Results 51 to 60 of about 353,889 (361)

Error analysis of Abel retrieved electron density profiles from radio occultation measurements [PDF]

Annales Geophysicae, 2010
This letter reports for the first time the simulated error distribution of radio occultation (RO) electron density profiles (EDPs) from the Abel inversion in a systematic way.
X. Yue, X. Yue, W. S. Schreiner, J. Lei, S. V. Sokolovskiy, C. Rocken, D. C. Hunt, Y.-H. Kuo   +7 more
doaj   +1 more source

COSMIC: mining complete cancer genomes in the Catalogue of Somatic Mutations in Cancer

Nucleic Acids Res., 2010
COSMIC (http://www.sanger.ac.uk/cosmic) curates comprehensive information on somatic mutations in human cancer. Release v48 (July 2010) describes over 136 000 coding mutations in almost 542 000 tumour samples; of the 18 490 genes documented, 4803 (26 ...
S. Forbes, Nidhi Bindal, S. Bamford, C. Cole, C. Kok, D. Beare, Mingming Jia, Rebecca Shepherd, Kenric Leung, A. Menzies, J. Teague, P. Campbell, M. Stratton, P. Futreal   +13 more
semanticscholar   +1 more source

Cosmic String Interpretation of NANOGrav Pulsar Timing Data. [PDF]

Physical Review Letters, 2020
Pulsar timing data used to provide upper limits on a possible stochastic gravitational wave background (SGWB). However, the NANOGrav Collaboration has recently reported strong evidence for a stochastic common-spectrum process, which we interpret as a ...
J. Ellis, Marek Lewicki
semanticscholar   +1 more source

Leading cluster approach to simulations of hadron collisions with GHOST generator [PDF]

EPJ Web of Conferences, 2019
The model HDPM of CORSIKA has been updated and developed on the base of the recent measurements by ALICE, CMS, TOTEM, LHCb, LHCf... The new model, GHOST, involving a four-source production reproduces correctly the pseudo-rapidity distributions of charged
Capdevielle Jean-Noël, Plebaniak Zbigniew, Szabelska Barbara, Szabelski Jacek   +3 more
doaj   +1 more source

Observation of an ultra-high-energy cosmic neutrino with KM3NeT

Nature
The detection of cosmic neutrinos with energies above a teraelectronvolt (TeV) offers a unique exploration into astrophysical phenomena1, 2–3. Electrically neutral and interacting only by means of the weak interaction, neutrinos are not deflected by ...
S. A. A. R. M. S. A. F. M. M. L. M. S. C. H. J. F. L. Aiello Albert Alhebsi Alshamsi Alves Garre Ambroso, S. Aiello, A. Albert, A. R. Alhebsi, M. Alshamsi, S. Alves Garre, A. Ambrosone, F. Ameli, M. André, M. Anghinolfi, L. Aphecetche, M. Ardid, S. Ardid, C. Argüelles, H. Atmani, J. Aublin, F. Badaracco, L. Bailly-Salins, Z. Bardacová, B. Baret, A. Bariego-Quintana, Y. Becherini, M. Bendahman, F. Benfenati Gualandi, M. Benhassi, M. Bennani, D. M. Benoit, E. Berbee, V. Bertin, S. Biagi, M. Boettcher, D. Bonanno, A. B. Bouasla, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, R. M. Bozza, H. Brânzas, F. Bretaudeau, M. Breuhaus, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, S. Buson, J. Busto, B. Caiffi, D. Calvo, A. Capone, F. Carenini, V. Carretero, T. Cartraud, P. Castaldi, V. Cecchini, S. Celli, L. Cerisy, M. Chabab, A. Chen, S. Cherubini, T. Chiarusi, M. Circella, R. Cocimano, J. Coelho, A. Coleiro, S. Colonges, A. Condorelli, R. Coniglione, P. Coyle, A. Creusot, G. Cuttone, A. D’Amico, R. Dallier, A. De Benedittis, B. De Martino, G. de Wasseige, V. Decoene, I. Del Rosso, L. S. Di Mauro, I. Di Palma, A. F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, E. Drakopoulou, D. Drouhin, J. Ducoin, R. Dvornický, T. Eberl, E. Eckerová, A. Eddymaoui, T. van Eeden, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, V. Ellajosyula, A. Enzenhöfer, G. Ferrara, M. Filipovic, F. Filippini, D. Franciotti, L. Fusco, S. Gagliardini, T. Gál, J. García Méndez, A. Garcia Soto, C. Gatius Oliver, N. Geißelbrecht, E. Genton, H. Ghaddari, L. Gialanella, B. K. Gibson, E. Giorgio, I. Goos, P. Goswami, S. Gozzini, R. Gracia, K. Graf, C. Guidi, B. Guillon, M. Gutiérrez, C. Haack, H. van Haren, A. Heijboer, L. Hennig, S. Henry, J. Hernández-Rey, W. Idrissi Ibnsalih, A. Ilioni, G. Illuminati, D. Joly, M. de Jong, P. de Jong, B. Jung, P. Kalaczynski, O. Kalekin, N. Kamp, U. Katz, G. Kistauri, C. Kopper, A. Kouchner, Y. Kovalev, V. Kueviakoe, V. Kulikovskiy, R. Kvatadze, M. Labalme, R. Lahmann, M. Lamoureux, S. Lancelin, G. Larosa, C. Lastoria, J. Lazar, A. Lazo, S. Le Stum, G. Lehaut, V. Lemaître, E. Leonora, N. Lessing, G. Levi, M. Lincetto, M. Lindsey Clark, F. Longhitano, N. Lumb, F. Magnani, J. Majumdar, L. Malerba, F. Mamedov, A. Manfreda, M. Marconi, A. Margiotta, A. Marinelli, C. Markou, L. Martin, F. Marzaioli, M. Mastrodicasa, S. Mastroianni, J. Mauro, G. Miele, P. Migliozzi, E. Migneco, M. Mitsou, C. Mollo, M. Mongelli, L. Morales-Gallegos, A. Moussa, I. Mozun Mateo, R. Muller, M. R. Musone, M. Musumeci, S. Navas, A. Nayerhoda, C. Nicolau, B. Nkosi, B. Fearraigh, V. Oliviero, A. Orlando, E. Oukacha, D. Paesani, J. Palacios González, G. Papalashvili, C. Paries, V. Parisi, E. P. Pastor Gomez, C. Pastore, A. Paun, G. Pavalas, S. Peña Martínez, M. Perrin-Terrin, V. Pestel, R. Pestes, L. Pfeiffer, P. Piattelli, A. Plavin, C. Poirè, V. Popa, T. Pradier, J. Prado, S. Pulvirenti, C. A. Quiroz-Rangel, N. Randazzo, S. Razzaque, I. C. Rea, D. Real, G. Riccobene, J. Robinson, A. Romanov, E. Ros, A. Saina, F. Salesa Greus, D. Samtleben, A. Sánchez Losa, S. Sanfilippo, M. Sanguineti, D. Santonocito, P. Sapienza, J. Schmelling, J. Schnabel, J. Schumann, H. Schutte, J. Seneca, N. Sennan, P. Sevle, I. Sgura, R. Shanidze, A. Sharma, Y. Shitov, F. Šimkovic, A. Simonelli, A. Sinopoulou, B. Spisso, M. Spurio, D. Stavropoulos, I. Stekl, M. Taiuti, Y. Tayalati, H. Thiersen, S. Thoudam, I. Tosta e Melo, B. Trocmé, V. Tsourapis, A. Tudorache, E. Tzamariudaki, A. Ukleja, A. Vacheret, V. Valsecchi, V. Van Elewyck, G. Vannoye, G. Vasileiadis, F. Vazquez de Sola, C. Verilhac, A. Veutro, S. Viola, D. Vivolo, A. van Vliet, A. Wen, E. de Wolf, I. Lhenry-Yvon, S. Zavatarelli, A. Zegarelli, D. Zito, J. Zornoza, J. Zúñiga, N. Żywucka   +286 more
semanticscholar   +1 more source

Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons [PDF]

Nature, 2017
High-energy cosmic-ray electrons and positrons (CREs), which lose energy quickly during their propagation, provide a probe of Galactic high-energy processes and may enable the observation of phenomena such as dark-matter particle annihilation or decay ...
G. Ambrosi, Q. An, R. Asfandiyarov, P. Azzarello, P. Bernardini, B. Bertucci, M. Cai, J. Chang, D. Chen, H. Chen, J. Chen, W. Chen, M. Cui, T. Cui, A. D’Amone, A. Benedittis, I. Mitri, M. D. Santo, J. N. Dong, T. Dong, Y. Dong, Z. Dong, G. Donvito, D. Droz, K. Duan, J. Duan, M. Duranti, D. D’Urso, R. Fan, Y. Fan, F. Fang, C. Feng, L. Feng, P. Fusco, V. Gallo, F. Gan, M. Gao, S. Gao, F. Gargano, S. Garrappa, K. Gong, Y. Gong, D. Guo, J. Guo, Y. Hu, G. Huang, Y. -. Huang, M. Ionica, D. Jiang, W. Jiang, X. Jin, J. Kong, S. Lei, S. Li, X. Li, W. Li, Y. Li, Y. Liang, Y. Liang, N. Liao, H. Liu, J. Liu, S. Liu, W. Liu, Y. Liu, F. Loparco, M. Ma, P. Ma, S. Ma, T. Ma, X. Ma, X. Ma, G. Marsella, M. Mazziotta, D. Mo, X. Niu, X. Peng, W. Peng, R. Qiao, J. Rao, M. Salinas, G. Shang, W. Shen, Z. Shen, Z. Shen, J. Song, H. Su, M. Su, Z. Sun, A. Surdo, X. Teng, X. Tian, A. Tykhonov, V. Vagelli, S. Vitillo, C. Wang, H. Wang, H. Wang, J. Wang, L. Wang, Q. Wang, S. Wang, X. H. Wang, X. Wang, Y. Wang, Y. Wang, Yu Wang, S. Wen, Z. Wang, D. Wei, J. Wei, Y. F. Wei, D. Wu, J. Wu, L. Wu, S. Wu, X. Wu, K. Xi, Z. Xia, Y. Xin, H. Xu, Z. L. Xu, Z. Xu, G. Xue, H. Yang, P. Yang, Y. Q. Yang, Z. L. Yang, H. Yao, Y. Yu, Q. Yuan, C. Yue, J. Zang, C. Zhang, D. L. Zhang, F. Zhang, J. Zhang, J. Zhang, J. Zhang, L. Zhang, P. Zhang, S. X. Zhang, W. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. P. Zhang, Z. Zhang, Z. Zhang, H. Zhao, H. Zhao, X. Zhao, C. Zhou, Y. Zhou, X. Zhu, Y. Zhu, S. Zimmer   +157 more
semanticscholar   +1 more source

The Updated Version of the A.Ne.Mo.S. GLE Alert System: The Case of the Ground-Level Enhancement GLE73 on 28 October 2021

Universe, 2022
A ground-level enhancement (GLE) event is a sudden increase in cosmic ray intensity originated by solar sources and recorded by ground-based detectors. GLEs are invariably associated with large solar flares that can release and accelerate solar particles
Helen Mavromichalaki, Pavlos Paschalis, Maria Gerontidou, Maria-Christina Papailiou, Evangelos Paouris, Anastasia Tezari, Dimitra Lingri, Maria Livada, Argyris N. Stassinakis, Norma Crosby, Mark Dierckxsens   +10 more
doaj   +1 more source

Cosmic superstrings

Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2008
Cosmic superstrings are expected to be formed at the end of brane inflation, within the context of brane-world cosmological models inspired from string theory. By studying the properties of cosmic superstring networks and comparing their phenomenological consequences against observational data, we aim to pin down the successful and natural inflationary
openaire   +4 more sources

Discord in Concordance Cosmology and Anomalously Massive Early Galaxies

Universe
Cosmological parameters are constrained by a wide variety of observations. We examine the concordance diagram for modern measurements of the Hubble constant, the shape parameter from the large-scale structure, the cluster baryon fraction, and the age of ...
Stacy S. McGaugh
doaj   +1 more source

Cosmic clocks, cosmic variance and cosmic averages

New Journal of Physics, 2007
Cosmic acceleration is explained quantitatively, purely in general relativity, as an apparent effect due to quasilocal gravitational energy differences that arise in the decoupling of bound systems from the global expansion of the universe. "Dark energy" is recognised as a misidentification of those aspects of gravitational energy which by virtue of ...
openaire   +3 more sources