Search Results - "Konstantinov, E.N."

The prototyping/early construction phase of the BAIKAL-GVD project by Avrorin, A.D., Avrorin, A.V., Aynutdinov, V.M., Bannasch, R., Belolaptikov, I.A., Bogorodsky, D.Yu, Brudanin, V.B., Budnev, N.M., Danilchenko, I.A., Domogatsky, G.V., Doroshenko, A.A., Dyachok, A.N., Dzhilkibaev, Zh-A.M., Fialkovsky, S.V., Gafarov, A.R., Gaponenko, O.N., Golubkov, K.V., Gress, T.I., Honz, Z., Kebkal, K.G., Kebkal, O.G., Konishchev, K.V., Konstantinov, E.N., Korobchenko, A.V., Koshechkin, A.P., Koshel, F.K., Kozhin, V.A., Kulepov, V.F., Kuleshov, D.A., Ljashuk, V.I., Lolenko, A.I., Milenin, M.B., Mirgazov, R.A., Osipova, E.R., Panfilov, A.I., Pan’kov, L.V., Perevalov, A.A., Pliskovsky, E.N., Poleshuk, V.A., Rozanov, M.I., Rubtsov, V.F., Rjabov, E.V., Shaybonov, B.A., Sheifler, A.A., Skurikhin, A.V., Smagina, A.A., Suvorova, O.V., Tarashchansky, B.A., Yakovlev, S.A., Zagorodnikov, A.V., Zhukov, V.A., Zurbanov, V.L.

“…The prototyping phase of the BAIKAL-GVD project has been started in April 2011 with the deployment of a three string engineering array which comprises all…”
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Status and perspectives of the BAIKAL-GVD project by Avrorin, A.D., Avrorin, A.V., Aynutdinov, V.M., Bannash, R., Belolaptikov, I.A., Bogorodsky, D.Yu, Brudanin, V.B., Budnev, N.M., Danilchenko, I.A., Domogatsky, G.V., Doroshenko, A.A., Dyachok, A.N., Dzhilkibaev, Zh.-A.M., Fialkovsky, S.V., Gafarov, A.R., Gaponenko, O.N., Golubkov, K.V., Gress, T.I., Honz, Z., Kebkal, K.G., Kebkal, O.G., Konischev, K.V., Konstantinov, E.N., Korobchenko, A.V., Koshechkin, A.P., Koshel, F.K., Kozhin, A.V., Kulepov, V.F., Kuleshov, D.A., Ljashuk, V.I., Milenin, M.B., Mirgazov, R.A., Osipova, E.R., Panfilov, A.I., Pan'kov, L.V., Perevalov, A.A., Pliskovsky, E.N., Rozanov, M.I., Rubtzov, V.Yu, Rjabov, E.V., Shaybonov, B.A., Sheifler, A.A., Skurihin, A.V., Smagina, A.A., Suvorova, O.V., Tabolenko, V.A., Tarashansky, B.A., Yakovlev, S.A., Zagorodnikov, A.V., Zhukov, V.A., Zurbanov, V.L.

“…The neutrino telescope Baikal-GVD in Lake Baikal will be a research infrastructure aimed mainly at studying astrophysical neutrino fluxes. The telescope will…”
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Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype by Prosin, V.V., Berezhnev, S.F., Budnev, N.M., Brückner, M., Chiavassa, A., Chvalaev, O.A., Dyachok, A.V., Epimakhov, S.N., Gafarov, A.V., Gress, O.A., Gress, T.I., Horns, D., Kalmykov, N.N., Karpov, N.I., Kiryuhin, S.N., Konstantinov, E.N., Korobchenko, A.V., Korosteleva, E.E., Kozhin, V.A., Kunnas, M., Kuzmichev, L.A., Lubsandorzhiev, B.K., Lubsandorzhiev, N.B., Mirgazov, R.R., Monkhoev, R.D., Nachtigall, R., Osipova, E.A., Pakhorukov, A.L., Panasyuk, M.I., Pankov, L.V., Poleschuk, V.A., Popova, E.G., Porelli, A., Ptuskin, V.S., Rubtsov, G.I., Rüger, M., Samoliga, V.S., Semeney, Y.A., Silaev, A.A., Silaev, A.A., Skurikhin, A.V., Spiering, C., Sveshnikova, L.G., Tluczykont, M., Wischnewski, R., Zagorodnikov, A.V., Zurbanov, A.V.

“…Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenkov light array for registration of extensive air showers…”
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Measurement of cosmic-ray air showers with the Tunka Radio Extension (Tunka-Rex) by Bezyazeekov, P.A., Budnev, N.M., Gress, O.A., Haungs, A., Hiller, R., Huege, T., Kazarina, Y., Kleifges, M., Konstantinov, E.N., Korosteleva, E.E., Kostunin, D., Krömer, O., Kuzmichev, L.A., Levinson, E., Lubsandorzhiev, N., Mirgazov, R.R., Monkhoev, R., Pakhorukov, A., Pankov, L., Prosin, V.V., Rubtsov, G.I., Rühle, C., Schröder, F.G., Wischnewski, R., Zagorodnikov, A.

“…Tunka-Rex is a radio detector for cosmic-ray air showers in Siberia, triggered by Tunka-133, a co-located air-Cherenkov detector. The main goal of Tunka-Rex is…”
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Tunka-133: Results of 3 year operation by Prosin, V.V., Berezhnev, S.F., Budnev, N.M., Chiavassa, A., Chvalaev, O.A., Gress, O.A., Dyachok, A.N., Epimakhov, S.N., Karpov, N.I., Kalmykov, N.N., Konstantinov, E.N., Korobchenko, A.V., Korosteleva, E.E., Kozhin, V.A., Kuzmichev, L.A., Lubsandorzhiev, B.K., Lubsandorzhiev, N.B., Mirgazov, R.R., Panasyuk, M.I., Pan'kov, L.V., Popova, E.G., Ptuskin, V.S., Semeney, Yu.A., Silaev, A.A., Silaev, A.A., Skurikhin, A.V., Spiering, C., Sveshnikova, L.G., Yashin, I.V., Zagorodnikov, A.V.

“…The EAS Cherenkov light array Tunka-133, with ~3km2 geometric area, is taking data since 2009. The array permits a detailed study of cosmic ray energy spectrum…”
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The Tunka-133 EAS Cherenkov light array: Status of 2011 by Berezhnev, S.F., Besson, D., Budnev, N.M., Chiavassa, A., Chvalaev, O.A., Gress, O.A., Dyachok, A.N., Epimakhov, S.N., Haungs, A., Karpov, N.I., Kalmykov, N.N., Konstantinov, E.N., Korobchenko, A.V., Korosteleva, E.E., Kozhin, V.A., Kuzmichev, L.A., Lubsandorzhiev, B.K., Lubsandorzhiev, N.B., Mirgazov, R.R., Panasyuk, M.I., Pankov, L.V., Popova, E.G., Prosin, V.V., Ptuskin, V.S., Semeney, Yu.A., Shaibonov, B.A., Silaev, A.A., Silaev, A.A., Skurikhin, A.V., Snyder, J., Spiering, C., Schröder, F.G., Stockham, M., Sveshnikova, L.G., Wischnewski, R., Yashin, I.V., Zagorodnikov, A.V.

“…A new EAS Cherenkov light array, Tunka-133, with ∼1km2 geometrical area has been installed at the Tunka Valley (50km from Lake Baikal) in 2009. The array…”
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Search for neutrino emission from relic dark matter in the sun with the Baikal NT200 detector by Avrorin, A.D., Avrorin, A.V., Aynutdinov, V.M., Bannasch, R., Belolaptikov, I.A., Bogorodsky, D.Yu, Brudanin, V.B., Budnev, N.M., Danilchenko, I.A., Demidov, S.V., Domogatsky, G.V., Doroshenko, A.A., Dyachok, A.N., Dzhilkibaev, Zh.-A.M., Fialkovsky, S.V., Gafarov, A.R., Gaponenko, O.N., Golubkov, K.V., Gress, T.I., Honz, Z., Kebkal, K.G., Kebkal, O.G., Konischev, K.V., Konstantinov, E.N., Korobchenko, A.V., Koshechkin, A.P., Koshel, F.K., Kozhin, A.V., Kulepov, V.F., Kuleshov, D.A., Ljashuk, V.I., Milenin, M.B., Mirgazov, R.A., Osipova, E.R., Panfilov, A.I., Pan’kov, L.V., Perevalov, A.A., Pliskovsky, E.N., Poleschuk, V.A., Rozanov, M.I., Rubtzov, V.F., Rjabov, E.V., Shaybonov, B.A., Sheifler, A.A., Shkurihin, A.V., Smagina, A.A., Suvorova, O.V., Tarashansky, B.A., Yakovlev, S.A., Zagorodnikov, A.V., Zhukov, V.A., Zurbanov, V.L.

“…We have analyzed a data set taken over 2.76years live time with the Baikal neutrino telescope NT200. The goal of the analysis is to search for neutrinos from…”
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The Tunka radio extension (Tunka-Rex): Radio measurements of cosmic rays in Siberia by Schröder, F.G., Bezyazeekov, P.A., Budnev, N.M., Gress, O.A., Haungs, A., Hiller, R., Huege, T., Kazarina, Y., Kleifges, M., Konstantinov, E.N., Korosteleva, E.E., Kostunin, D., Krömer, O., Kuzmichev, L.A., Lubsandorzhiev, N., Mirgazov, R.R., Monkhoev, R., Pakhorukov, A., Pankov, L., Prosin, V.V., Rubtsov, G.I., Wischnewski, R., Zagorodnikov, A.

“…The Tunka observatory is located close to Lake Baikal in Siberia, Russia. Its main detector, Tunka-133, is an array of photomultipliers measuring Cherenkov…”
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Tunka-Rex: Status and results of the first measurements by Kostunin, D., Budnev, N.M., Gress, O.A., Haungs, A., Hiller, R., Huege, T., Kazarina, Y., Kleifges, M., Konstantinov, A., Konstantinov, E.N., Korosteleva, E.E., Krömer, O., Kuzmichev, L.A., Mirgazov, R.R., Pankov, L., Prosin, V.V., Rubtsov, G.I., Rühle, C., Schröder, F.G., Svetnitsky, E., Wischnewski, R., Zagorodnikov, A.

“…Tunka-Rex is the new radio extension of Tunka-133 located in Siberia close to Lake Baikal. The latter is a photomultiplier array registering air-Cherenkov…”
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Primary CR energy spectrum and mass composition by the data of Tunka-133 array by Prosin, V.V., Berezhnev, S.F., Budnev, N.M., Chiavassa, A., Chvalaev, O.A., Dyachok, A.V., Epimakhov, S.N., Gress, O.A., Gress, T.I., Kalmykov, N.N., Karpov, N.I., Konstantinov, E.N., Korobchenko, A.V., Korosteleva, E.E., Kozhin, V.A., Kuzmichev, L.A., Lubsandorzhiev, B.K., Lubsandorzhiev, N.B., Mirgazov, R.R., Monkhoev, R.D., Osipova, E.A., Pakhorukov, A.L., Panasyuk, M.I., Pankov, L.V., Popova, E.G., Ptuskin, V.S., Semeney, Y.A., Silaev, A.A., (jun.), A.A. Silaev, Skurikhin, A.V., Spiering, C., Sveshnikova, L.G., Zagorodnikov, A.V.

“…The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons from 2009 to 2014. The…”
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The Tunka – Multi-component EAS detector for high energy cosmic ray studies by Berezhnev, S.F., Besson, D., Budnev, N.M., Büker, M., Brüeckner, M., Chiavassa, A., Chvalaev, O.A., Gress, O.A., Dyachok, A.N., Epimakhov, S.N., Hampf, D., Haungs, A., Hiller, R., Horns, D., Ivanova, A., Karpov, N.I., Kalmykov, N.N., Kazarina, Yu, Konstantinov, E.N., Kostunin, D., Korobchenko, A.V., Korosteleva, E.E., Kozhin, V.A., Kunnas, M., Kuzmichev, L.A., Lubsandorzhiev, B.K., Lubsandorzhiev, N.B., Mirgazov, R.R., Monhoev, R., Nachtigall, R., Panasyuk, M.I., Pankov, L.V., Pankov, A.L., Pokhorukov, A., Popova, E.G., Porelli, A., Prosin, V.V., Ptuskin, V.S., Rowell, G.P., Schröder, F.G., Semeney, Yu.A., Shaibonov, B.A., Silaev, A.A., Silaev, A.A., Skurikhin, A.V., Spiering, C., Spitschan, D., Sveshnikova, L.G., Wischnewski, R., Yashin, I.V., Zagorodnikov, A.V.

“…The EAS Cherenkov array Tunka-133, with about 3km2 sensitive area, has been installed in the Tunka Valley, Siberia. The accessible energy range is 1015–1018eV…”
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The optical detection unit for Baikal-GVD neutrino telescope by Avrorin, A.D., Avrorin, A.V., Aynutdinov, V.M., Bannash, R., Belolaptikov, I.A., Bogorodsky, D.Yu, Brudanin, V.B., Budnev, N.M., Danilchenko, I.A., Domogatsky, G.V., Doroshenko, A.A., Dyachok, A.N., Dzhilkibaev, Zh.-A.M., Fialkovsky, S.V., Gafarov, A.R., Gaponenko, O.N., Golubkov, K.V., Gress, T.I., Honz, Z., Kebkal, K.G., Kebkal, O.G., Konischev, K.V., Konstantinov, E.N., Korobchenko, A.V., Koshechkin, A.P., Koshel, F.K., Kozhin, A.V., Kulepov, V.F., Kuleshov, D.A., Ljashuk, V.I., Milenin, M.B., Mirgazov, R.A., Osipova, E.R., Panfilov, A.I., Pan'kov, L.V., Perevalov, A.A., Pliskovsky, E.N., Rozanov, M.I., Rubtzov, V.Yu, Rjabov, E.V., Shaybonov, B.A., Sheifler, A.A., Skurihin, A.V., Smagina, A.A., Suvorova, O.V., Tabolenko, V.A., Tarashansky, B.A., Yakovlev, S.A., Zagorodnikov, A.V., Zhukov, V.A., Zurbanov, V.L.

“…The first stage of the GVD-cluster composed of five strings was deployed in April 2014. Each string consists of two sections with 12 optical modules per…”
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