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321
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322por An, Zhendong, Qiu, Weiwei, Jiang, Wei, Yang, Gaole, Li, Xiankai, Liao, Zhengfa, Zhuang, Ziyue, Zhang, Xiaoping, Chen, Shengli, Guo, Chenchen, Xiao, Erxi, Fang, Xiao, Li, Xinxiang, Wang, Hongwei, Hu, Xinrong, Jiang, Bing, Shen, Wenqing, Wang, Jincheng, Ren, Jie, Ruan, Xichao, Wang, Dexin, Zhang, Su-Yalatu, Luo, Wen, Zhu, Zhichao, Lan, Haoyang, Cao, Zongwei, Ma, Xu, Liu, Yingdu, Wang, Pusen, Yang, Yi, Su, Ping, Deng, Xiangai, He, Wanbing, Ma, Yugang, Ma, Chunwang, Wang, Yuting, He, Pengqin, Tang, Renguang, Zhou, Tao, Wang, Jing, Yi, Han, Zhang, Yue, Chen, Yonghao, Fan, Ruirui, Gao, Keqing, Li, Qiang, Sun, Kang, Tan, Zhixin, Gu, Minhao, Jing, Hantao, Tang, Jingyu“…The new measurements strongly constrain the MACS of [Formula: see text] Ta([Formula: see text] ) reaction in the stellar s-process temperatures.…”
Publicado 2023
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323“…Stellar point image coordinates are one of the important observations needed for high-precision space attitude measurement with a star sensor. …”
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324
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325
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326por Fujii, K, Mosconi, M, Mengoni, A, Domingo-Pardo, C, Kappeler, F, Abbondanno, U, Aerts, G, Alvarez-Pol, H, Alvarez-Velarde, F, Andriamonje, S, Andrzejewski, J, Assimakopoulos, P, Audouin, L, Badurek, G, Baumann, P, Becvar, F, Belloni, F, Berthoumieux, E, Bisterzo, S, Calviani, M, Calvino, F, Cano-Ott, D, Capote, R, Carrillo de Albornoz, A, Cennini, P, Chepel, V, Chiaveri, E, Colonna, N, Cortes, G, Couture, A, Cox, J, Dahlfors, M, David, S, Dillmann, I, Dolfini, R, Dridi, W, Duran, I, Eleftheriadis, C, Embid-Segura, M, Ferrant, L, Ferrari, A, Ferreira-Marques, R, Fitzpatrick, L, Frais-Koelbl, H, Furman, W, Gallino, R, Goncalves, I, Gonzalez-Romero, E, Goverdovski, A, Gramegna, F, Griesmayer, E, Guerrero, C, Gunsing, F, Haas, B, Haight, R, Heil, M, Herrera-Martinez, A, Igashira, M, Isaev, S, Jericha, E, Kadi, Y, Karamanis, D, Karadimos, D, Kerveno, M, Ketlerov, V, Koehler, P, Konovalov, V, Kossionides, E, Krticka, M, Lamboudis, C, Leeb, H, Lindote, A, Lopes, I, Lozano, M, Lukic, S, Marganiec, J, Marques, L, Marrone, S, Massimi, C, Mastinu, P, Milazzo, P M, Moreau, C, Neves, F, Oberhummer, H, Oshima, M, O'Brien, S, Pancin, J, Papachristodoulou, C, Papadopoulos, C, Paradela, C, Patronis, N, Pavlik, A, Pavlopoulos, P, Perrot, L, Plag, R, Plompen, A, Plukis, A, Poch, A, Praena, J, Pretel, C, Quesada, J, Rauscher, T, Reifarth, R, Rosetti, M, Rubbia, C, Rudolf, G, Rullhusen, P, Salgado, J, Sarchiapone, L, Savvidis, I, Stephan, C, Tagliente, G, Tain, J L, Tassan-Got, L, Tavora, L, Terlizzi, R, Vannini, G, Vaz, P, Ventura, Alberto, Villamarin, D, Vincente, M C, Vlachoudis, V, Vlastou, R, Voss, F, Walter, S, Wendler, H, Wiescher, M, Wisshak, KEnlace del recurso
Publicado 2010
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327
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328por Jin, Jing, Tang, Yuan, Hu, Chen, Jiang, Li-Ming, Jiang, Jun, Li, Ning, Liu, Wen-Yang, Chen, Si-Lin, Li, Shuai, Lu, Ning-Ning, Cai, Yong, Li, Yong-Heng, Zhu, Yuan, Cheng, Guang-Hui, Zhang, Hong-Yan, Wang, Xin, Zhu, Su-Yu, Wang, Jun, Li, Gao-Feng, Yang, Jia-Lin, Zhang, Kuan, Chi, Yihebali, Yang, Lin, Zhou, Hai-Tao, Zhou, Ai-Ping, Zou, Shuang-Mei, Fang, Hui, Wang, Shu-Lian, Zhang, Hai-Zeng, Wang, Xi-Shan, Wei, Li-Chun, Wang, Wen-Ling, Liu, Shi-Xin, Gao, Yuan-Hong, Li, Ye-XiongEnlace del recurso
Publicado 2022
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329por Goeminne, G, Wagemans, C, Wagemans, J, Geltenbort, P, Loiselet, M, Gaelens, M, Denecke, B, Köster, U“…Therefore, complementary measurements were performed with thermal neutrons at the High Flux Reactor of the ILL (Grenoble, France) and with resonance neutrons at the GELINA neutron spectrometer of the IRMM (Geel, Belgium). The stellar cross sections, which were calculated from the obtained data, show important discrepancies with the theoretical values used in recent network calculations.…”
Publicado 2001
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330por Kubono, S, Michimasa, S, Teranishi, T, Yanagisawa, Y, Fülöp, Z, Liu, X, Kumagai, K, Abe, K, Yun, C C, Watanabe, S, Yamazaki, N, Ohshiro, Y, Kurokawa, M, Strasser, P, Hahn, K I, Kishida, T, Imai, N, Kato, S, Fuchi, Y, Tanaka, M HEnlace del recurso
Publicado 2001
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331por Le, Dung T, Crocenzi, Todd S, Urum, Jennifer N, Lutz, Eric R, Laheru, Daniel A, Sugar, Elizabeth A, Vonderheide, Robert H, Fisher, George A, Ko, Andrew H, Murphy, Aimee L, McDougall, Katherine, Ferber, Sandy, Brockstedt, Dirk G, Jaffee, Elizabeth MEnlace del recurso
Publicado 2015
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332
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333por Babiano-Suarez, V, Balibrea-Correa, J, Caballero-Ontanaya, L, Domingo-Pardo, C, Ladarescu, I, Lerendegui-Marco, J, Tain, J L, Calviño, F, Casanovas, A, Tarifeño-Saldivia, A, Guerrero, C, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Bacak, M, Barbagallo, M, Bennett, S, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Busso, M, Caamaño, M, Calviani, M, Cano-Ott, D, Cerutti, F, Chiaveri, E, Colonna, N, Cortés, G, CortésGiraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Davies, P J, Diakaki, M, Dietz, M, Dressler, R, Ducasse, Q, Dupont, E, Durán, I, Eleme, Z, Fernández-Domínguez, B, Ferrari, A, Finocchiaro, P, Furman, V, Göbel, K, Garg, R, Gawlik-Ramięga, A, Gilardoni, S, Gonçalves, I F, González-Romero, E, Gunsing, F, Harada, H, Heinitz, S, Heyse, J, Jenkins, D G, Junghans, A, Käppeler, F, Kadi, Y, Kimura, A, Knapová, I, Kokkoris, M, Kopatch, Y, Krtička, M, Kurtulgil, D, Lederer-Woods, C, Leeb, H, Lonsdale, S J, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Mastromarco, M, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Mingrone, F, Moreno-Soto, J, Musumarra, A, Negret, A, Nolte, R, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Persanti, L, Petrone, C, Pirovano, E, Porras, I, Praena, J, Quesada, J M, Ramos-Doval, D, Rauscher, T, Reifarth, R, Rochman, D, Romanets, Y, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Sekhar, A, Smith, A G, Sosnin, N V, Sprung, P, Stamatopoulos, A, Tagliente, G, Tassan-Got, L, Thomas, Th, Torres-Sánchez, P, Tsinganis, A, Ulrich, J, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T, Žugec, P“…Most elements heavier than iron have been generated in the stellar media by means of neutron capture reactions, approximately half are produced by the slow neutron capture or s-process. …”
Publicado 2022
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334
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335
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336por Appleby, Niamh, Eyre, Toby A., Cabes, Maite, Jackson, Aimee, Boucher, Rebecca, Yates, Francesca, Fox, Sonia, Rawstron, Andrew, Hillmen, Peter, Schuh, Anna“…The single-arm platform studies enable the incorporation of promising novel therapies into the protocol. The STELLAR study has potential to identify novel biomarkers of treatment response in this high-risk malignancy. …”
Publicado 2019
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337por Krishnamurti, Lakshmanan, Arnold, Staci D, Haight, Ann, Abraham, Allistair, Guilcher, Gregory MT, John, Tami, Bakshi, Nitya, Shenoy, Shalini, Syrjala, Karen, Martin, Paul L, Chaudhury, Sonali, Eames, Gretchen, Olowoselu, Olusola Festus, Hsieh, Matthew, De La Fuente, Josu, Kasow, Kimberly A, Stenger, Elizabeth, Mertens, Anne, El-Rassi, Fuad, Lane, Peter, Shaw, Bronwen E, Meacham, Lillian, Archer, David“…CONCLUSIONS: It is feasible to recruit subjects and conduct study procedures for STELLAR in order to determine the long-term and late effects of HCT for SCD. …”
Publicado 2022
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338
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339Publicado 1967Tabla de Contenidos:Procedimiento de la Conferencia Libro
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