Zobrazeno 1 - 10
of 812
pro vyhledávání: '"Hartner G"'
Autor:
Zhang, C., Ling, Z. X., Sun, X. J., Sun, S. L., Liu, Y., Li, Z. D., Xue, Y. L., Chen, Y. F., Dai, Y. F., Jia, Z. Q., Liu, H. Y., Zhang, X. F., Zhang, Y. H., Zhang, S. N., Chen, F. S., Cheng, Z. W., Fu, W., Han, Y. X., Li, H., Li, J. F., Li, Y., Liu, P. R., Ma, X. H., Tang, Y. J., Wang, C. B., Xie, R. J., Yan, A. L., Zhang, Q., Jiang, B. W., Jin, G., Li, L. H., Qiu, X. B., Su, D. T., Sun, J. N., Xu, Z., Zhang, S. K., Zhang, Z., Zhang, N., Bi, X. Z., Cai, Z. M., He, J. W., Liu, H. Q., Zhu, X. C., Cheng, H. Q., Cui, C. Z., Fan, D. W., Hu, H. B., Huang, M. H., Jin, C. C., Li, D. Y., Pan, H. W., Wang, W. X., Xu, Y. F., Yang, X., Zhang, B., Zhang, M., Zhang, W. D., Zhao, D. H., Bai, M., Ji, Z., Liu, Y. R., Ma, F. L., Su, J., Tong, J. Z., Wang, Y. S., Zhao, Z. J., Feldman, C., O'Brien, P., Osborne, J. P., Willingale, R., Burwitz, V., Hartner, G., Langmeier, A., Müller, T., Rukdee, S., Schmidt, T., Kuulkers, E., Yuan, W.
As a novel X-ray focusing technology, lobster eye micro-pore optics (MPO) feature both a wide observing field of view and true imaging capability, promising sky monitoring with significantly improved sensitivity and spatial resolution in soft X-rays.
Externí odkaz:
http://arxiv.org/abs/2211.10007
Autor:
Basso, S., Salmaso, B., Spiga, D., Ghigo, M., Vecchi, G., Sironi, G., Cotroneo, V., Conconi, P., Redaelli, E., Bianco, A., Pareschi, G., Tagliaferri, G., Sisana, D., Pelliciari, C., Fiorini, M., Incorvaia, S., Uslenghi, M., Paoletti, L., Ferrari, C., Lolli, R., Zappettini, A., del Rio, M. Sanchez, Parodi, G., Burwitz, V., Rukdee, S., Hartner, G., Müller, T., Schmidt, T., Langmeier, A., Ferreira, D. Della Monica, Massahi, S., Gellert, N. C., Christensen, F., Bavdaz, M., Ferreira, I., Collon, M., Vacanti, G., Barrière, N. M.
The Beam Expander Testing X-ray facility (BEaTriX) is a unique X-ray apparatus now operated at the Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Brera (OAB), in Merate, Italy. It has been specifically designed to measure the p
Externí odkaz:
http://arxiv.org/abs/2206.15468
Autor:
Predehl, P., Andritschke, R., Arefiev, V., Babyshkin, V., Batanov, O., Becker, W., Böhringer, H., Bogomolov, A., Boller, T., Borm, K., Bornemann, W., Bräuninger, H., Brüggen, M., Brunner, H., Brusa, M., Bulbul, E., Buntov, M., Burwitz, V., Burkert, W., Clerc, N., Churazov, E., Coutinho, D., Dauser, T., Dennerl, K., Doroshenko, V., Eder, J., Emberger, V., Eraerds, T., Finoguenov, A., Freyberg, M., Friedrich, P., Friedrich, S., Fürmetz, M., Georgakakis, A., Gilfanov, M., Granato, S., Grossberger, C., Gueguen, A., Gureev, P., Haberl, F., Hälker, O., Hartner, G., Hasinger, G., Huber, H., Ji, L., Kienlin, A. v., Kink, W., Korotkov, F., Kreykenbohm, I., Lamer, G., Lomakin, I., Lapshov, I., Liu, T., Maitra, C., Meidinger, N., Menz, B., Merloni, A., Mernik, T., Mican, B., Mohr, J., Müller, S., Nandra, K., Nazarov, V., Pacaud, F., Pavlinsky, M., Perinati, E., Pfeffermann, E., Pietschner, D., Ramos-Ceja, M. E., Rau, A., Reiffers, J., Reiprich, T. H., Robrade, J., Salvato, M., Sanders, J., Santangelo, A., Sasaki, M., Scheuerle, H., Schmid, C., Schmitt, J., Schwope, A., Shirshakov, A., Steinmetz, M., Stewart, I., Strüder, L., Sunyaev, R., Tenzer, C., Tiedemann, L., Trümper, J., Voron, V., Weber, P., Wilms, J., Yaroshenko, V.
Publikováno v:
A&A 647, A1 (2021)
eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 13, 2019, from the Baikonour cosmodrome. After the commissioning of the
Externí odkaz:
http://arxiv.org/abs/2010.03477
Autor:
Spiga, D., Basso, S., Bavdaz, M., Burwitz, V., Civitani, M., Citterio, O., Ghigo, M., Hartner, G., Menz, B., Pareschi, G., Proserpio, L., Salmaso, B., Tagliaferri, G., Wille, E.
Publikováno v:
Proceedings of the SPIE, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VI, Vol. 8861, 88611F (2013)
The optics of a number of future X-ray telescopes will have very long focal lengths (10 - 20 m), and will consist of a number of nested/stacked thin, grazing-incidence mirrors. The optical quality characterization of a real mirror can be obtained via
Externí odkaz:
http://arxiv.org/abs/1509.02298
Autor:
ZEUS Collaboration, Abramowicz, H., Abt, I., Adamczyk, L., Adamus, M., Aggarwal, R., Antonelli, S., Arslan, O., Aushev, V., Aushev, Y., Bachynska, O., Barakbaev, A. N., Bartosik, N., Behnke, O., Behr, J., Behrens, U., Bertolin, A., Bhadra, S., Bloch, I., Bokhonov, V., Boos, E. G., Borras, K., Brock, I., Brugnera, R., Bruni, A., Brzozowska, B., Bussey, P. J., Caldwell, A., Capua, M., Catterall, C. D., Chwastowski, J., Ciborowski, J., Ciesielski, R., Cooper-Sarkar, A. M., Corradi, M., Corriveau, F., D'Agostini, G., Dementiev, R. K., Devenish, R. C. E., Dolinska, G., Drugakov, V., Dusini, S., Ferrando, J., Figiel, J., Foster, B., Gach, G., Garfagnini, A., Geiser, A., Gizhko, A., Gladilin, L. K., Gogota, O., Golubkov, Yu. A., Grebenyuk, J., Gregor, I., Grzelak, G., Gueta, O., Guzik, M., Hain, W., Hartner, G., Hochman, D., Hori, R., Ibrahim, Z. A., Iga, Y., Ishitsuka, M., Iudin, A., Januschek, F., Kadenko, I., Kananov, S., Kanno, T., Karshon, U., Kaur, M., Kaur, P., Khein, L. A., Kisielewska, D., Klanner, R., Klein, U., Kondrashova, N., Kononenko, O., Korol, Ie., Korzhavina, I. A., Kotanski, A., Kotz, U., Kovalchuk, N., Kowalski, H., Kuprash, O., Kuze, M., Levchenko, B. B., Levy, A., Libov, V., Limentani, S., Lisovyi, M., Lobodzinska, E., Lohmann, W., Lohr, B., Lohrmann, E., Longhin, A., Lontkovskyi, D., Lukina, O. Yu., Maeda, J., Makarenko, I., Malka, J., Martin, J. F., Mergelmeyer, S., Idris, F. Mohamad, Mujkic, K., Myronenko, V., Nagano, K., Nigro, A., Nobe, T., Notz, D., Nowak, R. J., Olkiewicz, K., Onishchuk, Yu., Paul, E., Perlanski, W., Perrey, H., Pokrovskiy, N. S., Proskuryakov, A. S., Przybycien, M., Raval, A., Roloff, P., Rubinsky, I., Ruspa, M., Samojlov, V., Saxon, D. H., Schioppa, M., Schmidke, W. B., Schneekloth, U., Schorner-Sadenius, T., Schwartz, J., Shcheglova, L. M., Shevchenko, R., Shkola, O., Singh, I., Skillicorn, I. O., Slominski, W., Sola, V., Solano, A., Spiridonov, A., Stanco, L., Stefaniuk, N., Stern, A., Stewart, T. P., Stopa, P., Sztuk-Dambietz, J., Szuba, D., Szuba, J., Tassi, E., Temiraliev, T., Tokushuku, K., Tomaszewska, J., Trofymov, A., Trusov, V., Tsurugai, T., Turcato, M., Turkot, O., Tymieniecka, T., Verbytskyi, A., Viazlo, O., Walczak, R., Abdullah, W. A. T. Wan, Wichmann, K., Wing, M., Wolf, G., Yamada, S., Yamazaki, Y., Zakharchuk, N., Zarnecki, A. F., Zawiejski, L., Zenaiev, O., Zhautykov, B. O., Zhmak, N., Zotkin, D. S.
Publikováno v:
JHEP 08 (2014) 23
In this extended analysis using the ZEUS detector at HERA, the photoproduction of isolated photons together with a jet is measured for different ranges of the fractional photon energy, $x_\gamma^{\mathrm{meas}}$, contributing to the photon-jet final
Externí odkaz:
http://arxiv.org/abs/1405.7127
Autor:
ZEUS collaboration, Abramowicz, H., Abt, I., Adamczyk, L., Adamus, M., Aggarwal, R., Antonelli, S., Arslan, O., Aushev, V., Aushev, Y., Bachynska, O., Barakbaev, A. N., Bartosik, N., Behnke, O., Behr, J., Behrens, U., Bertolin, A., Bhadra, S., Bloch, I., Bokhonov, V., Boos, E. G., Borras, K., Brock, I., Brugnera, R., Bruni, A., Brzozowska, B., Bussey, P. J., Caldwell, A., Capua, M., Catterall, C. D., Chwastowski, J., Ciborowski, J., Ciesielski, R., Cooper-Sarkar, A. M., Corradi, M., Corriveau, F., D'Agostini, G., Dementiev, R. K., Devenish, R. C. E., Dolinska, G., Drugakov, V., Dusini, S., Ferrando, J., Figiel, J., Foster, B., Gach, G., Garfagnini, A., Geiser, A., Gizhko, A., Gladilin, L. K., Gogota, O., Golubkov, Yu. A., Grebenyuk, J., Gregor, I., Grzelak, G., Gueta, O., Guzik, M., Hain, W., Hartner, G., Hochman, D., Hori, R., Ibrahim, Z. A., Iga, Y., Ishitsuka, M., Iudin, A., Januschek, F., Kadenko, I., Kananov, S., Kanno, T., Karshon, U., Kaur, M., Kaur, P., Khein, L. A., Kisielewska, D., Klanner, R., Klein, U., Kondrashova, N., Kononenko, O., Korol, Ie., Korzhavina, I. A., Kotański, A., Kötz, U., Kovalchuk, N., Kowalski, H., Kuprash, O., Kuze, M., Levchenko, B. B., Levy, A., Libov, V., Limentani, S., Lisovyi, M., Lobodzinska, E., Lohmann, W., Löhr, B., Lohrmann, E., Longhin, A., Lontkovskyi, D., Lukina, O. Yu., Maeda, J., Makarenko, I., Malka, J., Martin, J. F., Mergelmeyer, S., Idris, F. Mohamad, Mujkic, K., Myronenko, V., Nagano, K., Nigro, A., Nobe, T., Notz, D., Nowak, R. J., Olkiewicz, K., Onishchuk, Yu., Paul, E., Perlański, W., Perrey, H., Pokrovskiy, N. S., Proskuryakov, A. S., Przybycień, M., Raval, A., Roloff, P., Rubinsky, I., Ruspa, M., Samojlov, V., Saxon, D. H., Schioppa, M., Schmidke, W. B., Schneekloth, U., Schörner-Sadenius, T., Schwartz, J., Shcheglova, L. M., Shehzadi, R., Shevchenko, R., Shkola, O., Singh, I., Skillicorn, I. O., Słomiński, W., Sola, V., Solano, A., Spiridonov, A., Stanco, L., Stefaniuk, N., Stern, A., Stewart, T. P., Stopa, P., Sztuk-Dambietz, J., Szuba, D., Szuba, J., Tassi, E., Temiraliev, T., Tokushuku, K., Tomaszewska, J., Trofymov, A., Trusov, V., Tsurugai, T., Turcato, M., Turkot, O., Tymieniecka, T., Verbytskyi, A., Viazlo, O., Walczak, R., Abdullah, W. A. T. Wan, Wichmann, K., Wing, M., Wolf, G., Yamada, S., Yamazaki, Y., Zakharchuk, N., Żarnecki, A. F., Zawiejski, L., Zenaiev, O., Zhautykov, B. O., Zhmak, N., Zotkin, D. S.
The production of beauty and charm quarks in ep interactions has been studied with the ZEUS detector at HERA for exchanged four-momentum squared 5 < Q^2 < 1000 GeV^2 using an integrated luminosity of 354 pb^{-1}. The beauty and charm content in event
Externí odkaz:
http://arxiv.org/abs/1405.6915
Autor:
ZEUS Collaboration, Abramowicz, H., Abt, I., Adamczyk, L., Adamus, M., Aggarwal, R., Antonelli, S., Arslan, O., Aushev, V., Aushev, Y., Bachynska, O., Barakbaev, A. N., Bartosik, N., Behnke, O., Behr, J., Behrens, U., Bertolin, A., Bhadra, S., Bloch, I., Bokhonov, V., Boos, E. G., Borras, K., Brock, I., Brugnera, R., Bruni, A., Brzozowska, B., Bussey, P. J., Caldwell, A., Capua, M., Catterall, C. D., Chwastowski, J., Ciborowski, J., Ciesielski, R., Cooper-Sarkar, A. M., Corradi, M., Corriveau, F., D'Agostini, G., Dementiev, R. K., Devenish, R. C. E., Dolinska, G., Drugakov, V., Dusini, S., Ferrando, J., Figiel, J., Foster, B., Gach, G., Garfagnini, A., Geiser, A., Gizhko, A., Gladilin, L. K., Gogota, O., Golubkov, Yu. A., Grebenyuk, J., Gregor, I., Grzelak, G., Gueta, O., Guzik, M., Hain, W., Hartner, G., Hochman, D., Hori, R., Ibrahim, Z. A., Iga, Y., Ishitsuka, M., Iudin, A., Januschek, F., Kadenko, I., Kananov, S., Kanno, T., Karshon, U., Kaur, M., Kaur, P., Khein, L. A., Kisielewska, D., Klanner, R., Klein, U., Kondrashova, N., Kononenko, O., Korol, Ie., Korzhavina, I. A., Kotanski, A., Kotz, U., Kovalchuk, N., Kowalski, H., Kuprash, O., Kuze, M., Levchenko, B. B., Levy, A., Libov, V., Limentani, S., Lisovyi, M., Lobodzinska, E., Lohmann, W., Lohr, B., Lohrmann, E., Longhin, A., Lontkovskyi, D., Lukina, O. Yu., Maeda, J., Makarenko, I., Malka, J., Martin, J. F., Mergelmeyer, S., Idris, F. Mohamad, Mujkic, K., Myronenko, V., Nagano, K., Nigro, A., Nobe, T., Notz, D., Nowak, R. J., Olkiewicz, K., Onishchuk, Yu., Paul, E., Perlanski, W., Perrey, H., Pokrovskiy, N. S., Proskuryakov, A. S., Przybycien, M., Raval, A., Roloff, P., Rubinsky, I., Ruspa, M., Samojlov, V., Saxon, D. H., Schioppa, M., Schmidke, W. B., Schneekloth, U., Schorner-Sadenius, T., Schwartz, J., Shcheglova, L. M., Shevchenko, R., Shkola, O., Singh, I., Skillicorn, I. O., Slominski, W., Sola, V., Solano, A., Spiridonov, A., Stanco, L., Stefaniuk, N., Stern, A., Stewart, T. P., Stopa, P., Sztuk-Dambietz, J., Szuba, D., Szuba, J., Tassi, E., Temiraliev, T., Tokushuku, K., Tomaszewska, J., Trofymov, A., Trusov, V., Tsurugai, T., Turcato, M., Turkot, O., Tymieniecka, T., Verbytskyi, A., Viazlo, O., Walczak, R., Abdullah, W. A. T. Wan, Wichmann, K., Wing, M., Wolf, G., Yamada, S., Yamazaki, Y., Zakharchuk, N., Zarnecki, A. F., Zawiejski, L., Zenaiev, O., Zhautykov, B. O., Zhmak, N., Zotkin, D. S.
The photoproduction of $D^{*\pm}$ mesons has been measured with the ZEUS detector at HERA at three different ep centre-of-mass energies, $\sqrt{s}$, of 318, 251 and 225 GeV. For each data set, $D^*$ mesons were required to have transverse momentum, $
Externí odkaz:
http://arxiv.org/abs/1405.5068
Autor:
ZEUS Collaboration, Abramowicz, H., Abt, I., Adamczyk, L., Adamus, M., Aggarwal, R., Antonelli, S., Arslan, O., Aushev, V., Aushev, Y., Bachynska, O., Barakbaev, A. N., Bartosik, N., Behnke, O., Behr, J., Behrens, U., Bertolin, A., Bhadra, S., Bloch, I., Bokhonov, V., Boos, E. G., Borras, K., Brock, I., Brugnera, R., Bruni, A., Brzozowska, B., Bussey, P. J., Caldwell, A., Capua, M., Catterall, C. D., Chwastowski, J., Ciborowski, J., Ciesielski, R., Cooper-Sarkar, A. M., Corradi, M., Corriveau, F., D'Agostini, G., Dementiev, R. K., Devenish, R. C. E., Dolinska, G., Drugakov, V., Dusini, S., Ferrando, J., Figiel, J., Foster, B., Gach, G., Garfagnini, A., Geiser, A., Gizhko, A., Gladilin, L. K., Gogota, O., Golubkov, Yu. A., Grebenyuk, J., Gregor, I., Grzelak, G., Gueta, O., Guzik, M., Hain, W., Hartner, G., Hochman, D., Hori, R., Ibrahim, Z. A., Iga, Y., Ishitsuka, M., Iudin, A., Januschek, F., Kadenko, I., Kananov, S., Kanno, T., Karshon, U., Kaur, M., Kaur, P., Khein, L. A., Kisielewska, D., Klanner, R., Klein, U., Kondrashova, N., Kononenko, O., Korol, Ie., Korzhavina, I. A., Kotanski, A., Kotz, U., Kovalchuk, N., Kowalski, H., Kuprash, O., Kuze, M., Levchenko, B. B., Levy, A., Libov, V., Limentani, S., Lisovyi, M., Lobodzinska, E., Lohmann, W., Lohr, B., Lohrmann, E., Longhin, A., Lontkovskyi, D., Lukina, O. Yu., Maeda, J., Makarenko, I., Malka, J., Martin, J. F., Mergelmeyer, S., Idris, F. Mohamad, Mujkic, K., Myronenko, V., Nagano, K., Nigro, A., Nobe, T., Notz, D., Nowak, R. J., Olkiewicz, K., Onishchuk, Yu., Paul, E., Perlanski, W., Perrey, H., Pokrovskiy, N. S., Proskuryakov, A. S., Przybycien, M., Raval, A., Roloff, P., Rubinsky, I., Ruspa, M., Samojlov, V., Saxon, D. H., Schioppa, M., Schmidke, W. B., Schneekloth, U., Schorner-Sadenius, T., Schwartz, J., Shcheglova, L. M., Shevchenko, R., Shkola, O., Singh, I., Skillicorn, I. O., Slominski, W., Sola, V., Solano, A., Spiridonov, A., Stanco, L., Stefaniuk, N., Stern, A., Stewart, T. P., Stopa, P., Sztuk-Dambietz, J., Szuba, D., Szuba, J., Tassi, E., Temiraliev, T., Tokushuku, K., Tomaszewska, J., Trofymov, A., Trusov, V., Tsurugai, T., Turcato, M., Turkot, O., Tymieniecka, T., Verbytskyi, A., Viazlo, O., Walczak, R., Abdullah, W. A. T. Wan, Wichmann, K., Wing, M., Wolf, G., Yamada, S., Yamazaki, Y., Zakharchuk, N., Zarnecki, A. F., Zawiejski, L., Zenaiev, O., Zhautykov, B. O., Zhmak, N., Zotkin, D. S.
Publikováno v:
Phys. Rev. D 90, 072002 (2014)
The reduced cross sections for $e^{+}p$ deep inelastic scattering have been measured with the ZEUS detector at HERA at three different centre-of-mass energies, $318$, $251$ and $225$ GeV. The cross sections, measured double differentially in Bjorken
Externí odkaz:
http://arxiv.org/abs/1404.6376
Autor:
Fabiani, S., Costa, E., Del Monte, E., Muleri, F., Soffitta, P., Rubini, A., Bellazzini, R., Brez, A., de Ruvo, L., Minuti, M., Pinchera, M., Sgrò, C., Spandre, G., Spiga, D., Tagliaferri, G., Pareschi, G., Basso, S., Citterio, O., Burwitz, V., Burkert, W., Menz, B., Hartner, G.
X-rays are particularly suited to probe the physics of extreme objects. However, despite the enormous improvements of X-ray Astronomy in imaging, spectroscopy and timing, polarimetry remains largely unexplored. We propose the photoelectric polarimete
Externí odkaz:
http://arxiv.org/abs/1403.7200
Autor:
ZEUS Collaboration, Abramowicz, H., Abt, I., Adamczyk, L., Adamus, M., Aggarwal, R., Antonelli, S., Arslan, O., Aushev, V., Aushev, Y., Bachynska, O., Barakbaev, A. N., Bartosik, N., Behnke, O., Behr, J., Behrens, U., Bertolin, A., Bhadra, S., Bloch, I., Bokhonov, V., Boos, E. G., Borras, K., Brock, I., Brugnera, R., Bruni, A., Brzozowska, B., Bussey, P. J., Caldwell, A., Capua, M., Catterall, C. D., Chwastowski, J., Ciborowski, J., Ciesielski, R., Cooper-Sarkar, A. M., Corradi, M., Corriveau, F., Agostini, G. D, Dementiev, R. K., Devenish, R. C. E., Dolinska, G., Drugakov, V., Dusini, S., Ferrando, J., Figiel, J., Foster, B., Gach, G., Garfagnini, A., Geiser, A., Gizhko, A., Gladilin, L. K., Gogota, O., Golubkov, Yu. A., Grebenyuk, J., Gregor, I., Grzelak, G., Gueta, O., Guzik, M., Hain, W., Hartner, G., Hochman, D., Hori, R., Ibrahim, Z. A., Iga, Y., Ishitsuka, M., Iudin, A., Januschek, F., Kadenko, I., Kananov, S., Kanno, T., Karshon, U., Kaur, M., Kaur, P., Khein, L. A., Kisielewska, D., Klanner, R., Klein, U., Kondrashova, N., Kononenko, O., Korol, Ie., Korzhavina, I. A., Kotanski, A., Koetz, U., Kovalchuk, N., Kowalski, H., Kuprash, O., Kuze, M., Levchenko, B. B., Levy, A., Libov, V., Limentani, S., Lisovyi, M., Lobodzinska, E., Lohmann, W., Loehr, B., Lohrmann, E., Longhin, A., Lontkovskyi, D., Lukina, O. Yu., Maeda, J., Makarenko, I., Malka, J., Martin, J. F., Mergelmeyer, S., Idris, F. Mohamad, Mujkic, K., Myronenko, V., Nagano, K., Nigro, A., Nobe, T., Notz, D., Nowak, R. J., Olkiewicz, K., Onishchuk, Yu., Paul, E., Perlanski, W., Perrey, H., Pokrovskiy, N. S., Proskuryakov, A. S., Przybycien, M., Raval, A., Roloff, P., Rubinsky, I., Ruspa, M., Samojlov, V., Saxon, D. H., Schioppa, M., Schmidke, W. B., Schneekloth, U., Schoerner-Sadenius, T., Schwartz, J., Shcheglova, L. M., Shevchenko, R., Shkola, O., Singh, I., Skillicorn, I. O., Slominski, W., Sola, V., Solano, A., Spiridonov, A., Stanco, L., Stefaniuk, N., Stern, A., Stewart, T. P., Stopa, P., Sztuk-Dambietz, J., Szuba, D., Szuba, J., Tassi, E., Temiraliev, T., Tokushuku, K., Tomaszewska, J., Trofymov, A., Trusov, V., Tsurugai, T., Turcato, M., Turkot, O., Tymieniecka, T., Verbytskyi, A., Viazlo, O., Walczak, R., Abdullah, W. A. T. Wan, Wichmann, K., Wing, M., Wolf, G., Yamada, S., Yamazaki, Y., Zakharchuk, N., Zarnecki, A. F., Zawiejski, L., Zenaiev, O., Zhautykov, B. O., Zhmak, N., Zotkin, D. S.
Publikováno v:
Phys. Rev. D 89, 072007 (2014)
The neutral current e+/-p cross section has been measured up to values of Bjorken x of approximately 1 with the ZEUS detector at HERA using an integrated luminosity of 187 inv. pb of e-p and 142 inv. pb of e+p collisions at sqrt(s) = 318GeV. Differen
Externí odkaz:
http://arxiv.org/abs/1312.4438