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  1. 1021
  2. 1022
    “…SIMPLE SUMMARY: Fossils are the only direct evidence of life throughout Earth’s history. We examine the biology of ancient animals to learn about evolution and past ecosystems. …”
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  3. 1023
    “…The total calculated volume of erupted fallout deposit is 0.057 km(3), 0.042 km(3), or 0.090 km(3) using the exponential, power-law, and Weibull models, respectively, and all translate to a VEI of 3. …”
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  4. 1024
    Publicado 2002
    “…It is made by carbon fiber radiators and straw tube detectors and its main task is to complement the calorimeter in the particle identification; \\ 4. a plastic scintillator hodoscope system (TOF) providing the triggers, the charge determination and a precise time measurement plus an anti-coincidence system to identify particles interacting in the mechanical structure of the telescope (ANTI). \\ \\ The total height of PAMELA is 120 cm, the mass is 410 kg, the power consumption is 345 W and the geometrical factor is 20.5 $cm^{2}$ sr. \\ \\ Several tests have been performed at CERN PS (t9) and SPS (X7) beams during years 1999 and 2000 on prototypes of the detectors. …”
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  5. 1025
    por Lucchini, Marco Toliman
    Publicado 2014
    “…Attention is focused on inorganic crystals (LuAG, YAG, LSO, YSO) doped with rare earth ions (Ce$^{3+}$, Pr$^{3+}$) and cerium doped quartz (SiO$_2$:Ce) and barium disilicate (DSB:Ce). …”
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  6. 1026
    por Patwardhan, Juilee, Bhatt, Purvi
    Publicado 2016
    “…BACKGROUND: Ultraviolet-B (UV-B) radiation is a smaller fraction of the total radiation reaching the Earth but leads to extensive damage to the deoxyribonucleic acid (DNA) and other biomolecules through formation of free radicals altering redox homeostasis of the cell. …”
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  7. 1027
    por Stahl, A, Wiebusch, C, Guler, A M, Kamiscioglu, M, Sever, R, Yilmazer, A U, Gunes, C, Yilmaz, D, Del Amo Sanchez, P, Duchesneau, D, Pessard, H, Marcoulaki, E, Papazoglou, I A, Berardi, V, Cafagna, F, Catanesi, M G, Magaletti, L, Mercadante, A, Quinto, M, Radicioni, E, Ereditato, A, Kreslo, I, Pistillo, C, Weber, M, Ariga, A, Ariga, T, Strauss, T, Hierholzer, M, Kawada, J, Hsu, C, Haug, S, Jipa, A, Lazanu, I, Cardini, A, Lai, A, Oldeman, R, Thomson, M, Blake, A, Prest, M, Auld, A, Elliot, J, Lumbard, J, Thompson, C, Gornushkin, Y A, Pascoli, S, Collins, R, Haworth, M, Thompson, J, Bencivenni, G, Domenici, D, Longhin, A, Blondel, A, Bravar, A, Dufour, F, Karadzhov, Y, Korzenev, A, Noah, E, Ravonel, M, Rayner, M, Asfandiyarov, R, Haesler, A, Martin, C, Scantamburlo, E, Cadoux, F, Bayes, R, Soler, F J P, Aalto-Setälä, L, Enqvist, K, Huitu, K, Rummukainen, K, Nuijten, G, Eskola, K J, Kainulainen, K, Kalliokoski, T, Kumpulainen, J, Loo, K, Maalampi, J, Manninen, M, Moore, I, Suhonen, J, Trzaska, W H, Tuominen, K, Virtanen, A, Bertram, I, Finch, A, Grant, N, Kormos, L L, Ratoff, P, Christodoulou, G, Coleman, J, Touramanis, C, Mavrokoridis, K, Murdoch, M, McCauley, N, Payne, D, Jonsson, P, Kaboth, A, Long, K, Malek, M, Scott, M, Uchida, Y, Wascko, M O, Di Lodovico, F, Wilson, J R, Still, B, Sacco, R, Terri, R, Campanelli, M, Nichol, R, Thomas, J, Izmaylov, A, Khabibullin, M, Khotjantsev, A, Kudenko, Y, Matveev, V, Mineev, O, Yershov, N, Palladino, V, Evans, J, Söldner-Rembold, S, Yang, U K, Bonesini, M, Pihlajaniemi, T, Weckström, M, Mursula, K, Enqvist, T, Kuusiniemi, P, Räihä, T, Sarkamo, J, Slupecki, M, Hissa, J, Kokko, E, Aittola, M, Barr, G, Haigh, M D, de Jong, J, O'Keeffe, H, Vacheret, A, Weber, A, Galvanin, G, Temussi, M, Caretta, O, Davenne, T, Densham, C, Ilic, J, Loveridge, P, Odell, J, Wark, D, Robert, A, Andrieu, B, Popov, B, Giganti, C, Levy, J -M, Dumarchez, J, Buizza-Avanzini, M, Cabrera, A, Dawson, J, Franco, D, Kryn, D, Obolensky, M, Patzak, T, Tonazzo, A, Vanucci, F, Orestano, D, Di Micco, B, Tortora, L, Bésida, O, Delbart, A, Emery, S, Galymov, V, Mazzucato, E, Vasseur, G, Zito, M, Kudryavtsev, V A, Thompson, L F, Tsenov, R, Kolev, D, Rusinov, I, Bogomilov, M, Vankova, G, Matev, R, Vorobyev, A, Novikov, Yu, Kosyanenko, S, Suvorov, V, Gavrilov, G, Baussan, E, Dracos, M, Jollet, C, Meregaglia, A, Vallazza, E, Agarwalla, S K, Li, T, Autiero, D, Chaussard, L, Déclais, Y, Marteau, J, Pennacchio, E, Rondio, E, Lagoda, J, Zalipska, J, Przewlocki, P, Grzelak, K, Barker, G J, Boyd, S, Harrison, P F, Litchfield, R P, Ramachers, Y, Badertscher, A, Curioni, A, Degunda, U, Epprecht, L, Gendotti, A, Knecht, L, Di Luise, S, Horikawa, S, Lussi, D, Murphy, S, Natterer, G, Petrolo, F, Periale, L, Rubbia, A, Sergiampietri, F, Viant, T
    Publicado 2012
    “…With a three-fold increase in exposure (defined as the product neutrino beam power $\times$ far detector target mass), CPV becomes accessible at $>3\sigma$~C.L. for 75\% of the $\delta_{CP}$ parameter space, assuming that all systematic errors can be controlled below the 5\% level. …”
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