121 results on '"Naito T"'
Search Results
2. Simulation of mechanical stresses in reinforced REBaCuO disk bulks during pulsed-field magnetization
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Shimoyashiki, F, Fujishiro, H, Hirano, T, Naito, T, Ainslie, Mark, Apollo - University of Cambridge Repository, and Ainslie, Mark [0000-0003-0466-3680]
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Paper ,History ,51 Physical Sciences ,5103 Classical Physics ,Computer Science Applications ,Education - Abstract
We have performed numerical simulations of the electromagnetic hoop stress, ���� , in a REBaCuO disk bulk reinforced by a metal ring during pulsed-field magnetization (PFM) using a solenoid coil, in which the superconducting characteristics of the bulk material were assumed to have realistic J c-B-T ones. The compressive and tensile ���� stresses were applied in the bulk during the ascending and descending stages of PFM, respectively. The time and position dependences of the mechanical stresses were estimated. The possibility of mechanical fracture due to these hoop stresses and the effect of the metal ring reinforcement were discussed., Japan Society for the Promotion of Science (JSPS) KAKENHI Grant No. 15K04646
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- 2022
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3. Narrow Zero Mode in Organic Massless Dirac Electron System $��$-(BEDT-TTF)$_2$I$_3$
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Mori, A., Kawasugi, Y., Doi, R., Naito, T., Kato, R., Nishio, Y., and Tajima, N.
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Condensed Matter::Materials Science ,Strongly Correlated Electrons (cond-mat.str-el) ,Condensed Matter::Superconductivity ,FOS: Physical sciences ,Condensed Matter::Strongly Correlated Electrons ,Condensed Matter::Mesoscopic Systems and Quantum Hall Effect - Abstract
We investigated the interlayer magnetoresistance in an organic massless Dirac electron system $��$-(BEDT-TTF)$_2$I$_3$ under pressure. We experimentally demonstrate that the width of the zero mode owing to carrier scattering is much narrower than that of the other Landau levels., 6 pages, 1 figures
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- 2022
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4. Proton Penetration Efficiency over a High Altitude Observatory in Mexico
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Miyake, S., Koi, T., Muraki, Y., Matsubara, Y., Masuda, S., Miranda, P., Naito, T., Ortiz, E., Oshima, A., Sakai, T., Sako, T., Shibata, S., Takamaru, H., Tokumaru, M., and Valdes-Galicia, J. F.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Astrophysics - Solar and Stellar Astrophysics ,Astrophysics::High Energy Astrophysical Phenomena ,Physics::Space Physics ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena ,Nuclear Experiment ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
In association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250m) in Bolivia and Mt. Sierra Negra (4,600m) in Mexico recorded very interesting events. In order to explain these events, we have performed a calculation solving the equation of motion of anti-protons inside the magnetosphere. Based on these results, the Mt. Chacaltaya event may be explained by the detection of solar neutrons, while the Mt. Sierra Negra event may be explained by the first detection of very high energy solar neutron decay protons (SNDPs) around 6 GeV., Comment: Paper presented in the 21st International Symposium on Very High Energy Cosmic Ray Intercations (ISVHE-CRI 2022) by online
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- 2022
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5. Influence of Jc(B, T) Characteristics on the Pulsed Field Magnetization of REBaCuO Disk Bulks
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Hirano, T, Takahashi, K, Shimoyashiki, F, Fujishiro, H, Naito, T, Ainslie, Mark, Hirano, T [0000-0003-1658-914X], Takahashi, K [0000-0002-8278-2688], Naito, T [0000-0001-7594-3466], Ainslie, Mark [0000-0003-0466-3680], Apollo - University of Cambridge Repository, and Ainslie, MD [0000-0003-0466-3680]
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REBaCuO bulk ,J (c) (B,T) characteristics (Jirsa model, Kim model, Bean model) ,numerical simulation ,pulsed-field magnetization (PFM) - Abstract
The trapped field properties during pulsed-field magnetization (PFM) have been investigated numerically using three different assumptions relating to the Jc(B, T) characteristics (Jirsa, Kim and Bean models) and compared with experimental results. The trapped field properties using the Jirsa model with the so-called ‘peak effect’, in which a realistic Jc(B, T) is assumed, rather than the Kim model, result in a more realistic numerical simulation. The trapped field properties using a Kim model with a monotonically decreasing Jc(B) also show similar results to those using the Jirsa model. The trapped field properties using a Bean model, for which Jc is independent of magnetic field, are not necessarily enhanced because of a larger temperature rise. The numerical results suggest it is necessary to fabricate REBaCuO bulks with Jc(B, T) characteristics with moderate magnetic field and temperature dependences to enhance the trapped field by PFM.
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- 2019
6. Simulation of mechanical stresses in reinforced REBaCuO ring bulks during pulsed-field magnetization
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Hirano, T, Fujishiro, H, Naito, T, Ainslie, Mark, Apollo - University of Cambridge Repository, and Ainslie, Mark [0000-0003-0466-3680]
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Paper ,51 Physical Sciences - Abstract
We have performed numerical simulations of the electromagnetic, thermal and mechanical properties of a REBaCuO ring-shaped bulk with various reinforcement structures during pulsed-field magnetization (PFM). Compressive and tensile electromagnetic stresses, �� �� mag , are developed in the ring-shaped bulk during the ascending and descending stages of PFM, respectively. These stresses increase at lower operating temperatures and for higher applied pulsed fields. In order to reduce these stresses, the ring-shaped bulk was fully encapsulated by outer and inner ring with upper and lower plates made by Al alloy. In particular, this reinforcement structure can achieve the lowest electromagnetic compressive stress, which corresponds to about 54% of that for a conventional ring reinforcement structure, and the electromagnetic tensile stress was also reduced. We also compared the simulation results of the electromagnetic stresses for the ring-shaped bulk to those for a disk-shaped bulk., JSPS KAKENHI Grant No. 15K04646
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- 2020
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7. Experimental realization of a hybrid trapped field magnet lens using a GdBaCuO magnetic lens and MgB2 bulk cylinder
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Namba, S, Fujishiro, H, Naito, T, Ainslie, MD, and Takahashi, K
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hybrid trapped magnet field lens ,trapped field magnets ,magnetic lens ,bulk superconductors ,vortex pinning effect ,magnetic shielding effect - Abstract
A hybrid trapped field magnet lens (HTFML) is a promising device that is able to concentrate a magnetic field higher than the applied field continuously, even after removing an external field, which was conceptually proposed by the authors in 2018. This paper presents, for the first time, the experimental realization of the HTFML using a GdBaCuO magnetic lens and MgB2 trapped field magnet cylinder. A maximum concentrated magnetic field of B c = 3.55 T was achieved at the central bore of the HTFML after removing an applied field of B app = 2.0 T at T = 20 K. For higher B app, the B c value was not enhanced because of a weakened lens effect due to magnetic flux penetration into the bulk GdBaCuO material comprising the lens. The enhancement of the trapped field using such an HTFML for the present experimental setup is discussed in detail.
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- 2019
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8. Nonmonotonic bias dependence of local spin accumulation signals in ferromagnet/semiconductor lateral spin-valve devices
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Fujita, Y., Yamada, M., Tsukahara, M., Naito, T., Yamada, S., Oki, S., Sawano, K., and Hamaya, K.
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Physics ,Condensed Matter - Materials Science ,Spin polarization ,Condensed matter physics ,Condensed Matter - Mesoscale and Nanoscale Physics ,business.industry ,Spin valve ,Schottky diode ,Materials Science (cond-mat.mtrl-sci) ,FOS: Physical sciences ,Biasing ,02 engineering and technology ,021001 nanoscience & nanotechnology ,Condensed Matter::Mesoscopic Systems and Quantum Hall Effect ,01 natural sciences ,Nonlinear system ,Semiconductor ,Ferromagnetism ,0103 physical sciences ,Mesoscale and Nanoscale Physics (cond-mat.mes-hall) ,Condensed Matter::Strongly Correlated Electrons ,010306 general physics ,0210 nano-technology ,business - Abstract
We find extraordinary behavior of the local two-terminal spin accumulation signals in ferromagnet (FM)/semiconductor (SC) lateral spin-valve devices. With respect to the bias voltage applied between two FM/SC Schottky tunnel contacts, the local spin-accumulation signal can show nonmonotonic variations, including a sign inversion. A part of the nonmonotonic features can be understood qualitatively by considering the rapid reduction in the spin polarization of the FM/SC interfaces with increasing bias voltage. In addition to the sign inversion of the FM/SC interface spin polarization, the influence of the spin-drift effect in the SC layer and the nonlinear electrical spin conversion at a biased FM/SC contact are discussed., Comment: 10 pages, 7 figures, supplementary material
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- 2018
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9. Usefulness of a peripherally inserted central catheter for total parenteral nutrition in patients with inflammatory bowel disease
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Chiba, H., Endo, K., Izumiyama, Y., Nakano, T., Okamoto, D., Ichikawa, R., Nagai, H., Matsumoto, S., Yokoyama, N., Yamamoto, K., Shimoyama, Y., Naito, T., Onodera, M., Kusaka, J., Hiramoto, K., Kuroha, M., Kanazawa, Y., Kimura, T., Yoichi Kakuta, Kinouchi, Y., and Shimosegawa, T.
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Adult ,Male ,Catheterization, Peripheral ,Humans ,Female ,Parenteral Nutrition, Total ,Inflammatory Bowel Diseases ,Retrospective Studies - Abstract
Peripherally inserted central catheters (PICC) have been widely used as a blood access route for total parenteral nutrition (TPN) in recent years. However, there have been few reports that evaluated the usefulness of PICC for patients with inflammatory bowel disease (IBD). In this study, we compared the clinical courses in patients with IBD who received TPN during their hospitalization by conventional central venous catheters (CVC) and PICC.A total of 137 IBD patients were enrolled. The CVC group and the PICC group included 56 and 81 patients, respectively. The clinical courses in both groups were compared retrospectively.As a complication of the puncture, pneumothorax occurred in two patients (3.6%) in the CVC group, but in none (0%) in the PICC group. The PICC group had significantly higher rates of achieving the scheduled TPN without removing the catheter, lower rates of catheter-related blood stream infection (CRBSI) and longer periods without CRBSI than the CVC group.PICC might be more useful than CVC in terms of safety and the ability to deliver scheduled TPN for IBD patients.
- Published
- 2017
10. Prospects for CTA observations of the young SNR RX J1713.7-3946
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Cta Consortium, The, Acero, F., Aloisio, R., Amans, J., Amato, E., Antonelli, L. A., Aramo, C., Armstrong, T., Arqueros, F., Asano, K., Ashley, M., Backes, M., Balazs, C., Balzer, A., Bamba, A., Barkov, M., Barrio, J. A., Benbow, W., Bernlöhr, K., Beshley, V., Bigongiari, C., Biland, A., Bilinsky, A., Bissaldi, E., Biteau, J., Blanch, O., Blasi, P., Blazek, J., Boisson, C., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Braiding, C., Brau-Nogué, S., Bregeon, J., Brown, A. M., Bugaev, V., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Böttcher, M., Cameron, R., Capalbi, M., Caproni, A., Caraveo, P., Carosi, R., Cascone, E., Cerruti, M., Chaty, S., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Chudoba, J., Cohen-Tanugi, J., Colafrancesco, S., Conforti, V., Contreras, J. L., Costa, A., Cotter, G., Covino, S., Covone, G., Cumani, P., Cusumano, G., D Ammando, F., D Urso, D., Daniel, M., Dazzi, F., Angelis, A., Cesare, G., Franco, A., Frondat, F., Gouveia Dal Pino, E. M., Lisio, C., Los Reyes Lopez, R., Lotto, B., Naurois, M., Palma, F., Del Santo, M., Delgado, C., Della Volpe, D., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Di Venere, L., Doro, M., Dournaux, J., Dumas, D., Dwarkadas, V., Díaz, C., Ebr, J., Egberts, K., Einecke, S., Elsässer, D., Eschbach, S., Falceta-Goncalves, D., Fasola, G., Fedorova, E., Fernández-Barral, A., Ferrand, G., Fesquet, M., Fiandrini, E., Fiasson, A., Filipovíc, M. D., Fioretti, V., Font, L., Fontaine, G., Franco, F. J., Freixas Coromina, L., Fujita, Y., Fukui, Y., Funk, S., Förster, A., Gadola, A., Garcia López, R., Garczarczyk, M., Giglietto, N., Giordano, F., Giuliani, A., Glicenstein, J., Gnatyk, R., Goldoni, P., Grabarczyk, T., Graciani, R., Graham, J., Grandi, P., Granot, J., Green, A. J., Griffiths, S., Gunji, S., Hakobyan, H., Hara, S., Hassan, T., Hayashida, M., Heller, M., Helo, J. C., Hinton, J., Hnatyk, B., Huet, J., Huetten, M., Humensky, T. B., Hussein, M., Hörandel, J., Ikeno, Y., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Ioka, K., Iori, M., Jacquemier, J., Janecek, P., Jankowsky, D., Jung, I., Kaaret, P., Katagiri, H., Kimeswenger, S., Kimura, S., Knödlseder, J., Koch, B., Kocot, J., Kohri, K., Komin, N., Konno, Y., Kosack, K., Koyama, S., Kraus, M., Kubo, H., Kukec Mezek, G., Kushida, J., La Palombara, N., Lalik, K., Lamanna, G., Landt, H., Lapington, J., Laporte, P., Lee, S., Lees, J., Lefaucheur, J., Lenain, J. -P, Leto, G., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, M., Lucarelli, F., Luque-Escamilla, P. L., López-Coto, R., Maccarone, M. C., Maier, G., Malaguti, G., Mandat, D., Maneva, G., Mangano, S., Marcowith, A., Martí, J., Martínez, M., Martínez, G., Masuda, S., Maurin, G., Maxted, N., Melioli, C., Mineo, T., Mirabal, N., Mizuno, T., Moderski, R., Mohammed, M., Montaruli, T., Moralejo, A., Mori, K., Morlino, G., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Muraishi, H., Murase, K., Nagataki, S., Nagayoshi, T., Naito, T., Nakajima, D., Nakamori, T., Nemmen, R., Niemiec, J., Nieto, D., Nievas-Rosillo, M., Nikołajuk, M., Nishijima, K., Noda, K., Nogues, L., Nosek, D., Novosyadlyj, B., Nozaki, S., Ohira, Y., Ohishi, M., Ohm, S., Okumura, A., Ong, R. A., Orito, R., Orlati, A., Ostrowski, M., Oya, I., Padovani, M., Palacio, J., Palatka, M., Paredes, J. M., Pavy, S., Pe Er, A., Persic, M., Petrucci, P., Petruk, O., Pisarski, A., Pohl, M., Porcelli, A., Prandini, E., Prast, J., Principe, G., Prouza, M., Pueschel, E., Pühlhofer, G., Quirrenbach, A., Rameez, M., Reimer, O., Renaud, M., Ribó, M., Rico, J., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodríguez Vázquez, J. J., Romano, P., Romeo, G., Rosado, J., Rousselle, J., Rowell, G., Rudak, B., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sanchez, D., Sangiorgi, P., Sano, H., Santander, M., Sarkar, S., Sawada, M., Schioppa, E. J., Schoorlemmer, H., Schovanek, P., Schussler, F., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Siejkowski, H., Sillanpää, A., Simone, D., Sliusar, V., Sol, H., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Szanecki, M., Szepieniec, T., Tagliaferri, G., Tajima, H., Takahashi, M., Takeda, J., Tanaka, M., Tanaka, S., Tejedor, L. A., Telezhinsky, I., Temnikov, P., Terada, Y., Tescaro, D., Teshima, M., Testa, V., Thoudam, S., Tokanai, F., Torres, D. F., Torresi, E., Tosti, G., Townsley, C., Travnicek, P., Trichard, C., Trifoglio, M., Tsujimoto, S., Vagelli, V., Vallania, P., Valore, L., Driel, W., Eldik, C., Vandenbroucke, J., Vassiliev, V., Vecchi, M., Vercellone, S., Vergani, S., Vigorito, C., Vorobiov, S., Vrastil, M., Vázquez Acosta, M. L., Wagner, S. J., Wagner, R., Wakely, S. P., Walter, R., Ward, J. E., Watson, J. J., Weinstein, A., White, M., White, R., Wierzcholska, A., Wilcox, P., Williams, D. A., Wischnewski, R., Wojcik, P., Yamamoto, T., Yamamoto, H., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshida, M., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zampieri, L., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A., Zech, A., Zechlin, H., Zhdanov, V., Ziegler, A., and Zorn, J.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics::Galaxy Astrophysics - Abstract
We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX~J1713.7$-$3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very-high-energy (VHE) gamma rays. Special attention is paid to explore possible spatial (anti-)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/H{\sc i} emission. We present a series of simulated images of RX J1713.7$-$3946 for CTA based on a set of observationally motivated models for the gamma-ray emission. In these models, VHE gamma rays produced by high-energy electrons are assumed to trace the non-thermal X-ray emission observed by {\it XMM-Newton}, whereas those originating from relativistic protons delineate the local gas distributions. The local atomic and molecular gas distributions are deduced by the NANTEN team from CO and H{\sc i} observations. Our primary goal is to show how one can distinguish the emission mechanism(s) of the gamma rays (i.e., hadronic vs leptonic, or a mixture of the two) through information provided by their spatial distribution, spectra, and time variation. This work is the first attempt to quantitatively evaluate the capabilities of CTA to achieve various proposed scientific goals by observing this important cosmic particle accelerator., Comment: 19 pages, 5 figures. Accepted for publication in ApJ
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- 2017
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11. Binaries with the eyes of CTA
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Paredes, J. M., Bednarek, W., Bordas, P., Bosch Ramon, V., Cea, E. D., Dubus, G., Funk, S., Hadasch, D., Khangulyan, D., Markoff, S., Moldon, J., Munar Adrover, P., Nagataki, S., Naito, T., Naurois, M. d., Pedaletti, G., Reimer, O., Ribo, M., Szostek, A., Terada, Y., Torres, D. F., Zabalza, V., Zdziarski, A. A., Cta, Consortium, Acharya, B. S., Actis, M., Aghajani, T., Bissaldi, Elisabetta, J. M., Parede, W., Bednarek, P., Borda, V., Bosch Ramon, E. D., Cea, G., Dubu, S., Funk, D., Hadasch, D., Khangulyan, S., Markoff, J., Moldon, P., Munar Adrover, S., Nagataki, T., Naito, M. d., Nauroi, G., Pedaletti, O., Reimer, M., Ribo, A., Szostek, Y., Terada, D. F., Torre, V., Zabalza, A. A., Zdziarski, Cta, Consortium, Acharya, B. S., Actis, M., Aghajani, T., Bissaldi, Elisabetta, and High Energy Astrophys. & Astropart. Phys (API, FNWI)
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observations [gamma-rays] ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Binary number ,Context (language use) ,Astrophysics ,Compact star ,01 natural sciences ,Cherenkov astronomy ,general [binaries] ,Pulsar ,Observacions astronòmiques ,Gamma ray astronomy ,0103 physical sciences ,Astronomia de raigs gamma ,010303 astronomy & astrophysics ,acceleration of particle ,Astrophysics::Galaxy Astrophysics ,Estels binaris de raigs X ,acceleration of particles ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Telescopis ,Accretion (meteorology) ,010308 nuclear & particles physics ,Astronomy ,Astronomy and Astrophysics ,gamma rays: general ,radiation mechanisms: non-thermal ,non-thermal [radiation mechanisms] ,Cherenkov Telescope Array ,Particle acceleration ,X-ray binaries ,Stars ,binaries: general ,Astrophysics - High Energy Astrophysical Phenomena ,general [gamma rays] ,Telescopes ,Astronomical observations - Abstract
The binary systems that have been detected in gamma rays have proven very useful to study high-energy processes, in particular particle acceleration, emission and radiation reprocessing, and the dynamics of the underlying magnetized flows. Binary systems, either detected or potential gamma-ray emitters, can be grouped in different subclasses depending on the nature of the binary components or the origin of the particle acceleration: the interaction of the winds of either a pulsar and a massive star or two massive stars; accretion onto a compact object and jet formation; and interaction of a relativistic outflow with the external medium. We evaluate the potentialities of an instrument like the Cherenkov telescope array (CTA) to study the non-thermal physics of gamma-ray binaries, which requires the observation of high-energy phenomena at different time and spatial scales. We analyze the capability of CTA, under different configurations, to probe the spectral, temporal and spatial behavior of gamma-ray binaries in the context of the known or expected physics of these sources. CTA will be able to probe with high spectral, temporal and spatial resolution the physical processes behind the gamma-ray emission in binaries, significantly increasing as well the number of known sources. This will allow the derivation of information on the particle acceleration and emission sites qualitatively better than what is currently available., Comment: 23 pages, 13 figures, accepted for publication in Astroparticle Physics, special issue on Physics with the Cherenkov Telescope Array
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- 2013
12. Vortex pinning properties of (Y1-xLax)-Ba-Cu-O and (Y1-xPrx)-Ba-Cu-O superconducting bulks
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Naito, T, Sato, K, Yamaguchi, D, and Fujishiro, H
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Irreversibility field ,(Y1-xPrx)–Ba–Cu–O bulk ,(Y1-xLax)–Ba–Cu–O bulk ,Critical current density - Abstract
We have studied the effect of a small amount of Y-site substitution by La or Pr ions on the vortex pinning in the Y–Ba–Cu–O system. (Y1-xLax)–Ba–Cu–O and (Y1-xPrx)–Ba–Cu–O bulks were fabricated by the melt-textured growth, in which x was varied from 0 to 0.01. The critical current density Jc at 77 K is improved in magnetic fields parallel to the c-axis above 2–4.5 T and the corresponding irreversibility field, Hirr, shifts to the higher value in both bulks.
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- 2009
13. A highly efficient 3D micromixer fabricated by standard soft-lithography equipement
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Naito, T., Arayanarakool, Rerngchai, Kaji, N., le Gac, Severine, Tokeshi, M., van den Berg, Albert, Baba, Y., Fujii, T., Hibara, A., Takeuchi, S., and Fukuba, T.
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METIS-293258 ,IR-83541 ,EWI-22718 - Abstract
This paper reports a stereolithography-like 3D fabrication method based on soft-lithography techniques. It only requires standard equipment for photolithography, but it makes true 3D structures fabrication possible. We developed a rotating partition by this method in a microfluidic channel, which cannot be achieved by conventional soft-lithography, and demonstrated a prototyping three-dimensional flow mixer.
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- 2012
14. On-Chip electric power generation system from sound of portable music plyers and smartphones towerd portable uTAS
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Naito, T., Kaji, N., le Gac, Severine, Tokeshi, M., van den Berg, Albert, Baba, Y., Fujii, T., Hibara, A., Takeuchi, S., and Fukuba, T.
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EWI-22751 ,METIS-293270 ,IR-83545 - Abstract
This paper demonstrates electric generation from sound to minimize and integrate microfluidic systems for point of care testing or in-situ analysis. In this work, 5.4 volts and 50 mW DC was generated from sound through an earphone cable, which is a versatile system and able to actuate small size and low power consumption devices like an electro osmotic pump.
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- 2012
15. Possible evidence of tensor interactions in 16O observed via (p,d) reaction
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Ong, H. J., Tanihata, I., Tamii, A., Myo, T., Ogata, K., Fukuda, M., Hirota, K., Ikeda, K., Ishikawa, D., Kawabata, T., Matsubara, H., Matsuta, K., Mihara, M., Naito, T., Nishimura, D., Ogawa, Y., Okamura, H., Ozawa, A., Pang, D. Y., Sakaguchi, H., Sekiguchi, K., Suzuki, T., Taniguchi, M., Takashina, M., Toki, H., Yasuda, Y., Yosoi, M., and Zenihiro, J.
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FOS: Physical sciences ,Nuclear Experiment (nucl-ex) ,Nuclear Experiment - Abstract
We have measured 16O(p,d) reaction using 198-, 295- and 392-MeV proton beams to search for a direct evidence on the effect of the tensor interactions in light nucleus. Differential cross sections of the one-neutron transfer reactions populating the ground states and several low-lying excited states in 15O were measured. Comparing the ratios of the cross sections for each excited state to the one for the ground state over a wide range of momentum transfer, we found a marked enhancement for the positive-parity state(s). The observation indicates large components of high-momentum neutrons in the initial ground-state configurations, due possibly to the tensor interactions., Comment: 11 pages, 2 figures
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- 2012
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16. Simultaneous valence shift of Pr and Tb ions at the spin-state transition in ((Pr$_{1-y}$Tb$_{y})_{0.7}$Ca$_{0.3}$CoO$_{3}$
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Fujishiro, H., Naito, T., Takeda, D., Yoshida, N., Watanabe, T., Nitta, K., Hejtmanek, J., Knizek, K., and Jirak, Z.
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Condensed Matter - Materials Science ,Materials Science (cond-mat.mtrl-sci) ,FOS: Physical sciences - Abstract
Temperature dependence of the X-ray absorption near-edge structure (XANES) spectra at the Pr $L_{3}$- and Tb $L_{3}$-edges was measured for the (Pr$_{1-y}$Tb$_{y})_{0.7}$Ca$_{0.3}$CoO$_{3}$ system, in which a metal-insulator (MI) and spin-state (SS) transition took place simultaneously at a critical temperature $T_{\rm MI}$. A small increase in the valence of the terbium ion was found below $T_{\rm MI}$, besides the enhancement of the praseodymium valence; the trivalent states, which are stable at room temperature, change to a 3+/4+ ionic mixture at low temperatures. In particular for the $y$=0.2 sample, the average valence determined at 8 K amounts to 3.03+ and 3.25+ for the Tb and Pr ion, respectively. In analogous (Pr$_{1-y}$RE$_{y})_{0.7}$Ca$_{0.3}$CoO$_{3}$ samples (RE=Sm and Eu), in which the MI-SS transition also took place, no valence shift of the RE ion was detected in the XANES spectra at the RE ion $L_{3}$-edge. The role of the substituted RE ion for the Pr-site on the MI-SS transition is discussed.
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- 2012
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17. Study of Intrinsic Spin Hall Effect and Orbital Hall Effect in 4d- and 5d- Transition Metals
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Tanaka, T., Kontani, H., Naito, M., Naito, T., Hirashima, D. S., Yamada, K., and Inoue, J.
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Condensed Matter - Strongly Correlated Electrons ,Condensed Matter - Mesoscale and Nanoscale Physics ,Strongly Correlated Electrons (cond-mat.str-el) ,Mesoscale and Nanoscale Physics (cond-mat.mes-hall) ,FOS: Physical sciences ,Condensed Matter::Strongly Correlated Electrons - Abstract
We study the intrinsic spin Hall conductivity (SHC) in various $5d$-transition metals (Ta, W, Re, Os, Ir, Pt, and Au) and 4d-transition metals (Nb, Mo, Tc, Ru, Rh, Pd, and Ag) based on the Naval Research Laboratory tight-binding model, which enables us to perform quantitatively reliable analysis. In each metal, the obtained intrinsic SHC is independent of resistivity in the low resistive regime ($\rho < 50 \mu\Omega\text{cm}$) whereas it decreases in proportion to $\rho^{-2}$ in the high resistive regime. In the low resistive regime, the SHC takes a large positive value in Pt and Pd, both of which have approximately nine $d$-electrons per ion ($n_d=9$). On the other hand, the SHC takes a large negative value in Ta, Nb, W, and Mo where $n_d, Comment: 17 pages, 12 figures, 3 tables, resubmitted to Physical Review B
- Published
- 2007
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18. Mapping the Fermi velocity in the quasi-2D organic conductor k-(BEDT-TTF)2I3
- Author
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Kovalev, A. E., Hill, S., Kawano, K., Tamura, M., Naito, T., and Kobayashi, H.
- Subjects
Condensed Matter - Strongly Correlated Electrons ,Strongly Correlated Electrons (cond-mat.str-el) ,FOS: Physical sciences ,Condensed Matter::Strongly Correlated Electrons - Abstract
We demonstrate a new method for determining the Fermi velocity in quasi-two-dimensional (Q2D) organic conductors. Application of a magnetic field parallel to the conducting layers results in periodic open orbit quasiparticle trajectories along the Q2D Fermi surface. Averaging of this motion over the Fermi surface leads to a resonance in the interlayer microwave conductivity. The resonance frequency is simply related to the extremal value of the Fermi velocity perpendicular to the applied field. Thus, angle dependent microwave studies enable a complete mapping of the Fermi velocity. We illustrate the applicability of this method for the highly-2D organic conductor k-(BEDT-TTF)2I3., Comment: 7 pages, including figures
- Published
- 2003
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19. Intrabeam scattering analysis of measurements at KEK's ATF damping ring
- Author
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Bane, K. L. F., Hayano, H., Kubo, K., Naito, T., Okugi, T., and Urakawa, J.
- Subjects
Accelerator Physics (physics.acc-ph) ,Physics::Accelerator Physics ,FOS: Physical sciences ,Physics - Accelerator Physics - Abstract
We derive a simple relation for estimating the relative emittance growth in x and y due to intrabeam scattering (IBS) in electron storage rings. We show that IBS calculations for the ATF damping ring, when using the formalism of Bjorken-Mtingwa, a modified formalism of Piwinski (where eta squared divided by beta has been replaced by the dispersion invariant), or a simple high-energy approximate formula all give results that agree well. Comparing theory, including the effect of potential well bunch lengthening, with a complete set of ATF steady-state beam size vs. current measurements we find reasonably good agreement for energy spread and horizontal emittance. The measured vertical emittance, however, is larger than theory in both offset (zero current emittance) and slope (emittance change with current). The slope error indicates measurement error and/or additional current-dependent physics at the ATF; the offset error, that the assumed Coulomb log is correct to within a factor of 1.75., Comment: 17 pages, 6 figures, .bbl file
- Published
- 2002
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20. Search for gamma-rays above 10 TeV from Markarian 421 in a high state with the CANGAROO-II telescope
- Author
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Okumura, K., Enomoto, R., Asahara, A., Bicknell, G. V., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Hayashi, S., Itoh, C., Kabuki, S., Kajino, F., Katagiri, H., Kataoka, J., Kawachi, A., Kifune, T., Kubo, H., Kushida, J., Maeda, S., Maeshiro, A., Matsubara, Y., Mizumoto, Y., Mori, M., Moriya, M., Muraishi, H., Muraki, Y., Naito, T., Nakase, T., Nishijima, K., Ohishi, M., Patterson, J. R., Sakurazawa, K., Suzuki, R., Swaby, D. L., Takano, K., Takano, T., Tanimori, T., Tokanaia, F., Tsuchiya, K., Tsunoo, H., Uruma, K., Watanabe, A., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
A preliminary result from Markarian 421 observations in the energy region above 10 TeV with the CANGAROO-II 10 m telescope is presented. In January 2001, the HEGRA group reported that Markarian 421 had become very active, with flux levels up to 4 times that of the Crab Nebula. As a result, we observed Mkn 421 during six nights from January 24th to February 1st, and four nights from March 1st to 4th. Observations were carried out using the very large zenith angle technique ($\sim$70 degree) and the energy threshold is estimated from Monte Carlo simulations to be around 10 TeV. We have detected gamma-ray emission in this energy range., Comment: 4 pages, 5 figures, to appear in Proc. 27th ICRC (Hamburg, Germany)
- Published
- 2001
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21. Multi-bunch generation by thermionic gun
- Author
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Kuriki, M., Hayano, H., Naito, T., and Hasegawa, K.
- Subjects
Accelerator Physics (physics.acc-ph) ,Physics::Accelerator Physics ,FOS: Physical sciences ,Physics - Accelerator Physics - Abstract
KEK-ATF is studying the low-emittance multi-bunch electron beam for the future linear collider. In ATF, thermionic gun is used to generate 20 bunches electron beam with the bunch spacing of 2.8 ns. Due to a distortion of the gun emission and the beam loading effect in the bunching system, the intensity for each bunch is not uniform by up to 40 % at the end of the injector. We have developed a system to correct the gun emission by precisely controlling the cathode voltage with a function generator. For the beam loading effect, we have introduced RF amplitude modulation on Sub Harmonic Buncher, SHB. By these technique, bunch intensity uniformity was improved and beam transmission for later bunches was recovered from 67% to 91%, but intensity for first five bunches is still lower than others., Comment: HEACC01 proceedings
- Published
- 2001
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22. The CANGAROO-III Project: Status report
- Author
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Mori, M., Asahara, A., Bicknell, G. V., Clay, R. W., Edwards, P. G., Enomoto, R., Gunji, S., Hara, S., Hara, T., Hayashi, S., Itoh, C., Kabuki, S., Kajino, F., Katagiri, H., Kawachi, A., Kifune, T., Kubo, H., Kushida, J., Maeda, S., Maeshiro, A., Matsubara, Y., Mizumoto, Y., Muraishi, H., Muraki, Y., Naito, T., Nakase, T., Nishijima, K., Ohishi, M., Okumura, K., Patterson, J. R., Protheroe, R. J., Sakurazawa, K., Suzuki, R., Swaby, D. L., Tanimori, T., Tokanai, F., Tsuchiya, K., Tsunoo, H., Uruma, K., Watanabe, A., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
We report on the status of the construction of an array of four 10 m atmospheric Cherenkov telescopes for gamma-ray astronomy, near Woomera, in South Australia -- the CANGAROO-III project. The first telescope of this array is the upgraded version of the CANGAROO-II 7 m telescope and has been in operation since March 2000. The second telescope, an improved version of the first, is being constructed for installation in late 2001. Stereoscopic observation of sub TeV gamma-rays with the two 10 m telescopes will begin in 2002 and the full array will be operational in 2004., Comment: 4 pages, 7 figures, to appear in Proc. 27th ICRC (Hamburg, Germany)
- Published
- 2001
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23. Study of the TeV gamma-ray spectrum of SN 1006 around the NE Rim
- Author
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Tanimori, T., Naito, T., Yoshida, T., and collaboration, CANGAROO
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
The differential spectrum of TeV gamma rays between 1.5 TeV and 20 TeV from the north-east rim of SN1006 was obtained from the data observed in 1996 and 1997 using the 3.8m CANGAROO \v{C}erenkov telescope. This spectrum matches the model calculated using the Inverse Compton (IC) process with 2.7k Cosmic Microwave Background (CMB). This enables us to estimate the absolute strength of the magnetic field around the shock and the maximum energy of accelerated electrons with the considerable accuracy: the obtained field strength and maximum electron energy are $4\pm1$ $\mu$G and 50 TeV respectively. Also we have detected again the TeV gamma-ray emission from the same position using the 10m CANGAROO-II telescope in 2000, and the preliminary spectrum around 1 TeV region is presented in this conference. The two spectra agree well in the overlapped energy region., Comment: 4pages, 3 figures, to appear in proceedings of 27thICRC (Hamburg, August 7-15, 2001)
- Published
- 2001
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24. Impedance Analysis of Bunch Length Measurements at the ATF Damping Ring
- Author
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Bane, K. L. F., Naito, T., Okugi, T., Qin, Q., and Urakawa, J.
- Subjects
Accelerator Physics (physics.acc-ph) ,Mechanics of Materials ,Mechanical Engineering ,Physics::Accelerator Physics ,FOS: Physical sciences ,Physics - Accelerator Physics ,Electrical and Electronic Engineering ,Condensed Matter Physics ,Electronic, Optical and Magnetic Materials - Abstract
We present energy spread and bunch length measurements at the Accelerator Test Facility (ATF) at KEK, as functions of current, for different ring rf voltages, and with the beam both on and off the coupling resonance. We fit the on-coupling bunch shapes to those of an impedance model consisting of a resistor and an inductor connected in series. We find that the fits are reasonably good, but that the resulting impedance is unexpectedly large., Comment: 9 pages, 5 figures, presented at 10th International Symposium on Applied Electromagnetics and Mechanics (ISEM2001)
- Published
- 2001
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25. Development of rf reference line for the linear collider
- Author
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Naito, T., Ebihara, K., Hayano, H., and Urakawa, J.
- Subjects
High Energy Physics - Experiment (hep-ex) ,Physics::Optics ,FOS: Physical sciences ,High Energy Physics - Experiment - Abstract
The rf distribution system for the linear collider requires stable x-band(11.424GHz) rf phase signal over 25km length. In order to realize the distribution system, a fiber optic link using a phase stabilized optical fiber was tested. The phase stabilized optical fiber has been employed at LEP, KEKB, etc.. This paper describes the hardware system and result of the preliminary test of the feed back system for stabilization of the phase change., Comment: LINAC2000 THA04
- Published
- 2000
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26. Evidence for TeV gamma-ray emission from the shell type SNR RXJ1713.7-3946
- Author
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Muraishi, H., Tanimori, T., Yanagita, S., Yoshida, T., Moriya, M., Kifune, T., Dazeley, S. A., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Kawachi, A., Kubo, H., Matsubara, Y., Mizumoto, Y., Mori, M., Muraki, Y., Naito, T., Nishijima, K., Patterson, J. R., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Tamura, T., and Yoshikoshi, T.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,FOS: Physical sciences ,High Energy Physics::Experiment ,Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
We report the results of TeV gamma-ray observations of the shell type SNR RXJ1713.7-3946 (G347.3-0.5). The discovery of strong non-thermal X-ray emission from the northwest part of the remnant strongly suggests the existence of electrons with energies up to 100 TeV in the remnant, making the SNR a good candidate TeV gamma-ray source. We observed RXJ1713.7-3946 from May to August 1998 with the CANGAROO 3.8m atmospheric imaging Cerenkov telescope and obtained evidence for TeV gamma-ray emission from the NW rim of the remnant with the significance of 5.6 sigma. The observed TeV gamma-ray flux from the NW rim region was estimated to be (5.3 +/- 0.9[statistical] +/- 1.6[systematic]) * 10^{-12} photons cm^{-2} s^{-1} at energies >= 1.8 +/- 0.9 TeV. The data indicate that the emitting region is much broader than the point spread function of our telescope. The extent of the emission is consistent with that of hard X-rays observed by ASCA. This TeV gamma-ray emission can be attributed to the Inverse Compton scattering of the Cosmic Microwave Background Radiation by shock accelerated ultra-relativistic electrons. Under this assumption, a rather low magnetic field of 11 micro gauss is deduced for the remnant from our observation., Accepted for publication by Astronomy and Astrophysics (5 pages, 2 figures)
- Published
- 2000
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27. Bunch Length Measurements at the ATF Damping Ring in April 2000
- Author
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Bane, K. L. F., Naito, T., Okugi, T., and Urakawa, J.
- Subjects
Accelerator Physics (physics.acc-ph) ,Physics::Accelerator Physics ,FOS: Physical sciences ,Physics - Accelerator Physics - Abstract
This report presents bunch length and energy spread measurements performed in April 2000 at the ATF Damping Ring, at KEK. Measurements were performed with the beam on and then off the linear (difference) coupling resonance. Due to strong intra-beam scattering in the ATF ring, the results depended strongly on the coupling., Comment: 15 pages, 13 figures
- Published
- 2000
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- View/download PDF
28. The SNR W28 at TeV Energies
- Author
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Rowell, G. P., Naito, T., Dazeley, S. A., Edwards, P. G., Gunji, S., Hara, T., Holder, J., Kawachi, A., Kifune, T., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Sako, T., Sakurazawa, K., Susukita, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics::Galaxy Astrophysics - Abstract
The southern supernova remnant (SNR)W28 was observed in 1994 and 1995 by the CANGAROO 3.8m telescope in a search formulti-TeV gamma ray emission, using the Cerenkov imaging technique. We obtained upper limits for a variety of point-like and extended features within a +-1 degree-region and briefly discuss these results, together with that of EGRET within the framework of a shock acceleration model of the W28 SNR., 5 pages, 2 figures, to appear in the proceedings of the GeV-TeV Gamma-Ray Astrophysics Workshop, "Towards a Major Atmospheric Cherenkov Detector VI" (Snowbird, Utah, August 13-16, 1999)
- Published
- 1999
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29. Data Acquisition System of the CANGAROO-II Telescope
- Author
-
Mori, M., Dazeley, S. A., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Jinbo, J., Kawachi, A., Kifune, T., Kubo, H., Kushida, J., Matsubara, Y., Mizumoto, Y., Moriya, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Sakurazawa, K., Sato, Y., Susukita, R., Tamura, T., Tanimori, T., Yanagita, S., Yoshida, T., Yoshikoshi, T., and Yuki, A.
- Subjects
Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
The data acquisition system for the new CANGAROO-II 7m telescope is described., Comment: 4 pages, 3 figures, to appear in Proc. 26th ICRC (Salt Lake City), OG 4.3.31
- Published
- 1999
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30. TeV gamma-ray observations of three X-ray selected BL Lacs
- Author
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Roberts, M. D., Mcgee, P., steven dazeley, Edwards, P. G., Hara, T., Holder, J., Kawachi, A., Kifune, T., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Osaki, T., Patterson, J. R., Rowell, G. P., Sako, T., Sakurazawa, K., Susukita, R., Tamura, T., Tanimori, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
Despite extensive surveys of extragalactic TeV gamma-ray candidates only 3 sources have so far been detected. All three are northern hemisphere objects and all three are low-redshift X-ray selected BL Lacs (XBLs). In this paper we present the results of observations of the three nearest southern hemisphere XBLs (PKS0548-322, PKS2005-489 and PKS2155-304) with the CANGAROO 3.8m imaging telescope. During the period of observation we estimate that the threshold of the 3.8m telescope was around 1.5TeV. Searches for both steady and short timescale emission have been performed for each source. Additionally, we are able to monitor the X-ray state of each source on a daily basis and we have made contemporaneous measurements of optical activity for PKS0548-322 and PKS2155-304., Comment: 7 pages + 3 figures. Accepted by Astron. and Astrophys
- Published
- 1999
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31. Observation of Spectrum of TeV Gamma Rays up to 60 TeV from the Crab at the Large Zenith Angles
- Author
-
Sakurazawa, K., Tanimori, T., Dazeley, S. A., Edwards, P. G., Hara, T., Kamei, S., Kifune, T., Kita, R., Konishi, T., Masaike, A., Matsubara, Y., Matsuoka, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
The CANGAROO experiment has observed gamma-ray above 7TeV from the Crab pulsar/nebula at large zenith angle in Woomera, South Australia. We report the CANGAROO data taken in 1992, 1993 and 1995, from which it appears that the energy spectrum extends at least up to 50 TeV. The observed integral spectrum is (8.4+-1.0) x 10^{-13}(E/7 TeV)^(-1.53+-0.15)cm^{-2}s^{-1} between 7 TeV and 50 TeV. In November 1996, the 3.8m mirror was recoated in Australia, and its reflectivity was improved to be about 90% as twice as before. Due to this recoating, the threshold energy of ~4 TeV for gamma rays has been attained in the observation of the Crab at large zenith angle. Here we also report the preliminary result taken in 1996., Comment: 4 pages, 2 figures, LaTeX 2.09 with epsfig.sty, to appear in proceedings of the 25th ICRC, Durban, 1997
- Published
- 1997
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32. Detection of Gamma Rays of Up to 50 TeV From the Crab Nebula
- Author
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Tanimori, T., Sakurazawa, K., Dazeley, S. A., Edwards, P. G., Hara, T., Hayami, Y., Kamei, S., Kita, R., Kifune, T., Konishi, T., Masaike, A., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nishijima, K., Ogio, S., Patterson, J. R., Roberts, M. D., Rowell, G. P., Sako, T., Susukita, R., Suzuki, A., Suzuki, R., Tamura, T., Thornton, G. J., Yanagita, S., Yoshida, T., and Yoshikoshi, T.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,Physics::Accelerator Physics ,FOS: Physical sciences ,High Energy Physics::Experiment ,Astrophysics - Abstract
Gamma rays with energies greater than 7 TeV from the Crab pulsar/nebula have been observed at large zenith angles, using the Imaging Atmospheric Technique from Woomera, South Australia. CANGAROO data taken in 1992, 1993 and 1995 indicate that the energy spectrum extends up to at least 50 TeV, without a change of the index of the power law spectrum. The observed differential spectrum is \noindent $(2.01\pm 0.36)\times 10^{-13}(E/{7 TeV})^{-2.53 \pm 0.18} TeV^{-1}cm^{-2}s^{-1}$ between 7 TeV and 50 TeV. There is no apparent cut-off. The spectrum for photon energies above $\sim$10 TeV allows the maximum particle acceleration energy to be inferred, and implies that this unpulsed emission does not originate near the light cylinder of the pulsar, but in the nebula where the magnetic field is not strong enough to allow pair creation from the TeV photons. The hard gamma-ray energy spectrum above 10 TeV also provides information about the varying role of seed photons for the inverse Compton process at these high energies, as well as a possible contribution of $\pi ^{\circ}$-gamma rays from proton collisions., Comment: 19 pages, 4 figures, LaTeX2.09 with AASTeX 4.0 maros, to appear in Astrophys. J. Lett
- Published
- 1997
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33. OBSERVATIONS ON THE GASTROINTESTINAL MOVEMENTS OF THE TORTOISE (GEOCLEMYS REEVESII) BY MEANS OF THE ABDOMINAL-WINDOW-TECHNIQUE
- Author
-
Naito T, Kameyama H, and Hukuhara T
- Subjects
Physics ,medicine.anatomical_structure ,Geoclemys reevesii ,Physiology ,Aron alpha ,Stomach ,medicine ,Large intestine ,Anatomy ,Coprodaeum ,Small intestine ,Short distance - Abstract
In the tortoise the gastrointestinal movements were observed utilizing theabdominal-window-technique. The results obtained were summarized as follows:(1) So far as the intestine was exposed to the atmosphere both in vivo and in vitro, the intestine was motionless in most cases. On the other hand, the abdominal-window-technique proved to be very useful to observe the gastrointestinal movements.(2) The operation was carried out under the aseptic precuation as follows: First the back of the animal was removed at its left side to make a rectangular window of 8 × 2.5-4 cm, then ovaries and fallopian tubes on the left side were removed and lastly the window thus formed was covered with a 0.2 mm thick, transparent vinyl-plate, being sutured at its border to the back. In addition, the border of the window plate was firmly sticked to the back by means of adhesives, Aron Alpha A and Araldite.(3) a. In the region of the stomach situated just anal to the cardia contractions (stomach peristalses) recurrently started with a time interval of 21 to 32 sec, sweeping down the wall of the stomach with a velocity of 0.5 to 0.9 mm/sec, until they came to an end at the pylorus.b. In the small intestine, there recurrently occurred contraction waves with a time interval of about 45 seconds, traveling analwards with a velocity of about 0.3mm/sec.c. In the large intestine, there were observed two kinds of movements, i.e., antiperistalses as well as mass peristalses. Tn the former contraction waves recurrently started at the anal end (coprodaeum) of the large intestine with a time interval of 18 to 25 sec, propagating oralwards with a velocity of about 1 mm/sec, until they waned rapidly to disappear after propagating only a short distance (about 2 to 3 cm). In the latter powerful contractions occasionally started at the uppermost part of the large intestine to propagate analwards at first slowly with a velocity of about0.15 mm/sec, and then rapidly with a velocity of about 0.5 mm/sec, until they arrived at the proctodaeum to expel a fecal mass 7 to 8 mm thick and 15 mm long.
- Published
- 1975
34. THE MECHANISM OF THE EXPELLING OF THE BILE INTO THE DUODENAL CAVITY
- Author
-
Hukuhara T, Naito T, and Kameyama H
- Subjects
medicine.medical_specialty ,Common bile duct ,Physiology ,Chemistry ,Bile duct ,Stomach ,Anatomy ,Pylorus ,digestive system ,Gastroenterology ,Secretin ,medicine.anatomical_structure ,Internal medicine ,medicine ,Duodenum ,medicine.symptom ,Peristalsis ,Muscle contraction - Abstract
In guinea pigs, rabbits and dogs the movements of the intramurl portion of the common bile duct were studied. The results obtained were summarized as follows.1. The histological examinations revealed that the intramural bile duct was surrounded with muscles which were derived from the external muscle layers of the duodenum.2. The contraction waves which were rhythmically originated in the most proximal part of the duodenum, propagated then to the intramural bile duct to give rise to contractions of it; as a result the bile contained in it was expelled into the duodenal cavity.3. In guinea pigs Auerbach's plexus of the duodenom was continued to that of the intramural bile duct without any interruption.4. From the results described above it may be presumed that the expelling of the bile proceeds as follows: In the full vigor of digestion which continues for 1 to 3 hours after a meal, every time when the stomach peristalsis arrives at the pylorus a small amount of the content is expelled into the duodenum. The content thus expelled stimulates on the one hand the hormonal mechanism concerned with the production of secretin and on the other hand the mucosal intrinsic reflex into action. The former causes an increase of the bile secretion, while the latter an increase of duodenal contraction waves which in turn triggers contractions of the intramural bile duct, both mechanisms thus accelerating the expelling of the bile. When the digestion turns to the declining stage, the bile secretion decreases and contraction waves grow weak; as a result the expelling of the bile decreases. The corollary is that the gall bladder is not regarded as an indispensable organ, although on the one hand it takes a role of the reservoir when the bile secretion is increased to an undue extent and on the other hand it produces an elastic recoil which promotoes the filling of the bile into the intramural bile duct.
- Published
- 1974
35. Studies on Pyocine Typing of Pseudomonas aeruginosa
- Author
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Fukuhara A, Naito T, and Iwanaga Y
- Subjects
Reproducibility ,Pyocine typing ,Pseudomonas aeruginosa ,medicine ,Cross reactions ,General Medicine ,Biology ,medicine.disease_cause ,Microbiology - Published
- 1971
36. Science with the Cherenkov Telescope Array
- Author
-
Cascone, E., Valore, L., Vallania, P., Valentino, M., Vagnetti, F., Vagelli, V., Umana, G., Tsujimoto, S., Pujadas, I., Trifoglio, M., Trichard, C., Travnicek, P., Tovmassian, G., Tothill, N., Tosti, G., Torresi, E., Torres, D., Tornikoski, M., Tonev, D., Tomastik, J., Tokanai, F., Peixoto, C., Tluczykont, M., Tibaldo, L., Tian, W., Thoudam, S., Testa, V., Teshima, M., Terzic, T., Terrier, R., Terada, Y., Temnikov, P., Tejedor, L., Tayabaly, K., Tavernet, J., Tavecchio, F., Tavani, M., Tajima, H., Tagliaferri, G., Supanitsky, A., Suomijarvi, T., Straumann, U., Stratta, G., Stolarczyk, T., Stephan, M., Stefanik, S., Stawarz, Ł., Starling, R., Stanič, S., Stamerra, A., Sol, H., Slowikowska, A., Sliusar, V., Sitarek, J., Sironi, G., Sillanpää, A., Siejkowski, H., Sidoli, L., Shellard, R., Shalchi, A., Servillat, M., Sergijenko, O., Semikoz, D., Seitenzahl, I., Scuderi, S., Sciacca, E., Schwanke, U., Schussler, F., Schulz, A., Schovanek, P., Schoorlemmer, H., Schneider, M., Schlenstedt, S., Schioppa, E., Saturni, F., Satalecka, K., Sarkar, S., Santander, M., Sano, H., Sanguillon, M., Sangiorgi, P., Sandoval, A., Sandaker, H., Sánchez-Conde, M., Salina, G., Sakurai, S., Sakaki, N., Saito, T., Safi-Harb, S., Sadeh, I., Rulten, C., Rugliancich, A., Rudak, B., Rowell, G., Rovero, A., Rosado, J., Romeo, G., Romano, P., Rojas, G., Vázquez, J., Fernandez, G., Rodriguez, J., Rizi, V., Rivoire, S., Riquelme, M., Rieger, F., Rico, J., Richtler, T., Ribó, M., Ribeiro, D., Rhode, W., Rezaeian, A., Renaud, M., Reisenegger, A., Reimer, A., Reimer, O., Razzaque, S., Rainò, S., Quirrenbach, A., Queiroz, F., Pürckhauer, S., Punch, M., Pühlhofer, G., Prouza, M., Prokoph, H., Prokhorov, D., Principe, G., Prast, J., Prandini, E., Pozo, D., Polo, M., Pohl, M., Pita, S., Pisarski, A., Piano, G., Pfeifer, M., Peyaud, B., Petruk, O., Petrucci, P., Petrashyk, A., Persic, M., Perri, M., Pedaletti, G., Pech, M., PeEr, A., Parsons, R., Pareschi, G., Paredes, J., Naito, T., Nagayoshi, T., Nagataki, S., Nagai, A., Murase, K., Muraishi, H., Murach, T., Mundell, C., Mukherjee, R., Moulin, E., Morselli, A., Morris, P., Morlino, G., Mori, K., Morcuende-Parrilla, D., Moralejo, A., Montaruli, T., Mohrmann, L., Mohammed, M., Moderski, R., Mizuno, T., Mitchell, A., Mirzoyan, R., Mirabal, N., Minaya, I., Meyer, M., Mereghetti, S., Melandri, A., Medina, C., Mazin, D., Maxted, N., Maurin, G., Masuda, S., Masetti, N., Martínez, G., Martínez, M., Martin, P., Martí, J., Markoff, S., Marín, J., Marcowith, A., Mangano, S., Manganaro, M., Maneva, G., Mandat, D., Malaguti, G., Majumdar, P., Maier, G., Maccarone, M., Lyard, E., Luque-Escamilla, P., Lucarelli, F., Lu, C., López-Coto, R., López, M., Longo, F., Lombardi, S., Lohse, T., Lindfors, E., Limon, M., Lico, R., Lenain, J., De Oliveira, M., Lefaucheur, J., Lees, J., Leach, S., Blanc, O., Lapington, J., Lang, R., Lamanna, G., La Palombara, N., Kushida, J., Kuroda, H., Mezek, G., Kubo, H., Krauß, F., Krause, M., Kraus, M., Kosack, K., Komin, N., Kohri, K., Koch, B., Knödlseder, J., Knapp, J., Kisaka, S., Kimura, S., Kimeswenger, S., Kieda, D., Khélifi, B., Kazanas, D., Kawanaka, N., Katz, U., Katagiri, H., Karkar, S., Kaaret, P., Jurysek, J., Jung-Richardt, I., Jean, P., Jankowsky, D., Janecek, P., Jamrozy, M., Iwamura, Y., Ishio, K., Iori, M., Ioka, K., Iocco, F., Inoue, Y., Inoue, T., Inoue, S., Inome, Y., Inada, T., Iarlori, M., Hütten, M., Humensky, T., Hrupec, D., Hrabovsky, M., Hovatta, T., Horvath, P., Horns, D., Hörandel, J., Horan, D., Holder, J., Hofmann, W., Hnatyk, B., Hinton, J., Hermann, G., Helo, J., Heller, M., Hayashida, M., Hayashi, K., Hassan, T., Hardcastle, M., Hara, S., Hadasch, D., Gunji, S., Griffiths, S., Greenshaw, T., Green, A., Granot, J., Grandi, P., Graham, J., Götz, D., González, J., González, M., Gómez-Vargas, G., Goldoni, P., Godinovic, N., Gnatyk, R., Glicenstein, J., Giuliani, A., Giroletti, M., Giro, E., Giordano, F., Giommi, P., Giglietto, N., Giavitto, G., Gerard, L., Gaug, M., Gasparetto, T., Gaskins, J., Garczarczyk, M., López, R., Garcia, B., Gallant, Y., Gadola, A., Gabici, S., Füßling, M., Funk, S., Fukazawa, Y., Fujita, Y., Fruck, C., Coromina, L., Fortson, L., Fornasa, M., Fontaine, G., Fioretti, V., Filipovic, M., Fesquet, M., Ferrand, G., Fernández-Barral, A., Fernandez-Alonso, M., Fegan, S., Fedorova, E., Fasola, G., Farnier, C., Falcone, A., Falceta-Goncalves, D., Fairbairn, M., Evoli, C., Espinoza, C., Ernenwein, J., Elsässer, D., Ekoume, T., Einecke, S., Egberts, K., Eckner, C., Ebr, J., Dwarkadas, V., Dubus, G., Dravins, D., Drass, H., Doro, M., Dorner, D., Prester, D., Domínguez, A., Djannati-Ataï, A., Diebold, S., Dib, C., Díaz, C., Di Venere, L., Di Pierro, F., Di Girolamo, T., Della Volpe, D., Delgado, C., Del Santo, M., Deil, C., Covino, S., Cotter, G., Costantini, H., Costa, A., Cortina, J., Contreras, J., Conrad, J., Connaughton, V., Conforti, V., Colin, P., Colafrancesco, S., Coco, V., Cieślar, M., Chudoba, J., Christov, A., Chikawa, M., Chernyakova, M., Chen, X., Chen, A., Chaty, S., Chadwick, P., Cerruti, M., Cauz, D., Catalano, O., Catalani, F., Casanova, S., Carr, J., Carquín, E., Carosi, R., Carlile, C., Cárdenas, V., Caraveo, P., Caproni, A., Capitanio, F., Capalbi, M., Canestrari, R., Busetto, G., Burtovoi, A., Burton, M., Bulik, T., Bulgarelli, A., Bühler, R., Bugaev, V., Buckley, J., Buanes, T., Brunetti, G., Brun, P., Brill, A., Bregeon, J., Braiding, C., Böttcher, M., Bosnjak, Z., Bonnoli, G., Bonavolontà, C., Bonardi, A., Bonanno, G., Bolmont, J., Boisson, C., Blazek, J., Blanch, O., Biteau, J., Bissaldi, E., Biland, A., Bigongiari, C., Biasuzzi, B., Bertucci, B., Bernlöhr, K., Bernardos, M., Bernardini, E., Berge, D., Benbow, W., Belfiore, A., Becherini, Y., Bastieri, D., Barkov, M., Bamba, A., Ballet, J., Ballester, O., Balbo, M., Balazs, C., Backes, M., Ashley, M., Paoletti, R., Palatka, M., Palatiello, M., Paizis, A., Padovani, M., Oya, I., Otte, N., Ostrowski, M., Osborne, J., Orito, R., Orienti, M., Ong, R., Okumura, A., Okazaki, N., Ohm, S., Ohishi, M., Ohira, Y., Oakes, L., OBrien, P., Nozaki, S., Novosyadlyj, B., Nosek, D., Noda, K., Nishijima, K., Nikołajuk, M., Nieto, D., Niemiec, J., Nakamura, Y., Nakamori, T., Asano, K., Arrabito, L., Arqueros, F., Armstrong, T., Araya, M., Aramo, C., Antolini, E., Ambrosi, G., Amato, E., Alispach, C., Alfaro, J., Alfaro, R., Agudo, I., Zhdanov, V.I., Zdziarski, A.A., Williams, D.A., Watson, J.J., Ward, J.E., Wagner, S.J., Vettolani, G.P., Varner, G.S., Torres, D.F., Todero Peixoto, C.J., Tejedor, L.A., Tavernet, J.-P., Supanitsky, A.D., Shellard, R.C., Rovero, A.C., Vázquez, J.J., Rezaeian, A.H., Parsons, R.D., Paredes, J.M., Osborne, J.P., Ong, R.A., De Souza, V., De Persio, F., De Palma, F., Wilhelmi, E., De Naurois, M., De Lucia, M., De Luca, A., De Lotto, B., Lopez, R., De La Calle, I., Pino, E., De Franco, A., De Cesare, G., Anjos, R., De Angelis, A., Dazzi, F., Dawson, B., Davids, I., Daniel, M., DUrso, D., DAvanzo, P., DAmmando, F., DAì, A., Cumani, P., Cuevas, O., Cuadra, J., Crocker, R., Minaya, I.A., Maccarone, M.C., Luque-Escamilla, P.L., Lenain, J.-P., De Oliveira M.A., Leigui, Lees, J.-P., Lang, R.G., Kukec Mezek, G., Kieda, D.B., Humensky, T.B., De Los Reyes Lopez, R., De Gouveia Dal Pino, E.M., Contreras, J.L., Chaves, R.C., Brown, A.M., Schioppa, E.J., Saturni, F.G., Bernardini, M.G., Barrio, J.A., Barres De Almeida, U., Antonelli, L.A., Amans, J.-P., Alves Batista, R., Al Samarai, I., Acharya, B.S., Helo, J.C., Hardcastle, M.J., Green, A.J., González, J.M., González, M.M., Glicenstein, J.-F., Ernenwein, J.-P., Ekoume, T.R., Dwarkadas, V.V., Dominis Prester, D., Chaves, R., Brown, A., Bernardini, M., Barrio, J., De Almeida, U., Antonelli, L., Amans, J., Batista, R., Samarai, I., Acharya, B., Consortium, The Cherenkov, Zorn, J., Ziegler, A., Zhdanov, V., Zechlin, H., Zech, A., Zdziarski, A., Zavrtanik, D., Zavrtanik, M., Zanin, R., Zandanel, F., Zampieri, L., Zaharijas, G., Zacharias, M., Yoshikoshi, T., Yoshiike, S., Yoshida, T., Yang, L., Yanagita, S., Yamazaki, R., Yamamoto, T., Wood, M., Wischnewski, R., Williams, D., Will, M., Wilcox, P., Wierzcholska, A., White, R., White, M., Werner, F., Watson, J., Warren, D., Ward, J., Walter, R., Wagner, R., Wagner, S., Vuillaume, T., Vrastil, M., Vorobiov, S., Vollhardt, A., Voelk, H., Villanueva, J., Vigorito, C., Viana, A., Vettolani, G., Verzi, V., Vergani, S., Veres, P., Vercellone, S., Vega, A., Vecchi, M., Acosta, M., Vassiliev, V., Vasileiadis, G., Varner, G., Vandenbroucke, J., Van Eldik, C., Cherenkov Telescope Array Consortium, The, Acharya, B. S., Agudo, I., Al Samarai, I., Alfaro, R., Alfaro, J., Alispach, C., Alves Batista, R., Amans, J. -P., Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., Barres de Almeida, U., Barrio, J. A., Bastieri, D., Becherini, Y., Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernlöhr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Bosnjak, Z., Böttcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cárdenas, V., Carlile, C., Carosi, R., Carquín, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieślar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Aì, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., de Cássia dos Anjos, R., De Cesare, G., De Franco, A., de Gouveia Dal Pino, E. M., de la Calle, I., de los Reyes Lopez, R., De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., de Oña Wilhelmi, E., De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Díaz, C., Dib, C., Diebold, S., Djannati-Ataï, A., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. N., Elsässer, D., Ernenwein, J. -P., Espinoza, C., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Farnier, C., Fasola, G., Fedorova, E., Fegan, S., Fernandez-Alonso, M., Fernández-Barral, A., Ferrand, G., Fesquet, M., Filipovic, M., Fioretti, V., Fontaine, G., Fornasa, M., Fortson, L., Freixas Coromina, L., Fruck, C., Fujita, Y., Fukazawa, Y., Funk, S., Füßling, M., Gabici, S., Gadola, A., Gallant, Y., Garcia, B., Garcia López, R., Garczarczyk, M., Gaskins, J., Gasparetto, T., Gaug, M., Gerard, L., Giavitto, G., Giglietto, N., Giommi, P., Giordano, F., Giro, E., Giroletti, M., Giuliani, A., Glicenstein, J. -F., Gnatyk, R., Godinovic, N., Goldoni, P., Gómez-Vargas, G., González, M. M., González, J. M., Götz, D., Graham, J., Grandi, P., Granot, J., Green, A. J., Greenshaw, T., Griffiths, S., Gunji, S., Hadasch, D., Hara, S., Hardcastle, M. J., Hassan, T., Hayashi, K., Hayashida, M., Heller, M., Helo, J. C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Hörandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Hütten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khélifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knödlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauß, F., Kubo, H., Kukec Mezek, G., Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Le Blanc, O., Leach, S., Lees, J. -P., Lefaucheur, J., Leigui de Oliveira, M. A., Lenain, J. -P., Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., López, M., López-Coto, R., Lu, C. -C., Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marín, J., Markoff, S., Martí, J., Martin, P., Martínez, M., Martínez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikołajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'Er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, D., Prokoph, H., Prouza, M., Pühlhofer, G., Punch, M., Pürckhauer, S., Queiroz, F., Quirrenbach, A., Rainò, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribó, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodríguez Vázquez, J. J., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpää, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P., Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, S., Tian, W., Tibaldo, L., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Troyano Pujadas, I., Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Vázquez Acosta, M., Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., Zorn, J., Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPP), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CTA Consortium, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (INFN, Sezione di Perugia), Istituto Nazionale di Fisica Nucleare (INFN), Departamento de Física Atómica, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), College of Science and Engineering, Aoyama Gakuin University (AGU), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Istituto di Radioastronomia [Bologna] (IRA), University of Naples Federico II = Università degli studi di Napoli Federico II, Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Padova (OAPD), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ISDC Data Centre for Astrophysics, Université de Genève = University of Geneva (UNIGE), Département de Physique Nucléaire et Corpusculaire [Genève] (DPNC), Universities Space Research Association (USRA), Universidad Complutense de Madrid = Complutense University of Madrid [Madrid] (UCM), INAF - Osservatorio Astronomico di Brera (OAB), Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Fı'sica Generale dell'Università, Istituto Nazionale di Fisica Nucleare, sezione di Bari (INFN, sezione di Bari), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Institut für Theoretische Physik und Astrophysik [Würzburg], Julius-Maximilians-Universität Würzburg (JMU), Jodrell Bank Centre for Astrophysics (JBCA), University of Manchester [Manchester], Institut des sciences du végétal (ISV), Centre National de la Recherche Scientifique (CNRS), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Agenzia Spaziale Italiana (ASI), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Texas A&M University System, Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), Department of Natural Sciences [Ra'anana}, Open University of Israël, University of Hertfordshire [Hatfield] (UH), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Solar-Terrestrial Environment Laboratory [Nagoya] (STEL), Nagoya University, Laboratoire de l'Accélérateur Linéaire (LAL), Radboud University [Nijmegen], Metsähovi Radio Observatory, Aalto University, Humboldt University Of Berlin, The University of Tokyo (UTokyo), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Iowa City], University of Iowa [Iowa City], Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Max-Planck-Institut für Extraterrestrische Physik (MPE), INAF- Milano, Università degli Studi di Udine - University of Udine [Italie], Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), NASA Goddard Space Flight Center (GSFC), Institute for Physical Research (IPR), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Dept. of Physics, University of Wisconsin-Madison, Infrared Processing and Analysis Center (IPAC), California Institute of Technology (CALTECH), KEK (High energy accelerator research organization), Department of Physics [Tokyo], Tokyo Institure of Technology, Istituto di Radioastronomia INAF, Department of Physics and Astronomy [Leicester], University of Leicester, Departament d'Astronomia i Meteorologia [Barcelona] (DAM), Universitat de Barcelona (UB), IEEC-CSIC, INAF - Osservatorio Astronomico di Trieste (OAT), DLR Institut für Physik der Atmosphäre (IPA), Deutsches Zentrum für Luft- und Raumfahrt [Oberpfaffenhofen-Wessling] (DLR), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Centro de Ciencias de la Atmosfera [Mexico], Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Technische Universität Dortmund [Dortmund] (TU), Institut de Ciencies del Cosmos (ICCUB), International Agency for Cancer Research (IACR), School of Chemistry and Physics, University of Adelaide, Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), Polish Academy of Sciences (PAN), Centro de Ciencias Aplicadas y Desarrollo Tecnológico, University of Oxford, AGH University of Science and Technology [Krakow, PL] (AGH UST), Dipartimento di Fisica 'Giuseppe Occhialini' = Department of Physics 'Giuseppe Occhialini' [Milano-Bicocca], Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Department of Plant Sciences [Univ California Davis] (Plant - UC Davis), University of California [Davis] (UC Davis), University of California (UC)-University of California (UC), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institute for Climate and Atmospheric Science [Leeds] (ICAS), School of Earth and Environment [Leeds] (SEE), University of Leeds-University of Leeds, Antarctic Research a European Network for Astrophysics (ARENA), Institute of Atmospheric Physics [Prague] (IAP), Czech Academy of Sciences [Prague] (CAS), University of California (UC), Laboratoire d'études en Géophysique et océanographie spatiales (LEGOS), Instituto Nacional de Técnica Aeroespacial (INTA), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (INFN, Sezione di Trieste), Jozef Stefan Institute [Ljubljana] (IJS), Istituto di Astrofisica Spaziale e Fisica cosmica - Palermo (IASF-Pa), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), National Institute for Nuclear Physics (INFN), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Consejo Superior de Investigaciones Científicas [Spain] (CSIC)-Universitat de València (UV), University of Naples Federico II, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), University of Geneva [Switzerland], Université de Genève (UNIGE), Complutense University of Madrid (UCM), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Bureau d'Économie Théorique et Appliquée (BETA), Institut National de la Recherche Agronomique (INRA)-Université de Strasbourg (UNISTRA)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut für Theoretische Physik und Astrophysik [Wurzburg], Julius-Maximilians-Universität Würzburg [Wurtzbourg, Allemagne] (JMU), Jodrell Bank Centre for Astrophysics, Universitat Autònoma de Barcelona [Barcelona] (UAB), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Helmholtz-Gemeinschaft, Radboud university [Nijmegen], Humboldt Universität zu Berlin, The University of Tokyo, Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' [Rome], National Academy of Sciences of Armenia, CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA, CALTECH, Ctr Infrared Proc & Anal, Pasadena, High Energy Accelerator Research Organization (KEK), University of Tsukuba, Universidad Nacional Autónoma de México (UNAM), University of Oxford [Oxford], Dip. di Fisica 'Occhialini' - Università degli Studi di Milano-Bicocca Piazza della Scienza, Department of Plant Sciences [Davis, CA], University of California-University of California, INAF-OAB, Czech Academy of Sciences [Prague] (ASCR), University of California, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire Midi-Pyrénées (OMP), Observatoire de Paris - Site de Meudon (OBSPM), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Département de Physique des Particules (ex SPP) (DPhP), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Humboldt-Universität zu Berlin, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
- Subjects
propagation [photon] ,photon: propagation ,Cherenkov Telescope Array ,magnetic field ,01 natural sciences ,thermal ,Observatory ,formation [star] ,HESS ,site ,cluster ,ddc:522.6862 ,media_common ,pulsar ,High Energy Astrophysical Phenomena (astro-ph.HE) ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::Instrumentation and Methods for Astrophysics ,star: formation ,relativistic [jet] ,CERN LHC Coll ,binary [gamma ray] ,cosmic radiation [electron] ,axion-like particles ,violation ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,performance ,Astrophysics and Astronomy ,bepress|Physical Sciences and Mathematics|Physics ,media_common.quotation_subject ,Astrophysics::High Energy Astrophysical Phenomena ,burst [gamma ray] ,Higgs particle ,invariance: Lorentz ,X-ray ,ionization ,supernova ,cosmic radiation: UHE ,Lorentz [invariance] ,AGN ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,CTA ,010308 nuclear & particles physics ,Astronomy ,sensitivity ,Universe ,angular resolution ,gamma ray: VHE ,quantum gravity ,galaxy ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,HAWC ,Computer science ,VHE [gamma ray] ,feedback ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,ultraviolet ,black hole ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,cloud ,acceleration [hadron] ,neutron star ,010303 astronomy & astrophysics ,astro-ph.HE ,radio wave ,COSMIC cancer database ,imaging ,observatory ,Supernova ,annihilation ,bepress|Physical Sciences and Mathematics|Physics|Elementary Particles and Fields and String Theory ,infrared ,Particle Physics - Experiment ,accelerator ,WIMP ,Ground-based gamma-ray astronomy ,Dark matter ,UHE [cosmic radiation] ,FOS: Physical sciences ,gamma ray: burst ,GLAST ,dark matter ,jet: relativistic ,blazar ,target ,hadron: acceleration ,0103 physical sciences ,522.6862 ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,TeV gamma-ray astronomy ,hep-ex ,Gravitational wave ,background ,gravitational radiation ,electron: cosmic radiation ,gamma ray: binary ,redshift ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,monitoring ,Sky ,bepress|Physical Sciences and Mathematics|Astrophysics and Astronomy ,astro-ph.IM - Abstract
Singapur : WORLD SCIENTIFIC, Cherenkov Telescope Array (CTA) 211 pp. (2017). doi:10.1142/10986, The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. CTA is an explorer of the extreme universe, probing environments from the immediate neighbourhood of black holes to cosmic voids on the largest scales. Covering a huge range in photon energy from 20 GeV to 300 TeV, CTA will improve on all aspects of performance with respect to current instruments. The observatory will operate arrays on sites in both hemispheres to provide full sky coverage and will hence maximize the potential for the rarest phenomena such as very nearby supernovae, gamma-ray bursts or gravitational wave transients. With 99 telescopes on the southern site and 19 telescopes on the northern site, flexible operation will be possible, with sub-arrays available for specific tasks. CTA will have important synergies with many of the new generation of major astronomical and astroparticle observatories. Multi-wavelength and multi-messenger approaches combining CTA data with those from other instruments will lead to a deeper understanding of the broad-band non-thermal properties of target sources. The CTA Observatory will be operated as an open, proposal-driven observatory, with all data available on a public archive after a pre-defined proprietary period. Scientists from institutions worldwide have combined together to form the CTA Consortium. This Consortium has prepared a proposal for a Core Programme of highly motivated observations. The programme, encompassing approximately 40% of the available observing time over the first ten years of CTA operation, is made up of individual Key Science Projects (KSPs), which are presented in this document., Published by WORLD SCIENTIFIC, Singapur
37. Increase of the yield of DNA from barley nuclei in ethylene glycol by gamma-irradiation
- Author
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Naito T and Yamaguchi H
- Subjects
Cell Nucleus ,Radiation ,Chemistry ,food and beverages ,Hordeum ,DNA ,γ irradiation ,chemistry.chemical_compound ,Gamma Rays ,Yield (chemistry) ,Seeds ,Organic chemistry ,Ethylene Glycols ,Edible Grain ,Ethylene glycol ,Nuclear chemistry ,Gamma irradiation ,Macromolecule - Abstract
After gamma-irradiating the nuclei isolated from dry seed-embryo of barley in the presence of varying concentrations of ethylene glycol, macromolecular DNA (deoxyribonucleic acid) was extracted from them. The yields of DNA was determined by the 2 methods. The both method of determination on DNA showed a similar tendency; the higher the exposed dose and the concentration of ethylene glycol, the better the yields.
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38. Status of ATF2 IP-BPM project
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Blanco, O. R., Bambade, P., Bogard, F., Cornebise, P., Wallon, S., Blaskovic Kraljevic, N., Bett, D. R., Bromwich, T., Burrows, P. N., Christian, G. B., Perry, C., Araki, S., Yosuke Honda, Kubo, K., Kuroda, S., Naito, T., Okugi, T., Tauchi, T., Terunuma, N., Kim, E. -S, and Jang, S.
39. ESICM LIVES 2016: part three : Milan, Italy. 1-5 October 2016
- Author
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Velasquez, T., Mackey, G., Lusk, J., Kyle, Ug, Fontenot, T., Marshall, P., Shekerdemian, Ls, Coss-Bu, Ja, Nishigaki, A., Yatabe, T., Tamura, T., Yamashita, K., Yokoyama, M., Ruiz-Rodriguez, Jc, Encina, B., Belmonte, R., Troncoso, I., Tormos, P., Riveiro, M., Baena, J., Sanchez, A., Bañeras, J., Cordón, J., Duran, N., Ruiz, A., Caballero, J., Nuvials, X., Riera, J., Serra, J., Rutten, Am, Ieperen, Sn, Kinderen, Ep, Logten, T., Kovacikova, L., Skrak, P., Zahorec, M., Akcan-Arikan, A., Silva, Jc, Goldsworthy, M., Wood, D., Harrison, D., Parslow, R., Davis, P., Pappachan, J., Goodwin, S., Ramnarayan, P., Chernyshuk, S., Yemets, H., Zhovnir, V., Pulitano, Sm, Rosa, S., Mancino, A., Villa, G., Tosi, F., Franchi, P., Conti, G., Patel, B., Khine, H., Shah, A., Sung, D., Singer, L., Haghbin, S., Inaloo, S., Serati, Z., Idei, M., Nomura, T., Yamamoto, N., Sakai, Y., Yoshida, T., Matsuda, Y., Yamaguchi, Y., Takaki, S., Yamaguchi, O., Goto, T., Longani, N., Medar, S., Abdel-Aal, Ir, El Adawy, As, Mohammed, Hm, Mohamed, An, Parry, Sm, Knight, Ld, Denehy, L., Morton, N., Baldwin, Ce, Sani, D., Kayambu, G., Da Silva, Vz, Phongpagdi, P., Puthucheary, Za, Granger, Cl, Rydingsward, Je, Horkan, Cm, Christopher, Kb, Mcwilliams, D., Jones, C., Reeves, E., Atkins, G., Snelson, C., Aitken, Lm, Rattray, J., Kenardy, J., Hull, Am, Ullman, A., Le Brocque, R., Mitchell, M., Davis, C., Macfarlane, B., Azevedo, Jc, Rocha, Ll, Freitas, Ff, Cavalheiro, Am, Lucinio, Nm, Lobato, Ms, Ebeling, G., Kraegpoeth, A., Laerkner, E., Brito-Ashurst, I., White, C., Gregory, S., Forni, Lg, Flowers, E., Curtis, A., Wood, Ca, Siu, K., Venkatesan, K., Muhammad, Jb, Ng, L., Seet, E., Baptista, N., Escoval, A., Tomas, E., Agrawal, R., Mathew, R., Varma, A., Dima, E., Charitidou, E., Perivolioti, E., Pratikaki, M., Vrettou, C., Giannopoulos, A., Zakynthinos, S., Routsi, C., Atchade, E., Houzé, S., Jean-Baptiste, S., Thabut, G., Genève, C., Tanaka, S., Lortat-Jacob, B., Augustin, P., Desmard, M., Montravers, P., Molina, Fj, Barbadillo, S., Alejandro, R., Álvarez-Lerma, F., Vallés, J., Catalán, Rm, Palencia, E., Jareño, A., Granada, Rm, Ignacio, Ml, Getgag, Working Group, Cui, N., Liu, D., Wang, H., Su, L., Qiu, H., Li, R., Jaffal, K., Rouzé, A., Poissy, J., Sendid, B., Nseir, S., Paramythiotou, E., Rizos, M., Frantzeskaki, F., Antoniadou, A., Vourli, S., Zerva, L., Armaganidis, A., Gottlieb, J., Greer, M., Wiesner, O., Martínez, M., Acuña, M., Rello, J., Welte, T., Mignot, T., Soussi, S., Dudoignon, E., Ferry, A., Chaussard, M., Benyamina, M., Alanio, A., Touratier, S., Chaouat, M., Lafaurie, M., Mimoun, M., Mebazaa, A., Legrand, M., Sheils, Ma, Patel, C., Mohankumar, L., Akhtar, N., Noriega, Sk, Aldana, Nn, León, Jl, Baquero, Jd, Bernal, Ff, Ahmadnia, E., Hadley, Js, Millar, M., Hall, D., Hewitt, H., Yasuda, H., Sanui, M., Komuro, T., Kawano, S., Andoh, K., Yamamoto, H., Noda, E., Hatakeyama, J., Saitou, N., Okamoto, H., Kobayashi, A., Takei, T., Matsukubo, S., Jseptic, Clinical Trial Group, Rotzel, Hb, Lázaro, As, Prada, Da, Gimillo, MR, Barinas, Od, Cortes, Ml, Franco, Jf, Roca, Jm, Carratalá, A., Gonçalves, B., Turon, R., Mendes, A., Miranda, F., Mata, Pj, Cavalcanti, D., Melo, N., Lacerda, P., Kurtz, P., Righy, C., Rosario, Le, Lesmes, Sp, Romero, Jc, Herrera, An, Pertuz, Ed, Sánchez, Mj, Sanz, Er, Hualde, Jb, Hernández, Aa, Irazabal, Jm, Spatenkova, V., Bradac, O., Suchomel, P., Urli, T., Lazzeri, Eh, Aspide, R., Zanello, M., Perez-Borrero, L., Garcia-Alvarez, Jm, Arias-Verdu, Md, Aguilar-Alonso, E., Rivera-Fernandez, R., Mora-Ordoñez, J., La Fuente-Martos, C., Castillo-Lorente, E., Guerrero-Lopez, F., Ramírez, Jr, León, Jp, Navarro-Guillamón, L., Cordovilla-Guardia, S., Iglesias-Santiago, A., Guerrero-López, F., Fernández-Mondéjar, E., Vidal, A., Perez, M., Juez, A., Arias, N., Colino, L., Perez, Jl, Pérez, H., Calpe, P., Alcala, Ma, Robaglia, D., Perez, C., Lan, Sk, Cunha, Mm, Moreira, T., Santos, F., Lafuente, E., Fernandes, Mj, Silva, Jg, Echeverría, Jg, Podlepich, V., Sokolova, E., Alexandrova, E., Lapteva, K., Shuinotsuka, C., Rabello, L., Vianna, G., Reis, A., Cairus, C., Salluh, J., Bozza, F., Torres, Jc, Araujo, Nj, García-Olivares, P., Keough, E., Dalorzo, M., Tang, Lk, Sousa, I., Díaz, M., Marcos-Zambrano, Lj, Guerrero, Je, Gomez, Se, Lopez, Gd, Cuellar, Ai, Nieto, Or, Gonzalez, Ja, Bhasin, D., Rai, S., Singh, H., Gupta, O., Bhattal, Mk, Sampley, S., Sekhri, K., Nandha, R., Aliaga, Fa, Olivares, F., Appiani, F., Farias, P., Alberto, F., Hernández, A., Pons, S., Sonneville, R., Bouadma, L., Neuville, M., Mariotte, E., Radjou, A., Lebut, J., Chemam, S., Voiriot, G., Dilly, Mp, Mourvillier, B., Dorent, R., Nataf, P., Wolff, M., Timsit, Jf, Ediboglu, O., Ataman, S., Ozkarakas, H., Kirakli, C., Vakalos, A., Avramidis, V., Obukhova, O., Kurmukov, Ia, Kashiya, S., Golovnya, E., Baikova, Vn, Ageeva, T., Haritydi, T., Kulaga, Ev, Rios-Toro, Jj, Lopez-Caler, C., Rodriguez-Fernandez, S., Sanchez-Orézzoli, Mg, Martin-Gallardo, F., Nikhilesh, J., Joshi, V., Villarreal, E., Ruiz, J., Gordon, M., Quinza, A., Gimenez, J., Piñol, M., Castellanos, A., Ramirez, P., Jeon, Yd, Jeong, Wy, Kim, Mh, Jeong, Iy, Ahn, My, Ahn, Jy, Han, Sh, Choi, Jy, Song, Yg, Kim, Jm, Ku, Ns, Shah, H., Kellner, F., Rezai, F., Mistry, N., Yodice, P., Ovnanian, V., Fless, K., Handler, E., Alejos, Rm, Romeu, Jd, Antón, Dg, Quinart, A., Martí, At, Laura Navarro Guillamon, Lobo-Civico, A., Ventura-Rosado, A., Piñol-Tena, A., Pi-Guerrero, M., Paños-Espinosa, C., Peralvo-Bernat, M., Marine-Vidal, J., Gonzalez-Engroba, R., Montesinos-Cerro, N., Treso-Geira, M., Valeiras-Valero, A., Martinez-Reyes, L., Sandiumenge, A., Jimenez-Herrera, Mf, Capcri, Study, Helyar, S., Riozzi, P., Noon, A., Hallows, G., Cotton, H., Keep, J., Hopkins, Pa, Taggu, A., Renuka, S., Sampath, S., Rood, Pj, Frenzel, T., Verhage, R., Bonn, M., Pickkers, P., Hoeven, Jg, Den Boogaard, M., Corradi, F., Melnyk, L., Moggia, F., Pienovi, R., Adriano, G., Brusasco, C., Mariotti, L., Lattuada, M., Bloomer, Mj, Coombs, M., Ranse, K., Endacott, R., Maertens, B., Blot, K., Blot, S., Amerongen, Mp, Heiden, Es, Twisk, Jw, Girbes, Ar, Spijkstra, Jj, Bell, C., Peters, K., Feehan, A., Churchill, K., Hawkins, K., Brook, R., Paver, N., Maistry, N., Wijk, A., Rouw, N., Galen, T., Evelein-Brugman, S., Krishna, B., Putzu, A., Fang, M., Berto, Mb, Belletti, A., Cassina, T., Cabrini, L., Mistry, M., Alhamdi, Y., Welters, I., Abrams, St, Toh, Ch, Han, Hs, Gil, Em, Lee, Ds, Park, Cm, Winder-Rhodes, S., Lotay, R., Doyle, J., Ke, Mw, Huang, Wc, Chiang, Ch, Hung, Wt, Cheng, Cc, Lin, Kc, Lin, Sc, Chiou, Kr, Wann, Sr, Shu, Cw, Kang, Pl, Mar, Gy, Liu, Cp, Dubó, S., Aquevedo, A., Jibaja, M., Berrutti, D., Labra, C., Lagos, R., García, Mf, Ramirez, V., Tobar, M., Picoita, F., Peláez, C., Carpio, D., Alegría, L., Hidalgo, C., Godoy, K., Bakker, J., Hernández, G., Sadamoto, Y., Katabami, K., Wada, T., Ono, Y., Maekawa, K., Hayakawa, M., Sawamura, A., Gando, S., Marin-Mateos, H., Perez-Vela, Jl, Garcia-Gigorro, R., Peiretti, Ma, Lopez-Gude, Mj, Chacon-Alves, S., Renes-Carreño, E., Montejo-González, Jc, Parlevliet, Kl, Touw, Hr, Beerepoot, M., Boer, C., Elbers, Pw, Tuinman, Pr, Abdelmonem, Sa, Helmy, Ta, El Sayed, I., Ghazal, S., Akhlagh, Sh, Masjedi, M., Hozhabri, K., Kamali, E., Zýková, I., Paldusová, B., Sedlák, P., Morman, D., Youn, Am, Ohta, Y., Sakuma, M., Bates, D., Morimoto, T., Su, Pl, Chang, Wy, Lin, Wc, Chen, Cw, Facchin, F., Zarantonello, F., Panciera, G., Cassai, A., Venrdramin, A., Ballin, A., Tonetti, T., Persona, P., Ori, C., Del Sorbo, L., Rossi, S., Vergani, G., Cressoni, M., Chiumello, D., Chiurazzi, C., Brioni, M., Algieri, I., Guanziroli, M., Colombo, A., Tomic, I., Crimella, F., Carlesso, E., Gasparovic, V., Gattinoni, L., Neto, As, Schmidt, M., Pham, T., Combes, A., Abreu, Mg, Pelosi, P., Schultz, Mj, Prove, Reva Research Network And The Network Investigators, Katira, Bh, Engelberts, D., Giesinger, Re, Ackerley, C., Zabini, D., Otulakowski, G., Post, M., Kuebler, Wm, Mcnamara, Pj, Kavanagh, Bp, Pirracchio, R., Rigon, MR, Carone, M., Chevret, S., Annane, D., Eladawy, S., El-Hamamsy, M., Bazan, N., Elgendy, M., Pascale, G., Vallecoccia, Ms, Cutuli, Sl, Di Gravio, V., Pennisi, Ma, Antonelli, M., Andreis, Dt, Khaliq, W., Singer, M., Hartmann, J., Harm, S., Carmona, Sa, Almudevar, Pm, Abellán, An, Ramos, Jv, Pérez, Lp, Valbuena, Bl, Sanz, Nm, Simón, If, Arrigo, M., Feliot, E., Deye, N., Cariou, A., Guidet, B., Jaber, S., Leone, M., Resche-Rigon, M., Baron, Av, Gayat, E., Frog Icu, Investigators, Balik, M., Kolnikova, I., Maly, M., Waldauf, P., Tavazzi, G., Kristof, J., Herpain, A., Su, F., Post, E., Taccone, F., Vincent, Jl, Creteur, J., Lee, C., Hatib, F., Jian, Z., Buddi, S., Cannesson, M., Fileković, S., Turel, M., Knafelj, R., Gorjup, V., Stanić, R., Gradišek, P., Cerović, O., Mirković, T., Noč, M., Tirkkonen, J., Hellevuo, H., Olkkola, Kt, Hoppu, S., Chiang, Cc, Juan, Wc, Lin, Ph, Fong, Ky, Hou, Ds, Chen, Ys, Paul, M., Bougouin, W., Geri, G., Dumas, F., Champigneulle, B., Legriel, S., Charpentier, J., Mira, Jp, Sandroni, C., Zimmerman, J., Sullivan, E., Noursadeghi, M., Fox, B., Sampson, D., Mchugh, L., Yager, T., Cermelli, S., Seldon, T., Bhide, S., Brandon, Ra, Brandon, Rb, Zwaag, J., Beunders, R., Kox, M., Gul, F., Arslantas, Mk, Genc, D., Zibandah, N., Topcu, L., Akkoc, T., Cinel, I., Greco, E., Lauretta, Mp, Garcia, Ip, Cordero, M., Martin, Ad, Pallás, Ta, Montero, Jg, Rey, Jr, Malo, Lr, Montoya, Aa, Martinez, Ad, Ayala, Ly, Zepeda, Em, Granillo, Jf, Sanchez, Ja, Alejo, Gc, Cabrera, Ar, Montenegro, Ap, Beduneau, G., Schortgen, F., Piquilloud, L., Zogheib, E., Jonas, M., Grelon, F., Runge, I., Terzi, N., Grangé, S., Barberet, G., Guitard, Pg, Frat, Jp, Constan, A., Chrétien, Jm, Mancebo, J., Mercat, A., Richard, Jc, Brochard, L., Wind, Study Group, Soilemezi, E., Koco, E., Savvidou, S., Nouris, C., Matamis, D., Plug Working Group, Di Mussi, R., Spadaro, S., Volta, Ca, Mariani, M., Colaprico, A., Antonio, C., Bruno, F., Grasso, S., Rodriguez, A., Martín-Loeches, I., Díaz, E., Masclans, Jr, Gordo, F., Solé-Violán, J., Bodí, M., Avilés-Jurado, Fx, Trefler, S., Magret, M., Reyes, Lf, Marín-Corral, J., Yebenes, Jc, Esteban, A., Anzueto, A., Aliberti, S., Restrepo, Mi, GETGAG/SEMICYUC, Larsson, Js, Redfors, B., Ricksten, Se, Haines, R., Powell-Tuck, J., Leonard, H., Ostermann, M., Berthelsen, Re, Itenov, Ts, Perner, A., Jensen, Ju, Ibsen, M., Jensen, Ae, Bestle, Mh, Bucknall, T., Dixon, J., Boa, F., Macphee, I., Philips, Bj, Aki, Research Group, St George’s University of London, Saadat, F., Samuels, T., Huddart, S., Mccormick, B., Debrunnar, R., Preece, J., Swart, M., Peden, C., Richardson, S., Forni, L., Kalfon, P., Baumstarck, K., Estagnasie, P., Geantot, Ma, Berric, A., Simon, G., Floccard, B., Signouret, T., Boucekine, M., Fromentin, M., Nyunga, M., Sossou, A., Venot, M., Robert, R., Follin, A., Renault, A., Garrouste, M., Collange, O., Levrat, Q., Villard, I., Thévenin, D., Pottecher, J., Patrigeon, Rg, Revel, N., Vigne, C., Mimoz, O., Auquier, P., Iprea, Study Group, Pawar, S., Jacques, T., Deshpande, K., Pusapati, R., Wood, B., Pulham, Ra, Wray, J., Brown, K., Pierce, C., Nadel, S., Azevedo, Jr, Montenegro, Ws, Rodrigues, Dp, Sousa, Sc, Araujo, Vf, Leitao, Al, Prazeres, Ph, Mendonca, Av, Paula, Mp, Das Neves, A., Loudet, Ci, Busico, M., Vazquez, D., Villalba, D., Lischinsky, A., Veronesi, M., Emmerich, M., Descotte, E., Juliarena, A., Bisso, Mc, Grando, M., Tapia, A., Camargo, M., Ulla, Dv, Corzo, L., Dos Santos, Hp, Ramos, A., Doglia, Ja, Estenssoro, E., Carbonara, M., Magnoni, S., Donald, Cl, Shimony, Js, Conte, V., Triulzi, F., Stretti, F., Macrì, M., Snyder, Az, Stocchetti, N., Brody, Dl, Shimanskiy, V., Savin, I., Chumaev, A., Tjepkema-Cloostermans, Mc, Hofmeijer, J., Beishuizen, A., Hom, H., Blans, Mj, Putten, Mj, Longhi, L., Frigeni, B., Curinga, M., Mingone, D., Beretta, S., Patruno, A., Gandini, L., Vargiolu, A., Ferri, F., Ceriani, R., Rottoli, MR, Lorini, L., Citerio, G., Pifferi, S., Battistini, M., Cordolcini, V., Agarossi, A., Di Rosso, R., Ortolano, F., Lourido, Cm, Cabrera, Jl, Santana, Jd, Alzola, Lm, Del Rosario, Cg, Pérez, Hr, Torrent, Rl, Eslami, S., Dalhuisen, A., Fiks, T., Hanna, Aa, Spronk, Pe, Wood, M., Maslove, D., Muscedere, J., Scott, Sh, Saha, T., Hamilton, A., Petsikas, D., Payne, D., Boyd, Jg, Mcnelly, As, Rawal, J., Connolly, B., Mcphail, Mj, Sidhu, P., Rowlerson, A., Moxham, J., Harridge, Sd, Hart, N., Montgomery, He, Jovaisa, T., Thomas, B., Gupta, D., Wijayatilake, Ds, Shum, Hp, King, Hs, Chan, Kc, Tang, Kb, Yan, Ww, Arias, Cc, Latorre, J., La Rica, As, Garrido, Em, Feijoo, Am, Gancedo, Ch, Tofiño, Al, Rodríguez, Fg, Gemmell, Lk, Campbell, R., Doherty, P., Mackay, A., Singh, N., Vitaller, S., Nagib, H., Prieto, J., Del Arco, A., Zayas, B., Gomez, C., Tirumala, S., Pasha, Sa, Kumari, Bk, Martinez-Lopez, P., Puerto-Morlán, A., Nuevo-Ortega, P., Pujol, Lm, Dolset, Ra, González, Bs, Riera, Sq, Álvarez, Jt, Quintana, S., Martínez, L., Algarte, R., Sánchez, B., Trenado, J., Brock, N., Viegas, E., Filipe, E., Cottle, D., Traynor, T., Martínez, Mv, Márquez, Mp, Gómez, Lc, Martínez, Na, Muñoz, Jm, Bellver, Bq, Varea, Mm, Llorente, Má, Calvo, Cp, Hillier, Sd, Faulds, Mc, Hendra, H., Lawrence, N., Kodate, A., Tominaga, N., Mizugaki, A., Murakami, H., Silva, S., Kerhuel, L., Malagurski, B., Chabanne, R., Laureys, S., Puybasset, L., Nobile, L., Pognuz, Er, Rossetti, Ao, Verginella, F., Gaspard, N., Ben-Hamouda, N., Oddo, M., Taccone, Fs, Iijima, H., Andersen, Lw, Raymond, T., Berg, R., Nadkarni, V., Grossestreuer, A., Kurth, T., Donnino, M., Krüger, A., Ostadal, P., Janotka, M., Vondrakova, D., Kongpolprom, N., Cholkraisuwat, J., Pekkarinen, Pt, Ristagno, G., Masson, S., Latini, R., Bendel, S., Ala-Kokko, T., Varpula, T., Vaahersalo, J., Tiainen, M., Mion, Mm, Plebani, M., Pettilä, V., Skrifvars, Mb, Finnresusci, Study Group, Son, Y., Kim, Ks, Suh, Gj, Kwon, Wy, Ko, Ji, Park, Mj, Cavicchi, Fz, Iesu, E., Tanaka, H., Otani, N., Ode, S., Ishimatsu, S., Romero, I., Martínez, F., Kruger, A., Malek, F., Neuzil, P., Yeh, Yc, Wang, Ch, Huang, Ch, Chao, A., Lee, Ct, Lai, Ch, Chan, Ws, Cheng, Yj, Sun, Wz, Kaese, S., Horstmann, C., Lebiedz, P., Mourad, M., Gaudard, P., Eliet, J., Zeroual, N., Colson, P., Mlcek, M., Hrachovina, M., Mates, M., Hala, P., Kittnar, O., Jacky, A., Rudiger, A., Spahn, Dr, Bettex, Da, Kara, A., Akin, S., Dos Reis Miranda, D., Struijs, A., Caliskan, K., Thiel, Rj, Dubois, Ea, Wilde, W., Zijlstra, F., Gommers, D., Ince, C., Marca, L., Xini, A., Mongkolpun, W., Cordeiro, Cp, Leite, Rt, Lheureux, O., Bader, A., Rincon, L., Santacruz, C., Preiser, Jc, Chao, As, Kim, W., Ahn, C., Cho, Y., Lim, Th, Oh, J., Choi, Ks, Jang, Bh, Ha, Jk, Mecklenburg, A., Stamm, J., Soeffker, G., Kubik, M., Sydow, K., Reichenspurner, H., Kluge, S., Braune, S., Bergantino, B., Ruberto, F., Magnanimi, E., Privato, E., Zullino, V., Bruno, K., Pugliese, F., Sales, G., Girotto, V., Vittone, F., Brazzi, L., Fritz, C., Kimmoun, A., Vanhuyse, F., Trifan, B., Orlowski, S., Albuisson, E., Tran, N., Levy, B., Chhor, V., Joachim, J., Chatelon, J., Fave, G., Mantz, J., Diaz, Dd, Villanova, M., Aguirregabyria, M., Andrade, G., López, L., John, G., Cowan, R., Hart, R., Lake, K., Litchfield, K., Song, Jw, Lee, Yj, Cho, Yj, Choi, S., Vermeir, P., Vandijck, D., Mariman, A., Verhaeghe, R., Deveugele, M., Vogelaers, D., Chok, L., Bachli, Eb, Bettex, D., Cottini, Sr, Keller, E., Maggiorini, M., Schuepbach, R., Stiphout, C., Grevelink, M., Vaneker, I., Ruijter, A., Buise, M., Tena, Sa, Barrachina, Lg, Portillo, Jh, Aznar, Gp, Campos, Lm, Sellés, Md, Tomás, Ma, Muncharaz, Ab, Skinner, L., Monsalvo, S., Olavarria, E., Stümpfle, R., Na, Sj, Park, J., Chung, Cr, Suh, Gy, Yang, Jh, Witter, T., Brousseau, C., Butler, Mb, Erdogan, M., Dougall, Pc, Green, Rs, Abbott, Te, Torrance, Hd, Cron, N., Vaid, N., Emmanuel, J., Siddiqui, Ss, Prabu, N., Chaudhari, Hk, Patil, Vp, Divatia, Jv, Solanki, S., Kulkarni, Ap, Gutierrez, La, Brasseur, A., Hempel, D., Stauffert, N., Recker, F., Schröder, T., Reusch, S., Schleifer, J., Breitkreutz, R., Sjövall, F., Møller, Mh, Moraes, Rb, Borges, Fk, Guillen, Ja, Zabaletta, Wj, Pics- Hcpa, Programa Intrahospitalar Combate À Sepse Do Hospital Clínicas Porto Alegre, Ruiz-Ramos, J., Marqués-Miñana, MR, Sosa, M., Concha, P., Menendez, R., Ramírez, Cs, Santana, Mc, Balcázar, Lc, Escalada, Sh, Viera, Ma, Vázquez, Cf, Díaz, Jj, Campelo, Fa, Monroy, Ns, Santana, Ps, Santana, Sr, Gutiérrez-Pizarraya, A., Garnacho-Montero, J., Martin, C., Mainardi, Jl, Cholley, B., Hubbard, A., Frontera, Pr, Vega, Lm, Miguelena, Pr, Usón, Mc, López, Ar, Clemente, Ea, Ibañes, Pg, Aguilar, Al, Palomar, M., Olaechea, P., Uriona, S., Vallverdu, M., Catalan, M., Aragon, C., Lerma, Fa, Envin-Helics, Study Group, Bassi, Gl, Xiol, Ea, Senussi, T., Idone, Fa, Motos, A., Travierso, C., Fernández-Barat, L., Amaro, R., Hua, Y., Ranzani, Ot, Bobi, Q., Rigol, M., Torres, A., Fernández, If, Soler, Ea, Vera, Ap, Pastor, Ee, Hernandis, V., Ros Martínez, J., Rubio, Rj, Torner, Mm, Brugger, Sc, Eroles, Aa, Moles, Si, Cabello, Jt, Schoenenberger, Ja, Casals, Xn, Vidal, Mv, Garrido, Bb, Martinez, Mp, Mirabella, L., Cotoia, A., Tullo, L., Stella, A., Di Bello, F., Di Gregorio, A., Dambrosio, M., Cinnella, G., Ramirez, Jr, Takahashi, H., Kazutoshi, F., Okada, Y., Oobayashi, W., Naito, T., Baidya, Dk, Maitra, S., Anand, Rk, Ray, Br, Arora, Mk, Ruffini, C., Rota, L., Corona, A., Sesana, G., Ravasi, S., Catena, E., Naumann, Dn, Mellis, C., Husheer, Sl, Bishop, J., Midwinter, Mj, Hutchings, S., Manca, T., Ramelli, A., Nicolini, F., Gherli, T., Vezzani, A., Young, A., Carmona, Af, Santiago, Ai, Guillamon, Ln, Delgado, Mj, Delgado-Amaya, M., Curiel-Balsera, E., Rivera-Romero, L., Carrero-Gómez, F., Aguayo-Dehoyos, E., Ariam, Registry Of Adult Cardiac Surgery, Healey, Aj, Cameron, C., Jiao, Lr, Pérez, A., Martin, S., Del Moral, Ol, Toval, S., Rico, J., Aldecoa, C., Oguzhan, K., Demirkiran, O., Kirman, M., Bozbay, S., Kosuk, Me, Asyralyyeva, G., Dilek, M., Duzgun, M., Telli, S., Aydin, M., Yilmazer, F., Hodgson, Le, Dimitrov, Bd, Stubbs, C., Venn, R., Vedage, D., Shawaf, S., Naran, P., Sirisena, N., Kinnear, J., Londoño, Jg, Cardenas, Cl, Ginés, As, Gubianas, Cm, Sánchez, Ec, Sirvent, Jm, Panafidina, V., Shlyk, I., Ilyina, V., Judickas, S., Kezyte, G., Urbanaviciute, I., Serpytis, M., Gaizauskas, E., Sipylaite, J., Sprung, Cl, Munteanu, G., Morales, Rc, Kasdan, H., Volker, T., Reiter, A., Cohen, Y., Himmel, Y., Meissonnier, J., Banderas-Bravo, Me, Gómez-Jiménez, C., García-Martínez, Mv, Martínez-Carmona, Jf, Fernández-Ortega, Jf, O Dwyer, Mj, Starczewska, M., Wilks, M., Rapid Diagnosis of Infections in the Critically Ill Team, Torsvik, M., Gustad, Lt, Bangstad, Il, Vinje, Lj, Damås, Jk, Solligård, E., Mehl, A., Tsunoda, M., Kang, M., Saito, M., Saito, N., Akizuki, N., Namiki, M., Takeda, M., Yuzawa, J., Yaguchi, A., Tokyo Womens Medical University, Tsirigotis, P., Chondropoulos, S., Theodorakopoulou, M., Stamouli, M., Gkirkas, K., Dimopoulou, Ik, Makiko, S., Akiduki, N., Preau, S., Ambler, M., Sigurta, A., Saeed, S., Jochmans, S., Chelly, J., Vong, Lv, Sy, O., Serbource-Goguel, J., Rolin, N., Weyer, Cm, Abdallah, Ri, Adrie, C., Vinsonneau, C., Monchi, M., Mayr, U., Huber, W., Karsten, E., Lahmer, T., Thies, P., Henschel, B., Fischer, G., Schmid, Rm, Naz, I., Yaman, G., Kou, Ps, Lozano, Ja, Sánchez, Pc, Francioni, Je, Ferrón, Fr, Simón, Jm, Riad, Z., Mezidi, M., Aublanc, M., Perinel, S., Lissonde, F., Louf-Durier, A., Yonis, H., Tapponnier, R., Louis, B., Guérin, C., Plug, Working Group, Marmanidou, K., Oikonomou, M., Loizou, C., Somhorst, P., Hayashi, K., Hirayama, T., Yumoto, T., Tsukahara, K., Iida, A., Nosaka, N., Sato, K., Ugawa, T., Nakao, A., Ujike, Y., Hirohata, S., Mojoli, F., Torriglia, F., Giannantonio, M., Orlando, A., Bianzina, S., Mongodi, S., Pozzi, M., Iotti, Ga, Braschi, A., Jansen, D., Gadgil, S., Doorduin, J., Roesthuis, L., Heunks, Lm, Chen, Gq, Sun, Xm, He, X., Yang, Yl, Shi, Zh, Xu, M., Zhou, Jx, Pereira, Sm, Tucci, MR, Tonelotto, Bf, Simoes, Cm, Morais, Cc, Pompeo, Ms, Kay, Fu, Amato, Mb, Vieira, Je, Suzuki, S., Mihara, Y., Hikasa, Y., Okahara, S., Morimatsu, H., Okayama Research Investigation Organizing Network (ORION)investigators, Kwon, Hm, Moon, Yj, Lee, Sh, Jung, Kw, Shin, Wj, Jun, Ig, Song, Jg, Hwang, Gs, Lee, S., Jung, K., Brianti, R., Fanzaghi, P., Tudor, Ba, Klaus, Da, Lebherz-Eichinger, D., Lechner, C., Schwarz, C., Bodingbauer, M., Seemann, R., Kaczirek, K., Fleischmann, E., Roth, Ga, Krenn, Cg, Malyshev, A., Sergey, S., Yoshitake, E., Kaneko, M., Tencé, N., Zaien, I., Wolf, M., Trouiller, P., Jacobs, Fm, Kelly, Jm, Veigas, P., Hollands, S., Min, A., Rizoli, S., Robles, Cm, Oca Sandoval, Ma, Tarabrin, O., Gavrychenko, D., Mazurenko, G., Tarabrin, P., Mendez, Mc, Orden, Va, Noval, Rl, Mccue, C., Gemmell, L., Luján, J., Villa, P., Llorente, B., Molina, R., Alcázar, L., Juanas, Ca, Rogero, S., Pascual, T., Cambronero, Ja, Almudévar, Pm, Domínguez, Jp, Castañeda, Dp, Lucendo, Ap, Rivas, Rf, Villamizar, Pr, Javadpour, S., Kalani, N., Amininejad, T., Jamali, S., Sobhanian, S., Laurent, A., Bonnet, M., Rigal, R., Aslanian, P., Hebert, P., Capellier, G., Ps-Icu, Group, Contreras, MR, Mejías, Cr, Ruiz, Fc, Lombardo, Md, Perez, Jc, Hoyos, Ea, Estella, A., Viciana, R., Fontaiña, Lp, Rico, T., Madueño, Vp, Recuerda, M., Fernández, L., Bonet, S., Mazo, C., Rubiera, M., Ruiz-Rodríguez, Jc, Gracia, Rm, Espinel, E., Pont, T., Kotsopoulos, A., Jansen, N., Abdo, Wf, Gopcevic, A., Gavranovic, Z., Vucic, M., Glogoski, Mz, Penavic, Lv, Horvat, A., Martin-Villen, L., Egea-Guerero, Jj, Revuelto-Rey, J., Aldabo-Pallas, T., Correa-Chamorro, E., Gallego-Corpa, Ai, Granados, Pr, Faivre, V., Wildenberg, L., Huot, B., Lukaszewicz, Ac, Simsir, M., Mengelle, C., Payen, D., La Fuente, Mv, Almudena, Pm, Muñoz, Jj, Abellan, An, Lucendo, Ma, Perez, Lp, Dominguez, Jp, Wee, S., Ong, C., Lau, Yh, Wong, Y., Olea-Jiménez, V., Mora-Ordóñez, Jm, Muñoz-Muñoz, Jl, Vallejo-Báez, J., Daga-Ruiz, D., Lebrón-Gallardo, M., Rialp, G., Raurich, Jm, Morán, I., Martín, Mc, Heras, G., Mas, A., Vallverdú, I., Hraiech, S., Bourenne, J., Guervilly, C., Forel, Jm, Adda, M., Sylla, P., Mouaci, A., Gainnier, M., Papazian, L., Bauer, Pr, Kumbamu, A., Wilson, Me, Pannu, Jk, Egginton, Js, Kashyap, R., Gajic, O., Yoshihiro, S., Sakuraya, M., Hirata, A., Kawamura, N., Tsutui, T., Yoshida, K., Hashimoto, Y., Japan Septic Disseminated Intravascular Coagulation (JSEPTIC DIC) study group, Chang, Ch, Hu, Hc, Chiu, Lc, Hung, Cy, Li, Sh, Kao, Kc, Sibley, S., Drover, J., D Arsigny, C., Parker, C., Howes, D., Moffatt, S., Erb, J., Ilan, R., Messenger, D., Ball, I., Harrison, M., Ridi, S., Andrade, Ah, Costa, Rc, Souza, Va, Gonzalez, V., Amorim, V., Rolla, F., Filho, Ca, Miranda, R., Atchasiri, S., Buranavanich, P., Wathanawatthu, T., Suwanpasu, S., Bureau, C., Rolland-Debord, C., Poitou, T., Clavel, M., Perbet, S., Kouatchet, A., Similowski, T., Demoule, A., Diaz, P., Nunes, J., Escórcio, S., Silva, G., Chaves, S., Jardim, M., Câmara, M., Fernandes, N., Duarte, R., Jardim, Jj, Pereira, Ca, Nóbrega, Jj, Chen, Cm, Lai, Cc, Cheng, Kc, Chou, W., Lee, Sj, Cha, Ys, Lee, Wy, Onodera, M., Nakataki, E., Oto, J., Imanaka, H., Nishimura, M., Khadjibaev, A., Sabirov, D., Rosstalnaya, A., Akalaev, R., Parpibaev, F., Antonucci, E., Rossini, P., Gandolfi, S., Montini, E., Orlando, S., Nes, M., Karachi, F., Hanekom, S., Pereira, Uv, Parkin, Ms, Moore, M., Carvalho, Kv, Min, Hj, Kim, Hj, Choi, Yy, Lee, Ey, Song, I., Kim, Dj, E, Yy, Kim, Jw, Park, Js, Lee, Jh, Suh, Jw, Jo, Yh, Ferrero-Calleja, J., Merino-Vega, D., González-Jiménez, Ai, Sigcha, Ms, Hernández-Tejedor, A., Martin-Vivas, A., Gabán-Díez, Á, Luna, Rr, La Calle-Pedrosa, N., Temprano-Gómez, I., Afonso-Rivero, D., Pellin-Ariño, Ji, Algora-Weber, A., Fumis, Rr, Ferraz, Ab, Junior, Jm, Kirca, H., Cakin, O., Unal, M., Mutlu, H., Ramazanoglu, A., Cengiz, M., Nicolini, Ea, Pelisson, Fg, Nunes, Rs, Da Silva, Sl, Carreira, Mm, Bellissimo-Rodrigues, F., Ferez, Ma, Basile-Filho, A., Chao, Hc, Chen, L., Hravnak, M., Clermont, G., Pinsky, M., Dubrawski, A., Varas, Jl, Montero, Rm, Sánchez-Elvira, La, Díaz, Pv, Delgado, Cp, Ruiz, Bl, Guerrero, Ap, Galache, Ja, Sherif, H., Hassanin, H., El Hossainy, R., Samy, W., Ly, H., David, H., Burtin, P., Charpentier, C., Barral, M., Courant, P., Fournel, E., Gaide-Chevronnay, L., Durand, M., Albaladejo, P., Payen, Jf, Chavanon, O., Ortiz, Ab, Pozzebon, S., Fumagalli, F., Scala, S., Affatato, R., Maglie, M., Zani, D., Novelli, D., Marra, C., Luciani, A., Luini, M., Letizia, T., Pravettoni, D., Staszewsky, L., Belloli, A., Di Giancamillo, M., Scanziani, E., Kye, Yc, Yu, Km, Babini, G., Grassi, L., Reinikainen, M., Skrifvars, M., Kappler, F., Blobner, M., Schaller, Sj, Roasio, A., Costanzo, E., Cardellino, S., Fontana, V., Park, M., You, Km, Ko, Sb, Beane, A., Thilakasiri, Mc, Silva, Ap, Stephens, T., Sigera, Cs, Athapattu, P., Jayasinghe, S., Padeniya, A., Haniffa, R., Sáez, Vc, Ruiz-Ruano, Rdel, González, As, Kunze-Szikszay, N., Wand, S., Klapsing, P., Wetz, A., Heyne, T., Schwerdtfeger, K., Troeltzsch, M., Bauer, M., Quintel, M., Moerer, O., Cook, Dj, Rutherford, Wb, Scales, Dc, Adhikari, Nk, Cuthbertson, Bh, Suzuki, T., Fushimi, K., Iwamoto, M., Nakagawa, S., Mendsaikhan, N., Begzjav, T., Lundeg, G., Dünser, Mw, Romero, Dg, Padilla, Ys, Kleinpell, R., Chouris, I., Radu, V., Stougianni, M., Lavrentieva, A., Lagonidis, D., Price, Rd, Day, A., Arora, N., Henderson, Ma, Hickey, S., Costa, Mi, Carvalho, Jp, Gomes, Aa, Mergulhão, Pj, Chan, Kk, Maghsoudi, B., Tabei, Sh, Sabetian, G., Tabatabaei, Hr, Akbarzadeh, A., Student Research Committee - Shiraz University of Medical Sciences, Saigal, S., Pakhare, A., Joshi, R., Pattnaik, Sk, Ray, B., Rousseau, Af, Michel, L., Bawin, M., Cavalier, E., Reginster, Jy, Damas, P., Bruyere, O., Zhou, Jc, Cauwenberghs, H., Backer, A., Neels, H., Deblier, I., Berghmans, J., Himpe, D., Barea-Mendoza, Ja, Portillo, Ip, Fernández, Mv, Gigorro, Rg, Vela, Jl, Mateos, Hm, Alves, Sc, Varas, Gm, Rodriguez-Biendicho, A., Carreño, Er, González, Jc, Yang, Js, Lin, Kl, Choi, Yj, Yoon, Sz, Gordillo-Brenes, A., Fernandez-Zamora, Md, Herruzo-Aviles, A., Garcia-Delgado, M., Hinojosa-Perez, R., ARIAM-ANDALUCIA, Pascual, Oa, Pérez, Ag, Fernández, Pa, Amor, Ll, Albaiceta, Gm, Calvo, Sa, Spazzadeschi, A., Marrazzo, F., Gandola, A., Sciurti, R., Savi, C., Tseng, Cj, Bertini, P., Sanctis, F., Guarracino, F., Baldassarri, R., Buitinck, Sh, Voort, Ph, Tsunano, Y., Izawa, M., Tane, N., Ghosh, S., Gupta, A., Gasperi, A., Mazza, E., Limuti, R., Prosperi, M., Bissenova, N., Yergaliyeva, A., Talan, L., Yılmaz, G., Güven, G., Yoruk, F., Altıntas, Nd, Mukherjee, Dn, Agarwal, Lk, Mandal, K., Balsera, B., Martinez, M., Garcia, M., Castellana, D., Lopez, R., Barcenilla, F., Kaminsky, Ge, Carreño, R., Escribá, A., Fuentes, M., Gálvez, V., Del Olmo, R., Nieto, B., Vaquerizo, C., Alvarez, J., La Torre, Ma, Torres, E., Bogossian, E., Nouer, Sa, Salgado, Dr, Jiménez, Gj, Gaite, Fb, Martínez, Mp, Doganci, M., Izdes, S., Besevli, Sg, Alkan, A., Kayaaslan, B., Penichet, Sm, López, Ma, Repessé, X., Artiguenave, M., Paktoris-Papine, S., Espinasse, F., Dinh, A., El Sayed, F., Charron, C., Géri, G., Vieillard-Baron, A., Dimitroulakis, K., Ferré, A., Guillot, M., Teboul, Jl, Lichtenstein, D., Mézière, G., Richard, C., Monnet, X., Prīdāne, S., Sabeļņikovs, O., Bianchi, I., Kondili, E., Psarologakis, C., Kokkini, S., Amargianitakis, V., Babalis, D., Chytas, A., Chouvarda, I., Vaporidi, K., Georgopoulos, D., Trapp, O., Kalenka, A., Karbing, Ds, Gioia, A., Moro, F., Corte, Fd, Mauri, T., Rees, Se, Plug working group, Petrova, Mv, Mohan, R., Butrov, Av, Beeharry, Sd, Vatsik, Mv, Sakieva, Fi, Gobert, F., Fernandez, R., Labaune, Ma, Burle, Jf, Barbier, J., Vincent, B., Cleyet, M., Shinotsuka, Cr, Törnblom, S., Nisula, S., Vaara, S., Poukkanen, M., Andersson, S., Pesonen, E., Xie, Z., Liao, X., Kang, Y., Zhang, J., Kubota, K., Egi, M., Mizobuchi, S., Hegazy, S., El-Keraie, A., El Sayed, E., El Hamid, Ma, Rodrigues, Nj, Pereira, M., Godinho, I., Gameiro, J., Neves, M., Gouveia, J., E Silva, Zc, Lopes, Ja, Mckinlay, J., Kostalas, M., Kooner, G., Dudas, G., Horton, A., Kerr, C., Karanjia, N., Creagh-Brown, B., Yamazaki, A., Ganuza, Ms, Molina, Ja, Martinez, Fh, Freile, Mt, Fernandez, Ng, Travieso, Pm, Bandert, A., Frithiof, R., Lipcsey, M., Smekal, D., Schlaepfer, P., Durovray, Jd, Plouhinec, V., Chiappa, C., Bellomo, R., Schneider, Ag, Mitchell, S., Durrant, J., Street, H., Dunthorne, E., Shears, J., Caballero, Ch, Hutchison, R., Schwarze, S., Ghabina, S., Thompson, E., Prowle, Jr, Kirwan, Cj, Gonzalez, Ca, Pinto, Jl, Orozco, V., Patiño, Ja, Garcia, Pk, Contreras, Km, Rodriguez, P., and Echeverri, Je
40. Status of CANGAROO-III
- Author
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Mori, M., Bicknell, G., Clay, R., Edwards, P., Enomoto, R., Gunji, S., Hara, S., Hara, T., Hattori, T., Hayashi, S., Yusuke Higashi, Hirai, Y., Inoue, K., Itoh, C., Kabuki, S., Kajino, F., Katagiri, H., Kawachi, A., Kifune, T., Kiuchi, R., Kubo, H., Kushida, J., Matsubara, Y., Mizukami, T., Mizumoto, Y., Mizuniwa, R., Muraishi, H., Muraki, Y., Naito, T., Nakamori, T., Nakano, S., Nishida, D., Nishijima, K., Ohishi, M., Sakamoto, Y., Seki, A., Stamatescu, V., Suzuki, T., Swaby, D., Tanimori, T., Thornton, G., Tokanai, F., Tsuchiya, K., Watanabe, S., Yamada, Y., Yamazaki, E., Yanagita, S., Yoshida, T., Yoshikoshi, T., and Yukawa, Y.
41. Searching for very-high-energy electromagnetic counterparts to gravitational-wave events with the Cherenkov Telescope Array
- Author
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Patricelli, B., Carosi, A., Nava, L., Seglar-Arroyo, M., Schüssler, F., Stamerra, A., Adelfio, A., Ashkar, H., Bulgarelli, A., Di Girolamo, T., Di Piano, A., Gasparetto, T., Green, J., Longo, F., Agudo, I., Berti, A., Bissaldi, E., Cella, G., Circiello, A., Covino, S., Ghirlanda, G., Humensky, B., Inoue, S., Lefaucheur, J., Filipovic, M., Razzano, M., Ribeiro, D., Sergijenko, O., Stratta, G., Vergani, S., Abdalla, H., Abe, H., Abe, S., Abusleme, A., Acero, F., Acharyya, A., Acín Portella, V., Ackley, K., Adam, R., Adams, C., Adhikari, S. S., Aguado-Ruesga, I., Aguilera, R., Aguirre-Santaella, A., Aharonian, F., Alberdi, A., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Alves Batista, R., Amans, J. -P, Amati, L., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Ammendola, R., Anderson, J., Anduze, M., Angüner, E. O., Antonelli, L. A., Antonuccio, V., Antoranz, P., Anutarawiramkul, R., Aragunde Gutierrez, J., Aramo, C., Araudo, A., Araya, M., Arbet-Engels, A., Arcaro, C., Arendt, V., Armand, C., Armstrong, T., Arqueros, F., Arrabito, L., Arsioli, B., Artero, M., Asano, K., Ascasíbar, Y., Aschersleben, J., Ashley, M., Attinà, P., Aubert, P., Singh, C. B., Baack, D., Babic, A., Backes, M., Baena, V., Bajtlik, S., Baktash, A., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Balmaverde, B., Bamba, A., Bandiera, R., Baquero Larriva, A., Barai, P., Barbier, C., Barbosa Martins, V., Barcelo, M., Barkov, M., Barnard, M., Baroncelli, L., Almeida, U. B., Barrio, J. A., Bastieri, D., Batista, P. I., Batkovic, I., Bauer, C., Bautista-González, R., Baxter, J., Becciani, U., Becerra González, J., Becherini, Y., Beck, G., Becker Tjus, J., Bednarek, W., Belfiore, A., Bellizzi, L., Belmont, R., Benbow, W., Berge, D., Bernardini, E., Bernardos, M. I., Bernlöhr, K., Berton, M., Bertucci, B., Beshley, V., Bhatt, N., Bhattacharyya, S., Bhattacharyya, W., Bi, B., Bicknell, G., Biederbeck, N., Bigongiari, C., Biland, A., Bird, R., Biteau, J., Bitossi, M., Blanch, O., Blank, M., Blazek, J., Bobin, J., Boccato, C., Bocchino, F., Boehm, C., Bohacova, M., Boisson, C., Boix, J., Bolle, J. -P, Bolmont, J., Bonanno, G., Bonavolontà, C., Bonneau Arbeletche, L., Bonnoli, G., Bordas, P., Borkowski, J., Bórquez, S., Bose, R., Bose, D., Bosnjak, Z., Bottacini, E., Böttcher, M., Botticella, M. T., Boutonnet, C., Bouyjou, F., Bozhilov, V., Bozzo, E., Brahimi, L., Braiding, C., Brau-Nogué, S., Breen, S., Bregeon, J., Breuhaus, M., Brill, A., Brisken, W., Brocato, E., Brown, A. M., Brügge, K., Brun, P., Brun, F., Brunetti, L., Brunetti, G., Bruno, P., Bruno, A., Bruzzese, A., Bucciantini, N., Buckley, J., Bühler, R., Bulik, T., Bünning, M., Bunse, M., Burton, M., Burtovoi, A., Buscemi, M., Buschjäger, S., Busetto, G., Buss, J., Byrum, K., Caccianiga, A., Cadoux, F., Calanducci, A., Calderón, C., Calvo Tovar, J., Cameron, R., Campaña, P., Canestrari, R., Cangemi, F., Cantlay, B., Capalbi, M., Capasso, M., Cappi, M., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Cárdenas, V., Cardiel, L., Cardillo, M., Carlile, C., Caroff, S., Carosi, R., Carquín, E., Carrère, M., Casandjian, J. -M, Casanova, S., Cascone, E., Cassol, F., Castro-Tirado, A. J., Catalani, F., Catalano, O., Cauz, D., Ceccanti, A., Celestino Silva, C., Celli, S., Cerny, K., Cerruti, M., Chabanne, E., Chadwick, P., Chai, Y., Chambery, P., Champion, C., Chandra, S., Chaty, S., Chen, A., Cheng, K., Chernyakova, M., Chiaro, G., Chiavassa, A., Chikawa, M., Chitnis, V. R., Chudoba, J., Chytka, L., Cikota, S., Clark, P., Çolak, M., Colombo, E., Colome, J., Colonges, S., Comastri, A., Compagnino, A., Conforti, V., Congiu, E., Coniglione, R., Conrad, J., Conte, F., Contreras, J. L., Coppi, P., Cornat, R., Coronado-Blazquez, J., Cortina, J., Costa, A., Costantini, H., Cotter, G., Courty, B., Crestan, S., Cristofari, P., Crocker, R., Croston, J., Cubuk, K., Cuevas, O., Cui, X., Cusumano, G., Cutini, S., D’aì, A., D’amico, G., D’ammando, F., D’avanzo, P., Da Vela, P., Dadina, M., Dai, S., Dalchenko, M., Dall’ Ora, M., Daniel, M. K., Dauguet, J., Davids, I., Davies, J., Dawson, B., Angelis, A., Araújo Carvalho, A. E., Bony Lavergne, M., Caprio, V., Cesare, G., Frondat, F., Gouveia Dal Pino, E. M., La Calle, I., Lotto, B., Luca, A., Martino, D., Menezes, R. M., Naurois, M., Oña Wilhelmi, E., Palma, F., Persio, F., Simone, N., Souza, V., Del Santo, M., Del Valle, M. V., Delagnes, E., Deleglise, G., Delfino Reznicek, M., Delgado, C., Delgado Giler, A. G., Delgado Mengual, J., Della Ceca, R., Della Valle, M., Della Volpe, D., Depaoli, D., Depouez, D., Devin, J., Di Giulio, C., Di Pierro, F., Di Venere, L., Díaz, C., Díaz-Bahamondes, C., Dib, C., Diebold, S., Digel, S., Dima, R., Djannati-Ataï, A., Djuvsland, J., Dmytriiev, A., Docher, K., Domínguez, A., Dominis Prester, D., Donath, A., Donini, A., Dorner, D., Doro, M., Dos Anjos, R. D. C., Dournaux, J. -L, Downes, T., Drake, G., Drass, H., Dravins, D., Duangchan, C., Duara, A., Dubus, G., Ducci, L., Duffy, C., Dumora, D., Dundas Morå, K., Durkalec, A., Dwarkadas, V. V., Ebr, J., Eckner, C., Eder, J., Ederoclite, A., Edy, E., Egberts, K., Einecke, S., Eisch, J., Eleftheriadis, C., Elsässer, D., Emery, G., Emmanoulopoulos, D., Ernenwein, J. -P, Errando, M., Escarate, P., Escudero, J., Espinoza, C., Ettori, S., Eungwanichayapant, A., Evans, P., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Fallah Ramazani, V., Falomo, R., Farakos, K., Fasola, G., Fattorini, A., Favre, Y., Fedora, R., Fedorova, E., Fegan, S., Feijen, K., Feng, Q., Ferrand, G., Ferrara, G., Ferreira, O., Fesquet, M., Fiandrini, E., Fiasson, A., Fink, D., Finley, J. P., Fioretti, V., Fiorillo, D. F. G., Fiorini, M., Flis, S., Flores, H., Foffano, L., Föhr, C., Fonseca, M. V., Font, L., Fontaine, G., Fornieri, O., Fortin, P., Fortson, L., Fouque, N., Fournier, A., Fraga, B., Franceschini, A., Franco, F. J., Franco Ordovas, A., Freixas Coromina, L., Fresnillo, L., Fruck, C., Fugazza, D., Fujikawa, Y., Fujita, Y., Fukami, S., Fukazawa, Y., Fukui, Y., Fulla, D., Funk, S., Furniss, A., Gabella, O., Gabici, S., Gaggero, D., Galanti, G., Galaz, G., Galdemard, P., Gallant, Y., Galloway, D., Gallozzi, S., Gammaldi, V., Garcia, R., Garcia, E., García, E., Garcia López, R., Garczarczyk, M., Gargano, F., Gargano, C., Garozzo, S., Gascon, D., Gasparrini, D., Gasparyan, H., Gaug, M., Geffroy, N., Gent, A., Germani, S., Gesa, L., Ghalumyan, A., Ghedina, A., Gianotti, F., Giarrusso, S., Giarrusso, M., Giavitto, G., Giebels, B., Giglietto, N., Gika, V., Gillardo, F., Gimenes, R., Giordano, F., Giovannini, G., Giro, E., Giroletti, M., Giuliani, A., Giunti, L., Gjaja, M., Glicenstein, J. -F, Gliwny, P., Godinovic, N., Göksu, H., Goldoni, P., Gómez, J. L., Gómez-Vargas, G., González, M. M., González, J. M., Gothe, K. S., Götz, D., Goulart Coelho, J., Gourgouliatos, K., Grabarczyk, T., Graciani, R., Grandi, P., Grasseau, G., Grasso, D., Green, A. J., Green, D., Greenshaw, T., Grenier, I., Grespan, P., Grillo, A., Grondin, M. -H, Grube, J., Guarino, V., Guest, B., Gueta, O., Gündüz, M., Gunji, S., Gusdorf, A., Gyuk, G., Hackfeld, J., Hadasch, D., Haga, J., Hagge, L., Hahn, A., Hajlaoui, J. E., Hakobyan, H., Halim, A., Hamal, P., Hanlon, W., Hara, S., Harada, Y., Hardcastle, M. J., Harvey, M., Hashiyama, K., Hassan Collado, T., Haubold, T., Haupt, A., Hautmann, U. A., Havelka, M., Hayashi, K., Hayashida, M., He, H., Heckmann, L., Heller, M., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Hernández Cadena, S., Herrera Llorente, J., Herrero, A., Hervet, O., Hinton, J., Hiramatsu, A., Hiroshima, N., Hirotani, K., Hnatyk, B., Hnatyk, R., Hoang, J. K., Hoffmann, D., Hofmann, W., Hoischen, C., Holder, J., Holler, M., Hona, B., Horan, D., Hörandel, J., Horns, D., Horvath, P., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huang, Y., Huet, J. -M, Hughes, G., Hui, D., Hull, G., Humensky, T. B., Hütten, M., Iaria, R., Iarlori, M., Illa, J. M., Imazawa, R., Impiombato, D., Inada, T., Incardona, F., Ingallinera, A., Inome, Y., Inoue, T., Inoue, Y., Insolia, A., Iocco, F., Ioka, K., Ionica, M., Iori, M., Iovenitti, S., Iriarte, A., Ishio, K., Ishizaki, W., Iwamura, Y., Jablonski, C., Jacquemier, J., Jacquemont, M., Jamrozy, M., Janecek, P., Jankowsky, F., Jardin-Blicq, A., Jarnot, C., Jean, P., Jiménez Martínez, I., Jin, W., Jocou, L., Jordana, N., Josselin, M., Jouvin, L., Jung-Richardt, I., Junqueira, F. J. P. A., Juramy-Gilles, C., Jurysek, J., Kaaret, P., Kadowaki, L. H. S., Kagaya, M., Kalekin, O., Kankanyan, R., Kantzas, D., Karas, V., Karastergiou, A., Karkar, S., Kasai, E., Kasperek, J., Katagiri, H., Kataoka, J., Katarzyński, K., Katsuda, S., Katz, U., Kawanaka, N., Kazanas, D., Kerszberg, D., Khélifi, B., Kherlakian, M. C., Kian, T. P., Kieda, D. B., Kihm, T., Kim, S., Kimeswenger, S., Kisaka, S., Kissmann, R., Kleijwegt, R., Kleiner, T., Kluge, G., Kluźniak, W., Knapp, J., Knödlseder, J., Kobakhidze, A., Kobayashi, Y., Koch, B., Kocot, J., Kohri, K., Kokkotas, K., Komin, N., Kong, A., Kosack, K., Kowal, G., Krack, F., Krause, M., Krennrich, F., Krumholz, M., Kubo, H., Kudryavtsev, V., Kunwar, S., Kuroda, Y., Kushida, J., Kushwaha, P., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lahmann, R., Lamanna, G., Lamastra, A., Landoni, M., Landriu, D., Lang, R. G., Lapington, J., Laporte, P., Lason, P., Lasuik, J., Lazendic-Galloway, J., Le Flour, T., Le Sidaner, P., Leach, S., Leckngam, A., Lee, S. -H, Lee, W. H., Lee, S., Oliveira, M. A. L., Lemière, A., Lemoine-Goumard, M., Lenain, J. -P, Leone, F., Leray, V., Leto, G., Leuschner, F., Levy, C., Lindemann, R., Lindfors, E., Linhoff, L., Liodakis, I., Lipniacka, A., Lloyd, S., Lobo, M., Lohse, T., Lombardi, S., Lopez, A., López, M., López-Coto, R., Loporchio, S., Louis, F., Louys, M., Lucarelli, F., Lucchesi, D., Ludwig Boudi, H., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maccarone, T., Mach, E., Maciejewski, A. J., Mackey, J., Madejski, G. M., Maeght, P., Maggio, C., Maier, G., Majczyna, A., Majumdar, P., Makariev, M., Mallamaci, M., Almeida, R. M. N., Maltezos, S., Malyshev, D., Mandat, D., Maneva, G., Manganaro, M., Manicò, G., Manigot, P., Mannheim, K., Maragos, N., Marano, D., Marconi, M., Marcowith, A., Marculewicz, M., Marčun, B., Marín, J., Marinello, N., Marinos, P., Mariotti, M., Markoff, S., Marquez, P., Marsella, G., Martí, J., Martin, J. -M, Martin, P., Martinez, O., Martínez, M., Martínez, G., Martínez, O., Martínez-Huerta, H., Marty, C., Marx, R., Masetti, N., Massimino, P., Mastichiadis, A., Matsumoto, H., Matthews, N., Maurin, G., Max-Moerbeck, W., Maxted, N., Mazin, D., Mazziotta, M. N., Mazzola, S. M., Mbarubucyeye, J. D., Mc Comb, L., Mchardy, I., Mckeague, S., Mcmuldroch, S., Medina, E., Medina Miranda, D., Melandri, A., Melioli, C., Melkumyan, D., Menchiari, S., Mender, S., Mereghetti, S., Merino Arévalo, G., Mestre, E., Meunier, J. -L, Meures, T., Meyer, M., Micanovic, S., Miceli, M., Michailidis, M., Michałowski, J., Miener, T., Mievre, I., Miller, J., Minaya, I. A., Mineo, T., Minev, M., Miranda, J. M., Mirzoyan, R., Mitchell, A., Mizuno, T., Mode, B., Moderski, R., Mohrmann, L., Molina, E., Molinari, E., Montaruli, T., Monteiro, I., Moore, C., Moralejo, A., Morcuende-Parrilla, D., Moretti, E., Morganti, L., Mori, K., Moriarty, P., Morik, K., Morlino, G., Morris, P., Morselli, A., Mosshammer, K., Moya, P., Mukherjee, R., Muller, J., Mundell, C., Mundet, J., Murach, T., Muraczewski, A., Muraishi, H., Murase, K., Musella, I., Musumarra, A., Nagai, A., Nagar, N., Nagataki, S., Naito, T., Nakamori, T., Nakashima, K., Nakayama, K., Nakhjiri, N., Naletto, G., Naumann, D., Navarro, R., Nawaz, M. A., Ndiyavala, H., Neise, D., Nellen, L., Nemmen, R., Newbold, M., Neyroud, N., Ngernphat, K., Nguyen Trung, T., Nicastro, L., Nickel, L., Niemiec, J., Nieto, D., Nievas, M., Nigro, C., Nikołajuk, M., Ninci, D., Nishijima, K., Noda, K., Nogami, Y., Nolan, S., Nomura, R., Norris, R., Nosek, D., Nöthe, M., Novosyadlyj, B., Novotny, V., Nozaki, S., Nunio, F., O’brien, P., Obara, K., Oger, R., Ohira, Y., Ohishi, M., Ohm, S., Ohtani, Y., Oka, T., Okazaki, N., Okumura, A., Olive, J. -F, Oliver, C., Olivera, G., Olmi, B., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, S., Orlando, E., Osborne, J. P., Ostrowski, M., Otte, N., Evgeni Ovcharov, Owen, E., Oya, I., Ozieblo, A., Padovani, M., Pagano, I., Pagliaro, A., Paizis, A., Palatiello, M., Palatka, M., Palazzi, E., Panazol, J. -L, Paneque, D., Panes, B., Panny, S., Pantaleo, F. R., Panter, M., Paoletti, R., Paolillo, M., Papitto, A., Paravac, A., Paredes, J. M., Pareschi, G., Park, N., Parmiggiani, N., Parsons, R. D., Paśko, P., Patel, S., Pauletta, G., Pavletić, L., Pavy, S., Pe’er, A., Pech, M., Pecimotika, M., Pellegriti, M. G., Del Campo, P. P., Penno, M., Pepato, A., Perard, S., Perennes, C., Peres, G., Peresano, M., Pérez-Aguilera, A., Pérez-Romero, J., Pérez-Torres, M. A., Perri, M., Persic, M., Petrera, S., Petrucci, P. -O, Petruk, O., Peyaud, B., Pfrang, K., Pian, E., Piano, G., Piatteli, P., Pietropaolo, E., Pillera, R., Pilszyk, B., Pimentel, D., Pintore, F., Pio García, C., Pirola, G., Piron, F., Pisarski, A., Pita, S., Pohl, M., Poireau, V., Poledrelli, P., Pollo, A., Polo, M., Pongkitivanichkul, C., Porthault, J., Powell, J., Pozo, D., Prado, R. R., Prandini, E., Prasit, P., Prast, J., Pressard, K., Principe, G., Priyadarshi, C., Produit, N., Prokhorov, D., Prokoph, H., Prouza, M., Przybilski, H., Pueschel, E., Pühlhofer, G., Puljak, I., Pumo, M. L., Punch, M., Queiroz, F., Quinn, J., Quirrenbach, A., Rainò, S., Rajda, P. J., Rando, R., Razzaque, S., Rebert, E., Recchia, S., Reichherzer, P., Reimer, O., Reimer, A., Reisenegger, A., Remy, Q., Renaud, M., Reposeur, T., Reville, B., Reymond, J. -M, Reynolds, J., Rhode, W., Ribó, M., Richards, G., Richtler, T., Rico, J., Rieger, F., Riitano, L., Ripepi, V., Riquelme, M., Riquelme, D., Rivoire, S., Rizi, V., Roache, E., Röben, B., Roche, M., Rodriguez, J., Fernandez, G. R., Ramirez, J. C. R., Vázquez, J. J. R., Roepke, F., Rojas, G., Romanato, L., Romano, P., Romeo, G., Romero Lobato, F., Romoli, C., Roncadelli, M., Ronda, S., Rosado, J., Leon, A. R., Rowell, G., Rudak, B., Rugliancich, A., Del Mazo, J. E. R., Rujopakarn, W., Rulten, C., Russell, C., Russo, F., Sadeh, I., Sæther Hatlen, E., Safi-Harb, S., Saha, L., Saha, P., Sahakian, V., Sailer, S., Saito, T., Sakaki, N., Sakurai, S., Salesa Greus, F., Salina, G., Salzmann, H., Sanchez, D., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Santangelo, A., Santos, E. M., Santos-Lima, R., Sanuy, A., Sapozhnikov, L., Saric, T., Sarkar, S., Sasaki, H., Sasaki, N., Satalecka, K., Sato, Y., Saturni, F. G., Sawada, M., Sawangwit, U., Schaefer, J., Scherer, A., Scherpenberg, J., Schipani, P., Schleicher, B., Schmoll, J., Schneider, M., Schoorlemmer, H., Schovanek, P., Schussler, F., Schwab, B., Schwanke, U., Schwarz, J., Schweizer, T., Sciacca, E., Scuderi, S., Seglar Arroyo, M., Segreto, A., Seitenzahl, I., Semikoz, D., Serna Franco, J. E., Servillat, M., Seweryn, K., Sguera, V., Shalchi, A., Shang, R. Y., Sharma, P., Shellard, R. C., Sidoli, L., Sieiro, J., Siejkowski, H., Silk, J., Sillanpää, A., Singh, B. B., Singh, K. K., Sinha, A., Siqueira, C., Sironi, G., Sitarek, J., Sizun, P., Sliusar, V., Slowikowska, A., Sobczyńska, D., Sobrinho, R. W., Sol, H., Sottile, G., Spackman, H., Specovius, A., Spencer, S., Spengler, G., Spiga, D., Spolon, A., Springer, W., Stanič, S., Starling, R., Stawarz, Ł., Steenkamp, R., Stefanik, S., Stegmann, C., Steiner, A., Steinmassl, S., Stella, C., Steppa, C., Sternberger, R., Sterzel, M., Stevens, C., Stevenson, B., Stolarczyk, T., Straumann, U., Strišković, J., Strzys, M., Stuik, R., Suchenek, M., Suda, Y., Sunada, Y., Suomijarvi, T., Suric, T., Sutcliffe, P., Suzuki, H., Świerk, P., Szepieniec, T., Tacchini, A., Tachihara, K., Tagliaferri, G., Tajima, H., Tajima, N., Tak, D., Takahashi, K., Takahashi, H., Takahashi, M., Takata, J., Takeishi, R., Tam, T., Tanaka, M., Tanaka, T., Tanaka, S., Tateishi, D., Tavani, M., Tavecchio, F., Tavernier, T., Taylor, L., Taylor, A., Tejedor, L. A., Temnikov, P., Terada, Y., Terauchi, K., Terrazas, J. C., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thibaut, D., Thocquenne, F., Tian, W., Tibaldo, L., Tiengo, A., Tiziani, D., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Toma, K., Tomankova, L., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tosti, L., Totani, T., Tothill, N., Toussenel, F., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Trois, A., Truzzi, S., Tsiahina, A., Tsuru, T., Turk, B., Tutone, A., Uchiyama, Y., Umana, G., Utayarat, P., Vaclavek, L., Vacula, M., Vagelli, V., Vagnetti, F., Vakili, F., Valdivia, J. A., Valentino, M., Valio, A., Vallage, B., Vallania, P., Valverde Quispe, J. V., Den Berg, A. M., Driel, W., Eldik, C., Rensburg, C., Soelen, B., Vandenbroucke, J., Vanderwalt, J., Vasileiadis, G., Vassiliev, V., Vázquez Acosta, M., Vecchi, M., Vega, A., Veh, J., Veitch, P., Venault, P., Venter, C., Ventura, S., Vercellone, S., Verguilov, V., Verna, G., Vernetto, S., Verzi, V., Vettolani, G. P., Veyssiere, C., Viale, I., Viana, A., Viaux, N., Vicha, J., Vignatti, J., Vigorito, C. F., Villanueva, J., Vink, J., Vitale, V., Vittorini, V., Vodeb, V., Voelk, H., Vogel, N., Voisin, V., Vorobiov, S., Vovk, I., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Wagner, P., Wakazono, K., Wakely, S. P., Walter, R., Ward, M., Warren, D., Watson, J., Webb, N., Wechakama, M., Wegner, P., Weinstein, A., Weniger, C., Werner, F., Wetteskind, H., White, M., White, R., Wierzcholska, A., Wiesand, S., Wijers, R., Wilkinson, M., Will, M., Williams, D. A., Williams, J., Williamson, T., Wolter, A., Wong, Y. W., Wood, M., Wunderlich, C., Yamamoto, T., Yamamoto, H., Yamane, Y., Yamazaki, R., Yanagita, S., Yang, L., Yoo, S., Yoshida, T., Yoshikoshi, T., Yu, P., Yusafzai, A., Zacharias, M., Zaharijas, G., Zaldivar, B., Zampieri, L., Zanmar Sanchez, R., Zaric, D., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zenin, A., Zerwekh, A., Zhdanov, V. I., Ziętara, K., Zink, A., Ziółkowski, J., Zitelli, V., Živec, M., and Zmija, A.
42. Turn-by-turn measurements at the KEK-ATF
- Author
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Renier, Y., Yannis Papaphilippou, Tomas, R., Wendt, M., Eddy, N., Kubo, K., Kuroda, S., Naito, T., Okugi, T., Terunuma, N., and Urakawa, J.
43. Development of timing distribution system with femto-second stability
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Naito, T., Ebihara, K., Shunsuke Nozawa, Terunuma, N., Urakawa, J., Amemiya, M., Suzuyama, T., and Watabe, T.
44. Conversion Surgery for Locally Advanced Unresectable Pancreatic Cancer Treated with FOLFIRINOX Therapy and Proton Beam Therapy Combined with S-1 Chemotherapy-A Case Report
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Umino, Y., Mizuma, M., Iseki, M., Hata, T., Takadate, T., Kawaguchi, K., Aoki, T., Fuyuhiko Motoi, Naito, T., Kamei, T., Masamune, A., Ishioka, C., Ono, T., Murakami, M., and Unno, M.
45. The Compact Linear Collider (CLIC) - 2018 Summary Report
- Author
-
CLICdp collaborations, The CLIC, Charles, T. K., Giansiracusa, P. J., Lucas, T. G., Rassool, R. P., Volpi, M., Balazs, C., Afanaciev, K., Makarenko, V., Patapenka, A., Zhuk, I., Collette, C., Boland, M. J., Hoffman, A. C. Abusleme, Diaz, M. A., Garay, F., Chi, Y., He, X., Pei, G., Pei, S., Shu, G., Wang, X., Zhang, J., Zhao, F., Zhou, Z., Chen, H., Gao, Y., Huang, W., Kuang, Y. P., Li, B., Li, Y., Meng, X., Shao, J., Shi, J., Tang, C., Wang, P., Wu, X., Zha, H., Ma, L., Han, Y., Fang, W., Gu, Q., Huang, D., Huang, X., Tan, J., Wang, Z., Zhao, Z., Uggerhøj, U. I., Wistisen, T. N., Aabloo, A., Aare, R., Kuppart, K., Vigonski, S., Zadin, V., Aicheler, M., Baibuz, E., Brücken, E., Djurabekova, F., Eerola, P., Garcia, F., Haeggström, E., Huitu, K., Jansson, V., Kassamakov, I., Kimari, J., Kyritsakis, A., Lehti, S., Meriläinen, A., Montonen, R., Nordlund, K., Österberg, K., Saressalo, A., Väinölä, J., Veske, M., Farabolini, W., Mollard, A., Peauger, F., Plouin, J., Bambade, P., Chaikovska, I., Chehab, R., Delerue, N., Davier, M., Faus-Golfe, A., Irles, A., Kaabi, W., LeDiberder, F., Pöschl, R., Zerwas, D., Aimard, B., Balik, G., J. -J. Blaising, Brunetti, L., Chefdeville, M., Dominjon, A., Drancourt, C., Geoffroy, N., Jacquemier, J., Jeremie, A., Karyotakis, Y., Nappa, J. M., Serluca, M., Vilalte, S., Vouters, G., Bernhard, A., Bründermann, E., Casalbuoni, S., Hillenbrand, S., Gethmann, J., Grau, A., Huttel, E., Müller, A.-S., Peiffer, P., Perić, I., Jauregui, D. Saez de, Emberger, L., Graf, C., Simon, F., Szalay, M., Kolk, N. van der, Brass, S., Kilian, W., Alexopoulos, T., Apostolopoulos, T., Gazis, E. N., Gazis, N., Kostopoulos, V., Kourkoulis, S., Heilig, B., Lichtenberger, J., Shrivastava, P., Dayyani, M. K., Ghasem, H., Hajari, S. S., Shaker, H., Ashkenazy, Y., Popov, I., Engelberg, E., Yashar, A., Abramowicz, H., Benhammou, Y., Borysov, O., Borysova, M., Levy, A., Levy, I., Alesini, D., Bellaveglia, M., Buonomo, B., Cardelli, A., Diomede, M., Ferrario, M., Gallo, A., Ghigo, A., Giribono, A., Piersanti, L., Stella, A., Vaccarezza, C., Blas, J. de, Franceschini, R., D’Auria, G., Mitri, S. Di, Abe, T., Aryshev, A., Fukuda, M., Furukawa, K., Hayano, H., Higashi, Y., Higo, T., Kubo, K., Kuroda, S., Matsumoto, S., Michizono, S., Naito, T., Okugi, T., Shidara, T., Tauchi, T., Terunuma, N., Urakawa, J., Yamamoto, A., Raboanary, R., Luiten, O. J., Stragier, X. F. D., Hart, R., Graaf, H. van der, Eigen, G., Adli, E., Lindstrøm, C. A., Lillestøl, R., Malina, L., Pfingstner, J., Sjobak, K. N., Ahmad, A., Hoorani, H., Khan, W. A., Bugiel, S., Bugiel, R., Firlej, M., Fiutowski, T. A., Idzik, M., Moroń, J., Świentek, K. P., Renstrom, P. Brückman de, Krupa, B., Kucharczyk, M., Lesiak, T., Pawlik, B., Sopicki, P., Turbiarz, B., Wojtoń, T., Zawiejski, L. K., Kalinowski, J., Nowak, K., Żarnecki, A. F., Firu, E., Ghenescu, V., Neagu, A. T., Preda, T., Zgura, I. S., Aloev, A., Azaryan, N., Boyko, I., Budagov, J., Chizhov, M., Filippova, M., Glagolev, V., Gongadze, A., Grigoryan, S., Gudkov, D., Karjavine, V., Lyablin, M., Nefedov, Yu, Olyunin, A., Rymbekova, A., Samochkine, A., Sapronov, A., Shelkov, G., Shirkov, G., Soldatov, V., Solodko, E., Trubnikov, G., Tyapkin, I., Uzhinsky, V., Vorozhtov, A., Zhemchugov, A., Levichev, E., Mezentsev, N., Piminov, P., Shatilov, D., Vobly, P., Zolotarev, K., Jelisavčić, I. Božović, Kačarević, G., Dumbelović, G. Milutinović, Pandurović, M., Radulović, M., Stevanović, J., Vukasinović, N., D. -H. Lee, Ayala, N., Benedetti, G., Guenzel, T., Iriso, U., Marti, Z., Perez, F., Pont, M., Trenado, J., Ruiz-Jimeno, A., Vila, I., Calero, J., Dominguez, M., Garcia-Tabares, L., Gavela, D., Lopez, D., Toral, F., Gutierrez, C. Blanch, Boronat, M., Esperante, D., Fullana, E., Fuster, J., García, I., Gimeno, B., Lopez, P. Gomis, González, D., Perelló, M., Ros, E., Villarejo, M. A., Vnuchenko, A., Vos, M., Borgmann, Ch, Brenner, R., Ekelöf, T., Jacewicz, M., Olvegård, M., Ruber, R., Ziemann, V., Aguglia, D., Gonzalvo, J. Alabau, Leon, M. Alcaide, Tehrani, N. Alipour, Anastasopoulos, M., Andersson, A., Andrianala, F., Antoniou, F., Apyan, A., Arominski, D., Artoos, K., Assly, S., Atieh, S., Baccigalupi, C., Sune, R. Ballabriga, Caballero, D. Banon, Barnes, M. J., Garcia, J. Barranco, Bartalesi, A., Bauche, J., Bayar, C., Belver-Aguilar, C., Morell, A. Benot, Bernardini, M., Bett, D. R., Bettoni, S., Bettencourt, M., Bielawski, B., Garcia, O. Blanco, Kraljevic, N. Blaskovic, Bolzon, B., Bonnin, X. A., Bozzini, D., Branger, E., Brondolin, E., Brunner, O., Buckland, M., Bursali, H., Burkhardt, H., Caiazza, D., Calatroni, S., Campbell, M., Lasheras, N. Catalan, Cassany, B., Castro, E., Soares, R. H. Cavaleiro, Bastos, M. Cerqueira, Cherif, A., Chevallay, E., Cilento, V., Corsini, R., Costa, R., Cure, B., Curt, S., Gobbo, A. Dal, Dannheim, D., Daskalaki, E., Deacon, L., Degiovanni, A., Michele, G. De, Oliveira, L. De, Romano, V. Del Pozo, Delahaye, J. P., Delikaris, D., Almeida, P. G. Dias de, Dobers, T., Doebert, S., Doytchinov, I., Draper, M., Ramos, F. Duarte, Duquenne, M., Plaja, N. Egidos, Elsener, K., Esberg, J., Esposito, M., Evans, L., Fedosseev, V., Ferracin, P., Fiergolski, A., Foraz, K., Fowler, A., Friebel, F., Fuchs, J.-F., Gaddi, A., Gamba, D., Fajardo, L. Garcia, Morales, H. Garcia, Garion, C., Gasior, M., Gatignon, L., Gayde, J.-C., Gerbershagen, A., Gerwig, H., Giambelli, G., Gilardi, A., Goldblatt, A. N., Anton, S. Gonzalez, Grefe, C., Grudiev, A., Guerin, H., Guillot-Vignot, F. G., Gutt-Mostowy, M. L., Lutz, M. Hein, Hessler, C., Holma, J. K., Holzer, E. B., Hourican, M., Hynds, D., Ikarios, E., Levinsen, Y. Inntjore, Janssens, S., Jeff, A., Jensen, E., Jonker, M., Kamugasa, S. W., Kastriotou, M., Kemppinen, J. M. K., Khan, V., Kieffer, R. B., Klempt, W., Kokkinis, N., Kossyvakis, I., Kostka, Z., Korsback, A., Platia, E. Koukovini, Kovermann, J. W., Kozsar, C.-I., Kremastiotis, I., Kröger, J., Kulis, S., Latina, A., Leaux, F., Lebrun, P., Lefevre, T., Leogrande, E., Linssen, L., Liu, X., Cudie, X. Llopart, Magnoni, S., Maidana, C., Maier, A. A., Durand, H. Mainaud, Mallows, S., Manosperti, E., Marelli, C., Lacoma, E. Marin, Marsh, S., Martin, R., Martini, I., Martyanov, M., Mazzoni, S., Mcmonagle, G., Mether, L. M., Meynier, C., Modena, M., Moilanen, A., Mondello, R., Cabral, P. B. Moniz, Irazabal, N. Mouriz, Munker, M., Muranaka, T., Nadenau, J., Navarro, J. G., Quirante, J. L. Navarro, Busto, E. Nebo Del, Nikiforou, N., Ninin, P., Nonis, M., Nisbet, D., Nuiry, F. X., Nürnberg, A., Ögren, J., Osborne, J., Ouniche, A. C., Pan, R., Papadopoulou, S., Papaphilippou, Y., Paraskaki, G., Pastushenko, A., Passarelli, A., Patecki, M., Pazdera, L., Pellegrini, D., Pepitone, K., Codina, E. Perez, Fontenla, A. Perez, Persson, T. H. B., Petrič, M., Pitman, S., Pitters, F., Pittet, S., Plassard, F., Popescu, D., Quast, T., Rajamak, R., Redford, S., Remandet, L., Renier, Y., Rey, S. F., Orozco, O. Rey, Riddone, G., Castro, E. Rodriguez, Roloff, P., Rossi, C., Rossi, F., Rude, V., Ruehl, I., Rumolo, G., Sailer, A., Sandomierski, J., Santin, E., Sanz, C., Bedolla, J. Sauza, Schnoor, U., Schmickler, H., Schulte, D., Senes, E., Serpico, C., Severino, G., Shipman, N., Sicking, E., Simoniello, R., Skowronski, P. K., Mompean, P. Sobrino, Soby, L., Sollander, P., Solodko, A., Sosin, M. P., Spannagel, S., Sroka, S., Stapnes, S., Sterbini, G., Stern, G., Ström, R., Stuart, M. J., Syratchev, I., Szypula, K., Tecker, F., Thonet, P. A., Thrane, P., Timeo, L., Tiirakari, M., Garcia, R. Tomas, Tomoiaga, C. I., Valerio, P., Vaňát, T., Vamvakas, A. L., Hoorne, J. Van, Viazlo, O., Pinto, M. Vicente Barreto, Vitoratou, N., Vlachakis, V., Weber, M. A., Wegner, R., Wendt, M., Widorski, M., Williams, O. E., Williams, M., Woolley, B., Wuensch, W., Wulzer, A., Uythoven, J., Xydou, A., Yang, R., Zelios, A., Zhao, Y., Zisopoulos, P., Benoit, M., Sultan, D. M. S., Riva, F., Bopp, M., Braun, H. H., Craievich, P., Dehler, M., Garvey, T., Pedrozzi, M., Raguin, J. Y., Rivkin, L., Zennaro, R., Guillaume, S., Rothacher, M., Aksoy, A., Nergiz, Z., Yavas, Ö., Denizli, H., Keskin, U., Oyulmaz, K. Y., Senol, A., Ciftci, A. K., Baturin, V., Karpenko, O., Kholodov, R., Lebed, O., Lebedynskyi, S., Mordyk, S., Musienko, I., Profatilova, Ia, Storizhko, V., Bosley, R. R., Price, T., Watson, M. F., Watson, N. K., Winter, A. G., Goldstein, J., Green, S., Marshall, J. S., Thomson, M. A., Xu, B., You, T., Gillespie, W. A., Spannowsky, M., Beggan, C., Martin, V., Zhang, Y., Protopopescu, D., Robson, A., Apsimon, R. J., Bailey, I., Burt, G. C., Dexter, A. C., Edwards, A. V., Hill, V., Jamison, S., Millar, W. L., Papke, K., Casse, G., Vossebeld, J., Aumeyr, T., Bergamaschi, M., Bobb, L., Bosco, A., Boogert, S., Boorman, G., Cullinan, F., Gibson, S., Karataev, P., Kruchinin, K., Lekomtsev, K., Lyapin, A., Nevay, L., Shields, W., Snuverink, J., Towler, J., Yamakawa, E., Boisvert, V., West, S., Jones, R., Joshi, N., Bett, D., Bodenstein, R. M., Bromwich, T., Burrows, P. N., Christian, G. B., Gohil, C., Korysko, P., Paszkiewicz, J., Perry, C., Ramjiawan, R., Roberts, J., Coates, T., Salvatore, F., Bainbridge, A., Clarke, J. A., Krumpa, N., Shepherd, B. J. A., Walsh, D., Chekanov, S., Demarteau, M., Gai, W., Liu, W., Metcalfe, J., Power, J., Repond, J., Weerts, H., Xia, L., Zupan, J., Wells, J. D., Zhang, Z., Adolphsen, C., Barklow, T., Dolgashev, V., Franzi, M., Graf, N., Hewett, J., Kemp, M., Kononenko, O., Markiewicz, T., Moffeit, K., Neilson, J., Nosochkov, Y., Oriunno, M., Phinney, N., Rizzo, T., Tantawi, S., Wang, J., Weatherford, B., White, G., and Woodley, M.
- Subjects
Technology ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,ddc:600 ,Accelerators and Storage Rings ,physics.acc-ph - Abstract
The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^-$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively. CLIC uses a two-beam acceleration scheme, in which 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept has been refined using improved software tools. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations and parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25-30 years.
46. Search for TeV gamma-rays from the active radio galaxy centaurus a with CANGAROO-III
- Author
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Kabuki, S., Enomoto, R., Adachi, Y., Asahara, A., Bicknell, G. V., Roger Clay, Doi, Y., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Hattori, T., Hayashi, S., Higashi, Y., Inoue, R., Itoh, C., Kajino, F., Katagiri, H., Kawachi, A., Kawasaki, S., Kifune, T., Kiuchi, R., Konno, K., Ksenofontov, L. T., Kubo, H., Kushida, J., Matsubara, Y., Mizumoto, Y., Mori, M., Muraishi, H., Muraki, Y., Naito, T., Nakamori, T., Nishida, D., Nishijima, K., Ohishi, M., Patterson, J. R., Protheroe, R. J., Sakamoto, Y., Sato, M., Suzuki, S., Suzuki, T., Swaby, D. L., Tanimori, T., Tanimura, H., Thornton, G., Tsuchiya, K., Watanabe, S., Yamaoka, T., Yamazaki, M., Yanagita, S., Yoshida, T., Yoshikoshi, T., Yuasa, M., and Yukawa, Y.
47. A case report of complete pathological response of a locally advanced rectal cancer after long term chemotherapy
- Author
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Kobayashi, M., Ohnuma, S., Kato, S., Hideaki Karasawa, Aoki, T., Kudo, K., Tanaka, N., Watanabe, K., Nagao, M., Abe, T., Musha, H., Morikawa, T., Motoi, F., Katayose, Y., Naito, T., and Unno, M.
48. Monte Carlo Simulations and Validation of NectarCAM, a Medium Sized Telescope Camera for CTA
- Author
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Armstrong, T. P., Costantini, H., Glicenstein, J. -F, Lenain, J. -P, Schwanke, U., Tavernier, T., Abdalla, H., Abe, H., Abe, S., Abusleme, A., Acero, F., Acharyya, A., Acín Portella, V., Ackley, K., Adam, R., Adams, C., Adhikari, S. S., Aguado-Ruesga, I., Agudo, I., Aguilera, R., Aguirre-Santaella, A., Aharonian, F., Alberdi, A., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Alves Batista, R., Amans, J. -P, Amati, L., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Ammendola, R., Anderson, J., Anduze, M., Angüner, E. O., Antonelli, L. A., Antonuccio, V., Antoranz, P., Anutarawiramkul, R., Aragunde Gutierrez, J., Aramo, C., Araudo, A., Araya, M., Arbet-Engels, A., Arcaro, C., Arendt, V., Armand, C., Armstrong, T., Arqueros, F., Arrabito, L., Arsioli, B., Artero, M., Asano, K., Ascasíbar, Y., Aschersleben, J., Ashley, M., Attinà, P., Aubert, P., Singh, C. B., Baack, D., Babic, A., Backes, M., Baena, V., Bajtlik, S., Baktash, A., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Balmaverde, B., Bamba, A., Bandiera, R., Baquero Larriva, A., Barai, P., Barbier, C., Barbosa Martins, V., Barcelo, M., Barkov, M., Barnard, M., Baroncelli, L., Barres Almeida, U., Barrio, J. A., Bastieri, D., Batista, P. I., Batkovic, I., Bauer, C., Bautista-González, R., Baxter, J., Becciani, U., Becerra González, J., Becherini, Y., Beck, G., Becker Tjus, J., Bednarek, W., Belfiore, A., Bellizzi, L., Belmont, R., Benbow, W., Berge, D., Bernardini, E., Bernardos, M. I., Bernlöhr, K., Berti, A., Berton, M., Bertucci, B., Beshley, V., Bhatt, N., Bhattacharyya, S., Bhattacharyya, W., Bi, B., Bicknell, G., Biederbeck, N., Bigongiari, C., Biland, A., Bird, R., Bissaldi, E., Biteau, J., Bitossi, M., Blanch, O., Blank, M., Blazek, J., Bobin, J., Boccato, C., Bocchino, F., Boehm, C., Bohacova, M., Boisson, C., Boix, J., Bolle, J. -P, Bolmont, J., Bonanno, G., Bonavolontà, C., Bonneau Arbeletche, L., Bonnoli, G., Bordas, P., Borkowski, J., Bórquez, S., Bose, R., Bose, D., Bosnjak, Z., Bottacini, E., Böttcher, M., Botticella, M. T., Boutonnet, C., Bouyjou, F., Bozhilov, V., Bozzo, E., Brahimi, L., Braiding, C., Brau-Nogué, S., Breen, S., Bregeon, J., Breuhaus, M., Brill, A., Brisken, W., Brocato, E., Brown, A. M., Brügge, K., Brun, P., Brun, F., Brunetti, L., Brunetti, G., Bruno, P., Bruno, A., Bruzzese, A., Bucciantini, N., Buckley, J., Bühler, R., Bulgarelli, A., Bulik, T., Bünning, M., Bunse, M., Burton, M., Burtovoi, A., Buscemi, M., Buschjäger, S., Busetto, G., Buss, J., Byrum, K., Caccianiga, A., Cadoux, F., Calanducci, A., Calderón, C., Calvo Tovar, J., Cameron, R., Campaña, P., Canestrari, R., Cangemi, F., Cantlay, B., Capalbi, M., Capasso, M., Cappi, M., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Cárdenas, V., Cardiel, L., Cardillo, M., Carlile, C., Caroff, S., Carosi, R., Carosi, A., Carquín, E., Carrère, M., Casandjian, J. -M, Casanova, S., Cascone, E., Cassol, F., Castro-Tirado, A. J., Catalani, F., Catalano, O., Cauz, D., Ceccanti, A., Celestino Silva, C., Celli, S., Cerny, K., Cerruti, M., Chabanne, E., Chadwick, P., Chai, Y., Chambery, P., Champion, C., Chandra, S., Chaty, S., Chen, A., Cheng, K., Chernyakova, M., Chiaro, G., Chiavassa, A., Chikawa, M., Chitnis, V. R., Chudoba, J., Chytka, L., Cikota, S., Circiello, A., Clark, P., Çolak, M., Colombo, E., Colome, J., Colonges, S., Comastri, A., Compagnino, A., Conforti, V., Congiu, E., Coniglione, R., Conrad, J., Conte, F., Contreras, J. L., Coppi, P., Cornat, R., Coronado-Blazquez, J., Cortina, J., Costa, A., Cotter, G., Courty, B., Covino, S., Crestan, S., Cristofari, P., Crocker, R., Croston, J., Cubuk, K., Cuevas, O., Cui, X., Cusumano, G., Cutini, S., D Aì, A., D Amico, G., D Ammando, F., D Avanzo, P., Da Vela, P., Dadina, M., Dai, S., Dalchenko, M., Dall Ora, M., Daniel, M. K., Dauguet, J., Davids, I., Davies, J., Dawson, B., Angelis, A., Araújo Carvalho, A. E., Bony Lavergne, M., Caprio, V., Cesare, G., Frondat, F., Gouveia Dal Pino, E. M., La Calle, I., Lotto, B., Luca, A., Martino, D., Menezes, R. M., Naurois, M., Oña Wilhelmi, E., Palma, F., Persio, F., Simone, N., Souza, V., Del Santo, M., Del Valle, M. V., Delagnes, E., Deleglise, G., Delfino Reznicek, M., Delgado, C., Delgado Giler, A. G., Delgado Mengual, J., Della Ceca, R., Della Valle, M., Della Volpe, D., Depaoli, D., Depouez, D., Devin, J., Di Girolamo, T., Di Giulio, C., Di Piano, A., Di Pierro, F., Di Venere, L., Díaz, C., Díaz-Bahamondes, C., Dib, C., Diebold, S., Digel, S., Dima, R., Djannati-Ataï, A., Djuvsland, J., Dmytriiev, A., Docher, K., Domínguez, A., Dominis Prester, D., Donath, A., Donini, A., Dorner, D., Doro, M., Dos Anjos, R. D. C., Dournaux, J. -L, Downes, T., Drake, G., Drass, H., Dravins, D., Duangchan, C., Duara, A., Dubus, G., Ducci, L., Duffy, C., Dumora, D., Dundas Morå, K., Durkalec, A., Dwarkadas, V. V., Ebr, J., Eckner, C., Eder, J., Ederoclite, A., Edy, E., Egberts, K., Einecke, S., Eisch, J., Eleftheriadis, C., Elsässer, D., Emery, G., Emmanoulopoulos, D., Ernenwein, J. -P, Errando, M., Escarate, P., Escudero, J., Espinoza, C., Ettori, S., Eungwanichayapant, A., Evans, P., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Fallah Ramazani, V., Falomo, R., Farakos, K., Fasola, G., Fattorini, A., Favre, Y., Fedora, R., Fedorova, E., Fegan, S., Feijen, K., Feng, Q., Ferrand, G., Ferrara, G., Ferreira, O., Fesquet, M., Fiandrini, E., Fiasson, A., Filipovic, M., Fink, D., Finley, J. P., Fioretti, V., Fiorillo, D. F. G., Fiorini, M., Flis, S., Flores, H., Foffano, L., Föhr, C., Fonseca, M. V., Font, L., Fontaine, G., Fornieri, O., Fortin, P., Fortson, L., Fouque, N., Fournier, A., Fraga, B., Franceschini, A., Franco, F. J., Franco Ordovas, A., Freixas Coromina, L., Fresnillo, L., Fruck, C., Fugazza, D., Fujikawa, Y., Fujita, Y., Fukami, S., Fukazawa, Y., Fukui, Y., Fulla, D., Funk, S., Furniss, A., Gabella, O., Gabici, S., Gaggero, D., Galanti, G., Galaz, G., Galdemard, P., Gallant, Y., Galloway, D., Gallozzi, S., Gammaldi, V., Garcia, R., Garcia, E., García, E., Garcia López, R., Garczarczyk, M., Gargano, F., Gargano, C., Garozzo, S., Gascon, D., Gasparetto, T., Gasparrini, D., Gasparyan, H., Gaug, M., Geffroy, N., Gent, A., Germani, S., Gesa, L., Ghalumyan, A., Ghedina, A., Ghirlanda, G., Gianotti, F., Giarrusso, S., Giarrusso, M., Giavitto, G., Giebels, B., Giglietto, N., Gika, V., Gillardo, F., Gimenes, R., Giordano, F., Giovannini, G., Giro, E., Giroletti, M., Giuliani, A., Giunti, L., Gjaja, M., Gliwny, P., Godinovic, N., Göksu, H., Goldoni, P., Gómez, J. L., Gómez-Vargas, G., González, M. M., González, J. M., Gothe, K. S., Götz, D., Goulart Coelho, J., Gourgouliatos, K., Grabarczyk, T., Graciani, R., Grandi, P., Grasseau, G., Grasso, D., Green, A. J., Green, D., Green, J., Greenshaw, T., Grenier, I., Grespan, P., Grillo, A., Grondin, M. -H, Grube, J., Guarino, V., Guest, B., Gueta, O., Gündüz, M., Gunji, S., Gusdorf, A., Gyuk, G., Hackfeld, J., Hadasch, D., Haga, J., Hagge, L., Hahn, A., Hajlaoui, J. E., Hakobyan, H., Halim, A., Hamal, P., Hanlon, W., Hara, S., Harada, Y., Hardcastle, M. J., Harvey, M., Hashiyama, K., Hassan Collado, T., Haubold, T., Haupt, A., Hautmann, U. A., Havelka, M., Hayashi, K., Hayashida, M., He, H., Heckmann, L., Heller, M., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Hernández Cadena, S., Herrera Llorente, J., Herrero, A., Hervet, O., Hinton, J., Hiramatsu, A., Hiroshima, N., Hirotani, K., Hnatyk, B., Hnatyk, R., Hoang, J. K., Hoffmann, D., Hofmann, W., Hoischen, C., Holder, J., Holler, M., Hona, B., Horan, D., Hörandel, J., Horns, D., Horvath, P., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huang, Y., Huet, J. -M, Hughes, G., Hui, D., Hull, G., Humensky, T. B., Hütten, M., Iaria, R., Iarlori, M., Illa, J. M., Imazawa, R., Impiombato, D., Inada, T., Incardona, F., Ingallinera, A., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Insolia, A., Iocco, F., Ioka, K., Ionica, M., Iori, M., Iovenitti, S., Iriarte, A., Ishio, K., Ishizaki, W., Iwamura, Y., Jablonski, C., Jacquemier, J., Jacquemont, M., Jamrozy, M., Janecek, P., Jankowsky, F., Jardin-Blicq, A., Jarnot, C., Jean, P., Jiménez Martínez, I., Jin, W., Jocou, L., Jordana, N., Josselin, M., Jouvin, L., Jung-Richardt, I., Junqueira, F. J. P. A., Juramy-Gilles, C., Jurysek, J., Kaaret, P., Kadowaki, L. H. S., Kagaya, M., Kalekin, O., Kankanyan, R., Kantzas, D., Karas, V., Karastergiou, A., Karkar, S., Kasai, E., Kasperek, J., Katagiri, H., Kataoka, J., Katarzyński, K., Katsuda, S., Katz, U., Kawanaka, N., Kazanas, D., Kerszberg, D., Khélifi, B., Kherlakian, M. C., Kian, T. P., Kieda, D. B., Kihm, T., Kim, S., Kimeswenger, S., Kisaka, S., Kissmann, R., Kleijwegt, R., Kleiner, T., Kluge, G., Kluźniak, W., Knapp, J., Knödlseder, J., Kobakhidze, A., Kobayashi, Y., Koch, B., Kocot, J., Kohri, K., Kokkotas, K., Komin, N., Kong, A., Kosack, K., Kowal, G., Krack, F., Krause, M., Krennrich, F., Krumholz, M., Kubo, H., Kudryavtsev, V., Samridha Kunwar, Kuroda, Y., Kushida, J., Kushwaha, P., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lahmann, R., Lamanna, G., Lamastra, A., Landoni, M., Landriu, D., Lang, R. G., Lapington, J., Laporte, P., Lason, P., Lasuik, J., Lazendic-Galloway, J., Le Flour, T., Le Sidaner, P., Leach, S., Leckngam, A., Lee, S. -H, Lee, W. H., Lee, S., Leigui Oliveira, M. A., Lemière, A., Lemoine-Goumard, M., Leone, F., Leray, V., Leto, G., Leuschner, F., Levy, C., Lindemann, R., Lindfors, E., Linhoff, L., Liodakis, I., Lipniacka, A., Lloyd, S., Lobo, M., Lohse, T., Lombardi, S., Longo, F., Lopez, A., López, M., López-Coto, R., Loporchio, S., Louis, F., Louys, M., Lucarelli, F., Lucchesi, D., Ludwig Boudi, H., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maccarone, T., Mach, E., Maciejewski, A. J., Mackey, J., Madejski, G. M., Maeght, P., Maggio, C., Maier, G., Majczyna, A., Majumdar, P., Makariev, M., Mallamaci, M., Malta Nunes Almeida, R., Maltezos, S., Malyshev, D., Mandat, D., Maneva, G., Manganaro, M., Manicò, G., Manigot, P., Mannheim, K., Maragos, N., Marano, D., Marconi, M., Marcowith, A., Marculewicz, M., Marčun, B., Marín, J., Marinello, N., Marinos, P., Mariotti, M., Markoff, S., Marquez, P., Marsella, G., Martí, J., Martin, J. -M, Martin, P., Martinez, O., Martínez, M., Martínez, G., Martínez, O., Martínez-Huerta, H., Marty, C., Marx, R., Masetti, N., Massimino, P., Mastichiadis, A., Matsumoto, H., Matthews, N., Maurin, G., Max-Moerbeck, W., Maxted, N., Mazin, D., Mazziotta, M. N., Mazzola, S. M., Mbarubucyeye, J. D., Mc Comb, L., Mchardy, I., Mckeague, S., Mcmuldroch, S., Medina, E., Medina Miranda, D., Melandri, A., Melioli, C., Melkumyan, D., Menchiari, S., Mender, S., Mereghetti, S., Merino Arévalo, G., Mestre, E., Meunier, J. -L, Meures, T., Meyer, M., Micanovic, S., Miceli, M., Michailidis, M., Michałowski, J., Miener, T., Mievre, I., Miller, J., Minaya, I. A., Mineo, T., Minev, M., Miranda, J. M., Mirzoyan, R., Mitchell, A., Mizuno, T., Mode, B., Moderski, R., Mohrmann, L., Molina, E., Molinari, E., Montaruli, T., Monteiro, I., Moore, C., Moralejo, A., Morcuende-Parrilla, D., Moretti, E., Morganti, L., Mori, K., Moriarty, P., Morik, K., Morlino, G., Morris, P., Morselli, A., Mosshammer, K., Moya, P., Mukherjee, R., Muller, J., Mundell, C., Mundet, J., Murach, T., Muraczewski, A., Muraishi, H., Murase, K., Musella, I., Musumarra, A., Nagai, A., Nagar, N., Nagataki, S., Naito, T., Nakamori, T., Nakashima, K., Nakayama, K., Nakhjiri, N., Naletto, G., Naumann, D., Nava, L., Navarro, R., Nawaz, M. A., Ndiyavala, H., Neise, D., Nellen, L., Nemmen, R., Newbold, M., Neyroud, N., Ngernphat, K., Nguyen Trung, T., Nicastro, L., Nickel, L., Niemiec, J., Nieto, D., Nievas, M., Nigro, C., Nikołajuk, M., Ninci, D., Nishijima, K., Noda, K., Nogami, Y., Nolan, S., Nomura, R., Norris, R., Nosek, D., Nöthe, M., Novosyadlyj, B., Novotny, V., Nozaki, S., Nunio, F., O Brien, P., Obara, K., Oger, R., Ohira, Y., Ohishi, M., Ohm, S., Ohtani, Y., Oka, T., Okazaki, N., Okumura, A., Olive, J. -F, Oliver, C., Olivera, G., Olmi, B., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, S., Orlando, E., Osborne, J. P., Ostrowski, M., Otte, N., Ovcharov, E., Owen, E., Oya, I., Ozieblo, A., Padovani, M., Pagano, I., Pagliaro, A., Paizis, A., Palatiello, M., Palatka, M., Palazzi, E., Panazol, J. -L, Paneque, D., Panes, B., Panny, S., Pantaleo, F. R., Panter, M., Paoletti, R., Paolillo, M., Papitto, A., Paravac, A., Paredes, J. M., Pareschi, G., Park, N., Parmiggiani, N., Parsons, R. D., Paśko, P., Patel, S., Patricelli, B., Pauletta, G., Pavletić, L., Pavy, S., Pe Er, A., Pech, M., Pecimotika, M., Pellegriti, M. G., Peñil Del Campo, P., Penno, M., Pepato, A., Perard, S., Perennes, C., Peres, G., Peresano, M., Pérez-Aguilera, A., Pérez-Romero, J., Pérez-Torres, M. A., Perri, M., Persic, M., Petrera, S., Petrucci, P. -O, Petruk, O., Peyaud, B., Pfrang, K., Pian, E., Piano, G., Piatteli, P., Pietropaolo, E., Pillera, R., Pilszyk, B., Pimentel, D., Pintore, F., Pio García, C., Pirola, G., Piron, F., Pisarski, A., Pita, S., Pohl, M., Poireau, V., Poledrelli, P., Pollo, A., Polo, M., Pongkitivanichkul, C., Porthault, J., Powell, J., Pozo, D., Prado, R. R., Prandini, E., Prasit, P., Prast, J., Pressard, K., Principe, G., Priyadarshi, C., Produit, N., Prokhorov, D., Prokoph, H., Prouza, M., Przybilski, H., Pueschel, E., Pühlhofer, G., Puljak, I., Pumo, M. L., Punch, M., Queiroz, F., Quinn, J., Quirrenbach, A., Rainò, S., Rajda, P. J., Rando, R., Razzaque, S., Rebert, E., Recchia, S., Reichherzer, P., Reimer, O., Reimer, A., Reisenegger, A., Remy, Q., Renaud, M., Reposeur, T., Reville, B., Reymond, J. -M, Reynolds, J., Rhode, W., Ribeiro, D., Ribó, M., Richards, G., Richtler, T., Rico, J., Rieger, F., Riitano, L., Ripepi, V., Riquelme, M., Riquelme, D., Rivoire, S., Rizi, V., Roache, E., Röben, B., Roche, M., Rodriguez, J., Rodriguez Fernandez, G., Rodriguez Ramirez, J. C., Rodríguez Vázquez, J. J., Roepke, F., Rojas, G., Romanato, L., Romano, P., Romeo, G., Romero Lobato, F., Romoli, C., Roncadelli, M., Ronda, S., Rosado, J., Rosales Leon, A., Rowell, G., Rudak, B., Rugliancich, A., Ruíz Del Mazo, J. E., Rujopakarn, W., Rulten, C., Russell, C., Russo, F., Sadeh, I., Sæther Hatlen, E., Safi-Harb, S., Saha, L., Saha, P., Sahakian, V., Sailer, S., Saito, T., Sakaki, N., Sakurai, S., Salesa Greus, F., Salina, G., Salzmann, H., Sanchez, D., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Santangelo, A., Santos, E. M., Santos-Lima, R., Sanuy, A., Sapozhnikov, L., Saric, T., Sarkar, S., Sasaki, H., Sasaki, N., Satalecka, K., Sato, Y., Saturni, F. G., Sawada, M., Sawangwit, U., Schaefer, J., Scherer, A., Scherpenberg, J., Schipani, P., Schleicher, B., Schmoll, J., Schneider, M., Schoorlemmer, H., Schovanek, P., Schussler, F., Schwab, B., Schwarz, J., Schweizer, T., Sciacca, E., Scuderi, S., Seglar Arroyo, M., Segreto, A., Seitenzahl, I., Semikoz, D., Sergijenko, O., Serna Franco, J. E., Servillat, M., Seweryn, K., Sguera, V., Shalchi, A., Shang, R. Y., Sharma, P., Shellard, R. C., Sidoli, L., Sieiro, J., Siejkowski, H., Silk, J., Sillanpää, A., Singh, B. B., Singh, K. K., Sinha, A., Siqueira, C., Sironi, G., Sitarek, J., Sizun, P., Sliusar, V., Slowikowska, A., Sobczyńska, D., Sobrinho, R. W., Sol, H., Sottile, G., Spackman, H., Specovius, A., Spencer, S., Spengler, G., Spiga, D., Spolon, A., Springer, W., Stamerra, A., Stanič, S., Starling, R., Stawarz, Ł., Steenkamp, R., Stefanik, S., Stegmann, C., Steiner, A., Steinmassl, S., Stella, C., Steppa, C., Sternberger, R., Sterzel, M., Stevens, C., Stevenson, B., Stolarczyk, T., Stratta, G., Straumann, U., Strišković, J., Strzys, M., Stuik, R., Suchenek, M., Suda, Y., Sunada, Y., Suomijarvi, T., Suric, T., Sutcliffe, P., Suzuki, H., Świerk, P., Szepieniec, T., Tacchini, A., Tachihara, K., Tagliaferri, G., Tajima, H., Tajima, N., Tak, D., Takahashi, K., Takahashi, H., Takahashi, M., Takata, J., Takeishi, R., Tam, T., Tanaka, M., Tanaka, T., Tanaka, S., Tateishi, D., Tavani, M., Tavecchio, F., Taylor, L., Taylor, A., Tejedor, L. A., Temnikov, P., Terada, Y., Terauchi, K., Terrazas, J. C., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thibaut, D., Thocquenne, F., Tian, W., Tibaldo, L., Tiengo, A., Tiziani, D., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Toma, K., Tomankova, L., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tosti, L., Totani, T., Tothill, N., Toussenel, F., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Trois, A., Truzzi, S., Tsiahina, A., Tsuru, T., Turk, B., Tutone, A., Uchiyama, Y., Umana, G., Utayarat, P., Vaclavek, L., Vacula, M., Vagelli, V., Vagnetti, F., Vakili, F., Valdivia, J. A., Valentino, M., Valio, A., Vallage, B., Vallania, P., Valverde Quispe, J. V., Den Berg, A. M., Driel, W., Eldik, C., Rensburg, C., Soelen, B., Vandenbroucke, J., Vanderwalt, J., Vasileiadis, G., Vassiliev, V., Vázquez Acosta, M., Vecchi, M., Vega, A., Veh, J., Veitch, P., Venault, P., Venter, C., Ventura, S., Vercellone, S., Vergani, S., Verguilov, V., Verna, G., Vernetto, S., Verzi, V., Vettolani, G. P., Veyssiere, C., Viale, I., Viana, A., Viaux, N., Vicha, J., Vignatti, J., Vigorito, C. F., Villanueva, J., Vink, J., Vitale, V., Vittorini, V., Vodeb, V., Voelk, H., Vogel, N., Voisin, V., Vorobiov, S., Vovk, I., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Wagner, P., Wakazono, K., Wakely, S. P., Walter, R., Ward, M., Warren, D., Watson, J., Webb, N., Wechakama, M., Wegner, P., Weinstein, A., Weniger, C., Werner, F., Wetteskind, H., White, M., White, R., Wierzcholska, A., Wiesand, S., Wijers, R., Wilkinson, M., Will, M., Williams, D. A., Williams, J., Williamson, T., Wolter, A., Wong, Y. W., Wood, M., Wunderlich, C., Yamamoto, T., Yamamoto, H., Yamane, Y., Yamazaki, R., Yanagita, S., Yang, L., Yoo, S., Yoshida, T., Yoshikoshi, T., Yu, P., Yusafzai, A., Zacharias, M., Zaharijas, G., Zaldivar, B., Zampieri, L., Zanmar Sanchez, R., Zaric, D., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zenin, A., Zerwekh, A., Zhdanov, V. I., Ziętara, K., Zink, A., Ziółkowski, J., Zitelli, V., Živec, M., and Zmija, A.
49. A case of pancreatic cancer with local recurrence and liver metastases eight years after surgery
- Author
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Taniguchi, H., Mizuma, M., Motoi, F., Abe, T., Okada, R., Kawaguchi, K., Karasawa, H., Masuda, K., Yabuuchi, S., Fukase, K., Naoaki Sakata, Okada, T., Nakagawa, K., Hayashi, H., Morikawa, T., Yoshida, H., Naito, T., Katayose, Y., Egawa, S., and Unno, M.
50. Proposal of the Next Incarnation of Accelerator Test Facility at KEK for the International Linear Collider
- Author
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Araki, S., Hayano, H., Higashi, Y., Honda, Y., Kanazawa, K., Kubo, K., Kume, T., Kuriki, M., Kuroda, S., Masuzawa, M., Naito, T., Okugi, T., Sugahara, R., Takahashi, T., Tauchi, T., Terunuma, N., Toge, N., Urakawa, J., Vogel, V., Yamaoka, H., Yokoya, K., Ibaraki, Gao, J., Liu, W., Pei, G., Wang, J., Grishanov, B., Logachev, P., Podgorny, F., Telnov, V., Angal-Kalinin, D., Appleby, R., Jones, J., Kalinin, A., Napoly, O., Payet, J., Saclay, Braun, Hans-Heinrich, Schulte, D., Zimmermann, F., Iwashita, Y., Mihara, T., Icr, Kyoto, Bambade, P., Gronberg, J., Kumada, M., Danagoulian, S., Mtingwa, S., Delerue, N., Howell, D., Reichold, A., Urner, D., Choi, J., Huang, J. -Y, Kang, H. S., Kim, E. -S, Kim, S., Ko, I. S., Burrows, P., Christian, G., Molloy, S., White, G., Agapov, I., Blair, G., Boorman, G., Carter, J., Driouichi, C., Price, M., Walker, N., Bane, K., Brachmann, A., Himel, T., Markiewicz, Thomas W., Nelson, J., Phinney, N., Pivi, M., Raubenheimer, T., Marc Ross, Ruland, R., Seryi, Andrei, Spencer, Cherrill M., Tenenbaum, P., Woodley, M., Boogert, S., Liapine, A., Malton, S., Torrence, E., Sanuki, T., and Suehara, T.
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