Tabolenko, V., Tarashansky, B., Tkachev, L., Tluczykont, M., Ushakov, N., Volchugov, A. Vaidyanathan P., Voronin, D., Wischnewski, R., Zagorodnikov, A., Zhurov, D., Zurbanov, V., Yashin, I.
The paper is a script of a lecture given at the ISAPP-Baikal summer school in 2018. The lecture gives an overview of the Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA) facility including historical introduction, description of
Externí odkaz:
http://arxiv.org/abs/1903.07460
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Autor:
Budnev, N., Astapov, I.I., Bezyazeekov, P.A., Borodin, A., Brückner, M., Chernykh, D., Chiavassa, A., Dyachok, A., Fedorov, O., Gafarov, A., Garmash, A., Grebenyuk, V., Gress, O., Gress, T., Grinyuk, A., Grishin, O., Horns, D., Ivanova, A., Kalmykov, N., Kazarina, Yu., Kindin, V., Kiryuhin, S., Kokoulin, R., Komponiets, K., Korosteleva, E., Kostunin, D., Kozhin, V., Kravchenko, E., Kryukov, A., Kuzmichev, L., Lagutin, A., Lubsandorzhiev, B., Lubsandorzhiev, N., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Osipova, E., Pakhorukov, A., Pan, A., Panasyuk, M., Pankov, L., Petrukhin, A., Poleschuk, V., Popesku, M., Popova, E., Porelli, A., Postnikov, E., Prosin, V., Ptuskin, V., Pushnin, A., Raikin, R., Rubtsov, G., Ryabov, E., Sagan, Y., Samoliga, V., Silaev, A., Silaev, A., junior, Sidorenkov, A., Skurikhin, A., Slunecka, M., Sokolov, A., Spiering, C., Sveshnikova, L., Suvorkin, Y., Tabolenko, V., Tarashchansky, B., Tkachev, L., Tluczykont, M., Ushakov, N., Ustinov, K., Vaidyanathan, A., Voronin, D., Wischnewski, R., Zagorodnikov, A., Zurbanov, V., Zhurov, D., Yashin, I.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 April 2020 958
Autor:
Kuzmichev, L., Astapov, I., Bezyazeekov, P., Borodin, A., Brückner, M., Budnev, N., Chiavassa, A., Gress, O., Gress, T., Grishin, O., Dyachok, A., Fedorov, O., Gafarov, A., Garmash, A., Grebenyuk, V., Grinyuk, A., Horns, D., Kalmykov, N., Kazarina, Y., Kindin, V., Kiryuhin, V., Kirilenko, P., Kokoulin, R., Kompaniets, K., Korosteleva, E., Kozhin, V., Kravchenko, E., Kryukov, A., Lagutin, A., Lenok, V., Lubsandorzhiev, B., Lubsandorzhiev, N., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Osipova, E., Pakharukov, A., Pan, A., Panasyuk, M., Pankov, L., Petrukhin, A., Poleschuk, V., Popesku, M., Popova, E., Porelli, A., Postnikov, E., Prosin, V., Ptuskin, V., Pushnin, A., Raikin, R., Rubtsov, G., Ryabov, E., Sagan, Y., Samoliga, V., Semeney, Yu., Silaev, A., Silaev, A., Jr., Sidorenkov, A., Skurikhin, A., Slunecka, M., Sokolov, A., Spiering, C., Sveshnikova, L., Tabolenko, V., Tarashansky, B., Tkachenko, A., Tkachev, L., Tluczykont, M., Ushakov, N., Voronin, D., Wischnewski, R., Zagorodnikov, A., Zhurov, D., Zurbanov, V., Yashin, I.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 February 2020 952