D
David Maurin
Researcher at University of Grenoble
Publications - 232
Citations - 19193
David Maurin is an academic researcher from University of Grenoble. The author has contributed to research in topics: Cosmic ray & Dark matter. The author has an hindex of 68, co-authored 215 publications receiving 17295 citations. Previous affiliations of David Maurin include Centre national de la recherche scientifique & Joseph Fourier University.
Papers
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Journal ArticleDOI
Non-parametric determination of H and He interstellar fluxes from cosmic-ray data
TL;DR: In this article, a Markov Chain Monte Carlo (MCMCMC) engine was used to extract the PDF and correlations of the sought parameters. But the authors did not consider the effect of the modulation level on the uncertainty of the IS flux.
Journal ArticleDOI
Neutron monitors and muon detectors for solar modulation studies: 2. ϕ time series
TL;DR: In this paper, the authors established a correspondence between the uncertainties on ground-based detectors count rates and the parameter ϕ (modulation level in the force-field approximation) reconstructed from these count rates.
Journal ArticleDOI
Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer
M. Aguilar,L. Ali Cavasonza,G. Ambrosi,Luísa Arruda,N. Attig,F. Barao,L. Barrin,A. Bartoloni,S. Başeğmez-du Pree,Roberto Battiston,U. Becker,M. Behlmann,B. Beischer,J. Berdugo,B. Bertucci,Veronica Bindi,W. De Boer,K. Bollweg,B. Borgia,Matteo Boschini,M. Bourquin,E F Bueno,J. D. Burger,W. J. Burger,S. Burmeister,X. D. Cai,M. Capell,J. Casaus,G. Castellini,F. Cervelli,Yung Huang Chang,Guo-Ming Chen,H. S. Chen,Y. Chen,Lin Cheng,H. Y. Chou,S. Chouridou,V. Choutko,C. H. Chung,C. Clark,G. Coignet,C. Consolandi,Andrea Contin,Claudio Corti,Z. Cui,K. Dadzie,Yaomin Dai,C. Delgado,S. Della Torre,M. B. Demirköz,Laurent Derome,S. Di Falco,V. Di Felice,Carlos Díaz,F. Dimiccoli,P. von Doetinchem,F. Dong,F. Donnini,M. Duranti,A. Egorov,A. Eline,Jonathan L. Feng,E. Fiandrini,P. H. Fisher,V. Formato,C. Freeman,Yu. Galaktionov,C. Gámez,R. J. García-López,Corrado Gargiulo,Henning Gast,I. Gebauer,Massimo Gervasi,F. Giovacchini,D M Gómez-Coral,J. Gong,Corinne Goy,Varlen Grabski,D. Grandi,M. Graziani,K. H. Guo,Sadakazu Haino,K. C. Han,R. K. Hashmani,Z. H. He,Bernd Heber,Timothy H. Hsieh,Jun Hu,Zhiqi Huang,M. Incagli,W. Y. Jang,Yi Jia,H. Jinchi,K. Kanishev,B. Khiali,G. N. Kim,T. Kirn,M. Konyushikhin,O. Kounina,Andrei Kounine,V. Koutsenko,A. Kuhlman,A. Kulemzin,G. La Vacca,Elisa Laudi,G. Laurenti,Ignazio Lazzizzera,A. Lebedev,H. T. Lee,S. C. Lee,J. Q. Li,M. Li,Qiang Li,S. Li,T. X. Li,Z. H. Li,C. Light,Chia-Hui Lin,Thomas Lippert,Z Liu,S. Q. Lu,Ying Lu,K. Luebelsmeyer,J. Z. Luo,S. S. Lyu,F. Machate,C. Mañá,Julio C. Marín,J. Marquardt,T. Martin,G. Martinez,N. Masi,David Maurin,Arturo Alejandro Menchaca-Rocha,Q. Meng,D. C. Mo,M. Molero,P. Mott,L Mussolin,J. Q. Ni,N. Nikonov,F. Nozzoli,A.I. Oliva,M. Orcinha,M. Palermo,F. Palmonari,M. Paniccia,A. Pashnin,M. Pauluzzi,S. Pensotti,H. D. Phan,R Piandani,V. Plyaskin,Stepan Poluianov,X. M. Qi,X. Qin,Z. Y. Qu,L. Quadrani,Pier-Giorgio Rancoita,D. Rapin,A. Reina Conde,S. Rosier-Lees,A. Rozhkov,D. Rozza,Roald Z. Sagdeev,S. Schael,S. M. Schmidt,A. Schulz von Dratzig,G. Schwering,Eun-Suk Seo,B. S. Shan,J. Y. Shi,T. Siedenburg,C. Solano,R. Sonnabend,J. W. Song,Qie Sun,Zhen Sun,Mauro Tacconi,X. W. Tang,Zhixiang Tang,J Tian,Samuel C.C. Ting,S. M. Ting,Nicola Tomassetti,J. J. Torsti,C. Tüysüz,T. Urban,Ilya Usoskin,V Vagelli,Rami Vainio,E. Valente,Eino Valtonen,M. Vazquez Acosta,M. Vecchi,Mayda Velasco,J. P. Vialle,C. Wallmann,Liqiu Wang,Naihua Wang,Q. L. Wang,S Wang,Xiaoqun Wang,Zhao Wang,J Wei,Z. L. Weng,H. Wu,R. Q. Xiong,W. Xu,Q. Yan,Yuh-Shyong Yang,H. Yi,Y. J. Yu,Z. Q. Yu,Mario Zannoni,Chuanguo Zhang,Fan Zhang,Fajun Zhang,J. H. Zhang,Zhihua Zhang,F. Zhao,Z. M. Zheng,H. L. Zhuang,Valery Zhukov,Antonino Zichichi,N. Zimmermann,Paolo Zuccon +226 more
TL;DR: The observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.65 GV shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary Cosmic rays.
Journal ArticleDOI
Very high energy gamma-ray observations of the galaxy clusters Abell 496 and Abell 85 with HESS
Felix Aharonian,Felix Aharonian,A. G. Akhperjanian,Gisela Anton,U. Barres de Almeida,A. R. Bazer-Bachi,Yvonne Becherini,B. Behera,Konrad Bernlöhr,Konrad Bernlöhr,Catherine Boisson,A. Bochow,V. Borrel,Ilana M. Braun,E. Brion,J. Brucker,Pierre Brun,Rolf Bühler,Tomasz Bulik,I. Büsching,Timothé Boutelier,P. M. Chadwick,A. Charbonnier,R. C. G. Chaves,A. Cheesebrough,L.-M. Chounet,A. C. Clapson,G. Coignet,M. Dalton,M. K. Daniel,B. Degrange,Christoph Deil,Hugh Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,F. Dubois,Guillaume Dubus,J. Dyks,Michal Dyrda,Kathrin Egberts,Dimitrios Emmanoulopoulos,P. Espigat,Christian Farnier,F. Feinstein,A. Fiasson,A. Förster,G. Fontaine,M. Füßling,Stefano Gabici,Y. A. Gallant,L. Gérard,B. Giebels,J. F. Glicenstein,B. Glück,P. Goret,D. Hauser,M. Hauser,S. Heinz,G. Heinzelmann,Gilles Henri,G. Hermann,Jim Hinton,A. Hoffmann,Werner Hofmann,M. Holleran,S. Hoppe,Dieter Horns,A. Jacholkowska,O. C. de Jager,I. Jung,K. Katarzyński,U. F. Katz,Sarah Kaufmann,Eckhard Kendziorra,M. Kerschhaggl,D. Khangulyan,B. Khélifi,D. Keogh,Nu. Komin,Karl Kosack,G. Lamanna,J.-P. Lenain,Thomas Lohse,V. Marandon,J. M. Martin,Olivier Martineau-Huynh,Alexandre Marcowith,David Maurin,T. J. L. McComb,M. C. Medina,R. Moderski,Emmanuel Moulin,M. Naumann-Godo,M. de Naurois,D. Nedbal,D. Nekrassov,Jacek Niemiec,S. J. Nolan,Stefan Ohm,J-F. Olive,E. de Oña Wilhelmi,E. de Oña Wilhelmi,K. J. Orford,Michał Ostrowski,M. Panter,M. Paz Arribas,G. Pedaletti,Guy Pelletier,P.-O. Petrucci,S. Pita,Gerd Pühlhofer,Michael Punch,Andreas Quirrenbach,B. C. Raubenheimer,Martin Raue,Martin Raue,S. M. Rayner,Matthieu Renaud,Frank M. Rieger,Frank M. Rieger,J. Ripken,L. Rob,S. Rosier-Lees,Gavin Rowell,B. Rudak,Cameron B Rulten,J. Ruppel,V. Sahakian,Andrea Santangelo,Reinhard Schlickeiser,F. M. Schöck,R. Schröder,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,A. Shalchi,J. L. Skilton,Helene Sol,D. Spangler,Łukasz Stawarz,R. Steenkamp,C. Stegmann,G. Superina,Anna Szostek,P. H. Tam,J.-P. Tavernet,Regis Terrier,O. Tibolla,O. Tibolla,C. van Eldik,G. Vasileiadis,Christo Venter,L. Venter,J. P. Vialle,P. Vincent,M. Vivier,Heinrich J. Völk,F. Volpe,F. Volpe,F. Volpe,Stefan Wagner,Martin Ward,A. A. Zdziarski,A. Zech +164 more
TL;DR: In this article, the gamma-ray flux at energies E>570 GeV and E>460 GeV for Abell 496 and Abell 85 was studied in the very high energy (VHE, E > 100 GeV) band to investigate VHE cosmic rays.
Journal ArticleDOI
Revisiting the Westerlund 2 Field with the H.E.S.S. Telescope Array
A. Abramowski,Fabio Acero,Felix Aharonian,A. G. Akhperjanian,Gisela Anton,Anna Barnacka,U. Barres de Almeida,A. R. Bazer-Bachi,Yvonne Becherini,J. K. Becker,B. Behera,Konrad Bernlöhr,A. Bochow,C. Boisson,J. Bolmont,P. Bordas,V. Borrel,J. Brucker,Francois Brun,Pierre Brun,T. Bulik,I. Büsching,Timothé Boutelier,Sabrina Casanova,Matteo Cerruti,P. M. Chadwick,A. Charbonnier,R. C. G. Chaves,A. Cheesebrough,Jan Conrad,L.-M. Chounet,A. C. Clapson,G. Coignet,M. Dalton,M. K. Daniel,Isak Delberth Davids,B. Degrange,Christoph Deil,Hugh Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,Franky Dubois,Guillaume Dubus,J. Dyks,Michal Dyrda,K. Egberts,Peter Eger,P. Espigat,L. Fallon,C. Farnier,S. J. Fegan,F. Feinstein,M. V. Fernandes,A. Fiasson,A. Förster,Gerard Fontaine,M. Füßling,Stefano Gabici,Y. A. Gallant,L. Gérard,D. Gerbig,B. Giebels,J. F. Glicenstein,B. Glück,P. Goret,D. Göring,J. D. Hague,Daniel Hampf,M. Hauser,S. Heinz,G. Heinzelmann,Gilles Henri,G. Hermann,Jim Hinton,A. Hoffmann,Werner Hofmann,Petter Hofverberg,M. Holleran,S. Hoppe,Dieter Horns,A. Jacholkowska,O. C. de Jager,C. Jahn,I. Jung,Krzysztof Katarzynski,U. Katz,Sarah Kaufmann,M. Kerschhaggl,D. Khangulyan,B. Khélifi,D. Keogh,D. Klochkov,W. Kluźniak,T. Kneiske,Nu. Komin,K. Kosack,R. Kossakowski,G. Lamanna,J.-P. Lenain,Dirk Lennarz,Thomas Lohse,C.-C. Lu,V. Marandon,A. Marcowith,Julien Masbou,David Maurin,T. J. L. McComb,M. C. Medina,J. Mehault,R. Moderski,E. Moulin,M. Naumann-Godo,M. de Naurois,D. Nedbal,D. Nekrassov,N. Nguyen,B. Nicholas,Jacek Niemiec,S. J. Nolan,Stefan Ohm,J-F. Olive,E. de Oña Wilhelmi,B. Opitz,K. J. Orford,Michal Ostrowski,M. Panter,M. Paz Arribas,G. Pedaletti,G. Pelletier,P.-O. Petrucci,S. Pita,G. Pühlhofer,Michael Punch,Andreas Quirrenbach,Martin Raue,S. M. Rayner,A. Reimer,Olaf Reimer,M. Renaud,R. de los Reyes,Frank M. Rieger,Joachim Ripken,L. Rob,S. Rosier-Lees,Gavin Rowell,B. Rudak,C. B. Rulten,J. Ruppel,Felix Ryde,V. Sahakian,Andrea Santangelo,Reinhard Schlickeiser,F. M. Schöck,A. Schönwald,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,A. Shalchi,I. Sushch,M. Sikora,J. L. Skilton,Helene Sol,G. Spengler,Łukasz Stawarz,Riaan Steenkamp,Christian Stegmann,F. Stinzing,Anna Szostek,P. H. Tam,J.-P. Tavernet,Regis Terrier,O. Tibolla,M. Tluczykont,K. Valerius,C. van Eldik,G. Vasileiadis,Christo Venter,J. P. Vialle,Aion Viana,Pascal Vincent,M. Vivier,Heinrich J. Völk,Francesca Volpe,Serguei Vorobiov,Stefan Wagner,Martin Ward,A. A. Zdziarski,A. Zech,H.-S. Zechlin,Y. Fukui,Naoko Furukawa,Akio Ohama,Hidetoshi Sano,Joanne Dawson,Akiko Kawamura +195 more
TL;DR: In this paper, a new very high-energy (VHE; E>100 GeV) γ-ray source, HESSJ1026-582, was discovered with a statistical significance of 7σ.