P
Pascal Vincent
Researcher at Claude Bernard University Lyon 1
Publications - 179
Citations - 10261
Pascal Vincent is an academic researcher from Claude Bernard University Lyon 1. The author has contributed to research in topics: High Energy Stereoscopic System & Pulsar. The author has an hindex of 50, co-authored 179 publications receiving 9465 citations. Previous affiliations of Pascal Vincent include University of Cambridge & Centre national de la recherche scientifique.
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Journal ArticleDOI
The H.E.S.S. Survey of the Inner Galaxy in Very High Energy Gamma Rays
Felix Aharonian,A. G. Akhperjanian,A. R. Bazer-Bachi,M. Beilicke,Wystan Benbow,David Berge,Konrad Bernlöhr,Konrad Bernlöhr,Catherine Boisson,O. Bolz,V. Borrel,Ilana M. Braun,F. Breitling,A. M. Brown,P. M. Chadwick,L.-M. Chounet,R. Cornils,Luigi Costamante,Luigi Costamante,B. Degrange,Hugh Dickinson,A. Djannati-Ataï,L. O'c. Drury,Guillaume Dubus,Dimitrios Emmanoulopoulos,P. Espigat,F. Feinstein,G. Fontaine,Y. Fuchs,Seb. Funk,Y. A. Gallant,B. Giebels,Stefan Gillessen,J. F. Glicenstein,P. Goret,C. Hadjichristidis,M. Hauser,G. Heinzelmann,Gilles Henri,G. Hermann,Jim Hinton,Werner Hofmann,M. Holleran,Dieter Horns,A. Jacholkowska,O. C. de Jager,B. Khélifi,Nu. Komin,A. Konopelko,A. Konopelko,I. J. Latham,R. Le Gallou,A. Lemière,M. Lemoine-Goumard,N. Leroy,Thomas Lohse,Jean Michel Martin,Olivier Martineau-Huynh,A. Marcowith,Conor Masterson,Conor Masterson,T. J. L. McComb,M. de Naurois,S. J. Nolan,A. Noutsos,K. J. Orford,J. L. Osborne,M. Ouchrif,M. Panter,Guy Pelletier,S. Pita,Gerd Pühlhofer,Michael Punch,B. C. Raubenheimer,Martin Raue,J. Raux,S. M. Rayner,A. Reimer,Olaf Reimer,J. Ripken,L. Rob,L. Rolland,Gavin Rowell,V. Sahakian,L. Saugé,S. Schlenker,Reinhard Schlickeiser,C. Schuster,Ullrich Schwanke,M. Siewert,Helene Sol,D. Spangler,R. Steenkamp,C. Stegmann,J.-P. Tavernet,R. Terrier,C. G. Théoret,M. Tluczykont,M. Tluczykont,G. Vasileiadis,Christo Venter,Pascal Vincent,Heinrich J. Völk,Stefan Wagner +103 more
TL;DR: The distribution in Galactic latitude of the detected sources appears to be consistent with a scale height in the Galactic disk for the parent population smaller than 100 pc, consistent with expectations for supernova remnants and/or pulsar wind nebulae.
Journal ArticleDOI
Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S.
Felix Aharonian,A. G. Akhperjanian,Gisela Anton,U. Barres de Almeida,A. R. Bazer-Bachi,Yvonne Becherini,B. Behera,Konrad Bernlöhr,A. Bochow,C. Boisson,J. Bolmont,V. Borrel,J. Brucker,Francois Brun,Pierre Brun,Rolf Bühler,T. Bulik,I. Büsching,Timothé Boutelier,P. M. Chadwick,A. Charbonnier,R. C. G. Chaves,A. Cheesebrough,L.-M. Chounet,G. Coignet,M. Dalton,M. K. Daniel,I. D. Davids,I. D. Davids,B. Degrange,Christoph Deil,Hugh Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,Franky Dubois,Guillaume Dubus,J. Dyks,M. Dyrda,Kathrin Egberts,Dimitrios Emmanoulopoulos,P. Espigat,Christian Farnier,F. Feinstein,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,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,C. Jahn,I. Jung,K. Katarzyński,Uli Katz,Sarah Kaufmann,Eckhard Kendziorra,M. Kerschhaggl,D. Khangulyan,B. Khélifi,D. Keogh,W. Klu'Zniak,T. Kneiske,Nu. Komin,Karl Kosack,R. Kossakowski,G. Lamanna,J.-P. Lenain,Thomas Lohse,V. Marandon,J. M. Martin,Olivier Martineau-Huynh,Alexandre Marcowith,Julien Masbou,David Maurin,T. J. L. McComb,M. C. Medina,R. Moderski,Emmanuel Moulin,M. Naumann-Godo,M. de Naurois,D. Nedbal,D. Nekrassov,B. Nicholas,Jacek Niemiec,S. J. Nolan,Stefan Ohm,J-F. Olive,E. de O˜na,K. J. Orford,Michał Ostrowski,M. Panter,M. Paz Arribas,G. Pedaletti,G. Pelletier,P.-O. Petrucci,S. Pita,Gerd Pühlhofer,Michael Punch,Andreas Quirrenbach,B. C. Raubenheimer,Martin Raue,S. M. Rayner,Olaf Reimer,Matthieu Renaud,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. Sch¨ock,R. Schröder,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,A. Shalchi,J. L. Skilton,Helene Sol,D. Spangler,L. Stawarz,R. Steenkamp,C. Stegmann,F. Stinzing,G. Superina,Anna Szostek,P. H. Tam,J.-P. Tavernet,Regis Terrier,O. Tibolla,M. Tluczykont,C. van Eldik,G. Vasileiadis,Christo Venter,L. Venter,J. P. Vialle,Pascal Vincent,M. Vivier,Heinrich J. Völk,Francesca Volpe,Stefan Wagner,Martin Ward,A. A. Zdziarski,A. Zech +168 more
TL;DR: In this article, the authors present a measurement of the cosmic-ray electron spectrum with H.E.S. starting at 340 GeV and show no indication of a structure in the electron spectrum, but rather a power-law spectrum with spectral index of 3.0 +- 0.1 (stat.) + − 0.3 (syst.) which steepens at about 1 TeV.
Journal ArticleDOI
Search for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S
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,Catherine Boisson,J. Bolmont,P. Bordas,V. Borrel,J. Brucker,Francois Brun,P. Brun,Tomasz Bulik,I. Büsching,Svenja Carrigan,Sabrina Casanova,Matteo Cerruti,P. M. Chadwick,A. Charbonnier,R. C. G. Chaves,A. Cheesebrough,L.-M. Chounet,A. C. Clapson,G. Coignet,J. Conrad,M. Dalton,M. K. Daniel,I. D. Davids,B. Degrange,Christoph Deil,H. J. Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,Franky Dubois,Guillaume Dubus,J. Dyks,M. Dyrda,K. Egberts,P. Eger,P. Espigat,L. Fallon,Christian Farnier,S. Fegan,F. Feinstein,M. V. Fernandes,A. Fiasson,G. Fontaine,A. Förster,M. Füßling,Y. A. Gallant,H. Gast,L. Gérard,D. Gerbig,B. Giebels,J. F. Glicenstein,B. Glück,P. Goret,D. Göring,J. D. Hague,D. Hampf,M. Hauser,S. Heinz,G. Heinzelmann,Gilles Henri,G. Hermann,Jim Hinton,A. Hoffmann,Werner Hofmann,P. Hofverberg,Dieter Horns,A. Jacholkowska,O. C. de Jager,C. Jahn,Marek Jamrozy,I. Jung,M. A. Kastendieck,Krzysztof Katarzynski,U. F. Katz,S. Kaufmann,D. Keogh,M. Kerschhaggl,D. Khangulyan,B. Khélifi,D. Klochkov,W. Kluźniak,T. Kneiske,Nu. Komin,K. Kosack,R. Kossakowski,H. Laffon,G. Lamanna,Dirk Lennarz,Thomas Lohse,A. Lopatin,Chia-Chun Lu,V. Marandon,A. Marcowith,Julien Masbou,David Maurin,N. Maxted,T. J. L. McComb,M. C. Medina,J. Mehault,R. Moderski,Emmanuel Moulin,C. L. Naumann,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,M. 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,M. Sikora,J. L. Skilton,Helene Sol,G. Spengler,Ł. Stawarz,Riaan Steenkamp,Christian Stegmann,F. Stinzing,I. Sushch,Anna Szostek,J.-P. Tavernet,Regis Terrier,O. Tibolla,M. Tluczykont,K. Valerius,C. van Eldik,G. Vasileiadis,Christo Venter,J. P. Vialle,A. Viana,Pascal Vincent,M. Vivier,Heinrich J. Völk,Francesca Volpe,Serguei Vorobiov,M. J. Vorster,Stefan Wagner,Martin Ward,Alicja Wierzcholska,Anna Zajczyk,A. A. Zdziarski,A. Zech,H.-S. Zechlin +193 more
TL;DR: Limits are derived on the velocity-weighted annihilation cross section (σv) as a function of the DM particle mass that are among the best reported so far for this energy range and in particular differ only little between the chosen density profile parametrizations.
Journal ArticleDOI
A single nitrogen-vacancy defect coupled to a nanomechanical oscillator
O. Arcizet,Vincent Jacques,Alessandro Siria,Philippe Poncharal,Pascal Vincent,Signe Seidelin +5 more
TL;DR: In this paper, a single quantum system comprising a nitrogen-vacancy in diamond is coupled to a nanowire cantilever and magnetic fields are used to couple the spin and the oscillator enabling read-out of the nanometre-scale motion.
Journal ArticleDOI
Search for Photon-Linelike Signatures from Dark Matter Annihilations with H.E.S.S.
A. Abramowski,Fabio Acero,Felix Aharonian,Felix Aharonian,Felix Aharonian,A. G. Akhperjanian,A. G. Akhperjanian,Gisela Anton,S. Balenderan,A. Balzer,A. Barnacka,Yvonne Becherini,J. Becker Tjus,Konrad Bernlöhr,Konrad Bernlöhr,E. Birsin,Jonathan Biteau,A. Bochow,Catherine Boisson,J. Bolmont,P. Bordas,J. Brucker,Francois Brun,Pierre Brun,Tomasz Bulik,Svenja Carrigan,Sabrina Casanova,Matteo Cerruti,P. M. Chadwick,R. C. G. Chaves,A. Cheesebrough,S. Colafrancesco,G. Cologna,Jan Conrad,C. Couturier,M. Dalton,M. K. Daniel,I. D. Davids,B. Degrange,Christoph Deil,P. Dewilt,Hugh Dickinson,A. Djannati-Ataï,W. Domainko,L. O'c. Drury,Guillaume Dubus,K. Dutson,J. Dyks,Michal Dyrda,Kathrin Egberts,Peter Eger,P. Espigat,L. Fallon,C. Farnier,S. J. Fegan,F. Feinstein,M. V. Fernandes,D. Fernandez,A. Fiasson,G. Fontaine,A. Förster,M. Füßling,M. Gajdus,Y. A. Gallant,T. Garrigoux,Henning Gast,B. Giebels,J. F. Glicenstein,B. Glück,D. Göring,M. H. Grondin,M. H. Grondin,S. Häffner,J. D. Hague,Joachim Hahn,Daniel Hampf,J. Harris,S. Heinz,G. Heinzelmann,Gilles Henri,G. Hermann,Andreas Hillert,Jim Hinton,Werner Hofmann,Petter Hofverberg,M. Holler,Dieter Horns,A. Jacholkowska,C. Jahn,Marek Jamrozy,I. Jung,M. A. Kastendieck,Krzysztof Katarzynski,U. F. Katz,S. Kaufmann,B. Khélifi,S. Klepser,Dmitry Klochkov,W. Kluźniak,T. Kneiske,Nu. Komin,K. Kosack,R. Kossakowski,F. Krayzel,P.P. Krüger,P.P. Krüger,H. Laffon,G. Lamanna,Julien Lefaucheur,M. Lemoine-Goumard,J.-P. Lenain,Dirk Lennarz,Thomas Lohse,A. Lopatin,Chia-Chun Lu,Vincent Marandon,A. Marcowith,Julien Masbou,Gilles Maurin,N. Maxted,M. Mayer,T. J. L. McComb,M. C. Medina,J. Mehault,U. Menzler,R. Moderski,M. Mohamed,Emmanuel Moulin,C. L. Naumann,M. Naumann-Godo,M. de Naurois,D. Nedbal,D. Nekrassov,N. Nguyen,Jacek Niemiec,S. J. Nolan,Stefan Ohm,Stefan Ohm,E. de Oña Wilhelmi,B. Opitz,Michał Ostrowski,I. Oya,M. Panter,R. D. Parsons,M. Paz Arribas,N. W. Pekeur,G. Pelletier,J. Perez,P.-O. Petrucci,B. Peyaud,S. Pita,G. Pühlhofer,Michael Punch,Andreas Quirrenbach,Martin Raue,A. Reimer,Olaf Reimer,M. Renaud,R. de los Reyes,Frank M. Rieger,Joachim Ripken,L. Rob,S. Rosier-Lees,Gavin Rowell,B. Rudak,Cameron B Rulten,V. Sahakian,Daniel Sánchez,Andrea Santangelo,Reinhard Schlickeiser,André Schulz,Ullrich Schwanke,S. Schwarzburg,S. Schwemmer,F. Sheidaei,J. L. Skilton,Helene Sol,G. Spengler,Łukasz Stawarz,R. Steenkamp,C. Stegmann,F. Stinzing,K. Stycz,Iurii Sushch,Anna Szostek,J.-P. Tavernet,Regis Terrier,M. Tluczykont,C. Trichard,K. Valerius,C. van Eldik,G. Vasileiadis,Christo Venter,Aion Viana,Pascal Vincent,Heinrich J. Völk,Francesca Volpe,Serguei Vorobiov,M. J. Vorster,Stefan Wagner,Martin Ward,R. White,Alicja Wierzcholska,Denis Wouters,Michael Zacharias,Anna Zajczyk,A. A. Zdziarski,A. Zech,H.-S. Zechlin +208 more
TL;DR: In this paper, the authors obtained upper limits on line-like emission in the energy range between ~500 GeV and ~25 TeV for the central part of the Milky Way halo and for extragalactic observations, complementing recent limits obtained with the Fermi-LAT instrument at lower energies.