F
F. Mayet
Researcher at University of Grenoble
Publications - 237
Citations - 8731
F. Mayet is an academic researcher from University of Grenoble. The author has contributed to research in topics: Dark matter & Galaxy cluster. The author has an hindex of 44, co-authored 230 publications receiving 7979 citations. Previous affiliations of F. Mayet include Centre national de la recherche scientifique & Chinese Academy of Sciences.
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Journal ArticleDOI
GATE : a simulation toolkit for PET and SPECT
Sébastien Jan,Giovanni Santin,D. Strul,D. Strul,Steven Staelens,Karine Assié,D. Autret,Stéphane Avner,Remi Barbier,Manuel Bardiès,Peter M. Bloomfield,David Brasse,Vincent Breton,P. Bruyndonckx,Irène Buvat,Arion F. Chatziioannou,Yong Choi,Y. H. Chung,Claude Comtat,D. Donnarieix,Ludovic Ferrer,Stephen J. Glick,C. J. Groiselle,David Guez,P. F. Honore,S. Kerhoas-Cavata,Assen S. Kirov,V. Kohli,Michel Koole,M. Krieguer,D.J. van der Laan,F. Lamare,G. Largeron,Carole Lartizien,D. Lazaro,Marnix C. Maas,Lydia Maigne,F. Mayet,F. Melot,C. Merheb,E. Pennacchio,J. Perez,Uwe Pietrzyk,F. R. Rannou,F. R. Rannou,M. Rey,Dennis R. Schaart,Charles Schmidtlein,Luc Simon,Luc Simon,Tae Yong Song,J. M. Vieira,Dimitris Visvikis,R. T. Van de Walle,E. Wieers,Christian Morel +55 more
TL;DR: A detailed description of the design and development of GATE is given by the OpenGATE collaboration, whose continuing objective is to improve, document and validate GATE by simulating commercially available imaging systems for PET and SPECT.
Journal ArticleDOI
The Alpha Magnetic Spectrometer (AMS)on the International Space Station : Part I - results from the test flight on the space shuttle
M. Aguilar,J. Alcaraz,Behcet Alpat,G. Ambrosi,G. Ambrosi,H. Anderhub,L. Ao,A. Arefiev,Philipp Azzarello,E. Babucci,L. Baldini,L. Baldini,M. Basile,D. Barancourt,F. Barao,G. Barbier,G.P. Barreira,Roberto Battiston,R. Becker,U. Becker,L. Bellagamba,P. Bene,J. Berdugo,P. Berges,B. Bertucci,Adrian Biland,S. Bizzaglia,S. Blasko,G. Boella,M. J. Boschini,M. Bourquin,L. Brocco,G. Bruni,M. Buenerd,J. D. Burger,W. J. Burger,X. D. Cai,C. Camps,P. Cannarsa,M. Capell,D. Casadei,J. Casaus,G. Castellini,Claudia Cecchi,Y. H. Chang,H.F. Chen,H. S. Chen,Z.G. Chen,N.A. Chernoplekov,Tzihong Chiueh,Kyung-Suk Cho,M.J. Choi,Y.Y. Choi,Y.L. Chuang,Federico Cindolo,V. Commichau,A. Contin,E. Cortina-Gil,Markus Cristinziani,J. P. Da Cunha,T. S. Dai,C. Delgado,J.D. Deus,N. Dinu,L. Djambazov,I. D'Antone,Z.R. Dong,P. Emonet,J. Engelberg,F. J. Eppling,T. Eronen,G. Esposito,P. Extermann,J. Favier,E. Fiandrini,Peter H. Fisher,G. Fluegge,N. Fouque,Yu. Galaktionov,Yu. Galaktionov,Massimo Gervasi,P. Giusti,D. Grandi,O. Grimm,W.Q. Gu,K. Hangarter,A. Hasan,V. Hermel,H. Hofer,M. A. Huang,W. Hungerford,Maria Ionica,R. Ionica,M. Jongmanns,K. Karlamaa,Waclaw Karpinski,G. Kenney,Jose Maria Kenny,D.H. Kim,Gui Nyun Kim,K.S. Kim,M.Y. Kim,A. Klimentov,A. Klimentov,R. Kossakowski,V. Koutsenko,V. Koutsenko,M. Kraber,G. Laborie,Timo Laitinen,G. Lamanna,E. Lanciotti,G. Laurenti,A. Lebedev,C. Lechanoine-Leluc,M.W. Lee,S.C. Lee,Giuseppe Levi,P. Levtchenko,C.L. Liu,Hengchang Liu,I. Lopes,G. Lu,Y.S. Lu,K. Luebelsmeyer,D. Luckey,Werner Lustermann,C. Maña,Anselmo Margotti,F. Mayet,R. R. McNeil,B. Meillon,Mauro Menichelli,A. Mihul,A. Mourao,Ari Mujunen,F. Palmonari,A. Papi,H.B. Park,W.H. Park,M. Pauluzzi,Felicitas Pauss,E. Perrin,A. Pesci,A. Pevsner,M. Pimenta,V. Plyaskin,V. Pojidaev,M. Pohl,V. Postolache,N. Produit,P. G. Rancoita,D. Rapin,Frank Raupach,D. Ren,Zhuoxiang Ren,M. Ribordy,J.P. Richeux,E. Riihonen,J. Ritakari,S. Ro,U. Roser,C. Rossin,Roald Z. Sagdeev,D. Santos,G. Sartorelli,C. Sbarra,Stefan Schael,A. Schultz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,Jungwook Shin,V. Shoutko,E. Shoumilov,R. Siedling,Dong-Chul Son,Tao Song,M. Steuer,G.S. Sun,H. Suter,X.W. Tang,S.C.C. Ting,Samuel C.C. Ting,Merja Tornikoski,J. J. Torsti,J. Trümper,J. Ulbricht,S. Urpo,Eino Valtonen,J. Vandenhirtz,F. Velcea,E. P. Velikhov,B. Verlaat,I. Vetlitsky,F. Vezzu,J. P. Vialle,G. Viertel,D. Vité,H. von Gunten,S. Waldmeier Wicki,W. Wallraff,B.C. Wang,Jian Wang,Yun Wang,K. Wiik,Ciaran Williams,S. X. Wu,S. X. Wu,P.C. Xia,J.L. Yan,L.G. Yan,Changgen Yang,J. Yang,Mao-Zhi Yang,S.W. Ye,P. Yeh,Zhenghao Xu,Hao Zhang,Zhidong Zhang,Dawei Zhao,Guohuai Zhu,W.Z. Zhu,H. L. Zhuang,Antonino Zichichi,B. Zimmermann,Paolo Zuccon +226 more
TL;DR: The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km as discussed by the authors.
Journal ArticleDOI
Cosmic-ray positron fraction measurement from 1 to 30 GeV with AMS-01
M. Aguilar,J. Alcaraz,J.V. Allaby,Behcet Alpat,Giovanni Ambrosi,H. Anderhub,L. Ao,A. Arefiev,P. Azzarello,L. Baldini,M. Basile,D. Barancourt,Fernando Barão,G. Barbier,G.P. Barreira,Roberto Battiston,R. Becker,U. Becker,L. Bellagamba,P. Bene,J. Berdugo,P. Berges,B. Bertucci,Adrian Biland,S. Blasko,G. Boella,M. J. Boschini,M. Bourquin,L. Brocco,G. Bruni,M. Buénerd,J. D. Burger,W. J. Burger,X. D. Cai,C. Camps,P. Cannarsa,M. Capell,F. Cardano,D. Casadei,J. Casaus,G. Castellini,G. Castellini,Yuan-Hann Chang,H.F. Chen,H. S. Chen,Z.G. Chen,N.A. Chernoplekov,Tzihong Chiueh,Kyung-Suk Cho,M.J. Choi,Y.Y. Choi,Federico Cindolo,V. Commichau,A. Contin,E. Cortina-Gil,Markus Cristinziani,T. S. Dai,C. Delgado,S. Difalco,L. Djambazov,I. D'Antone,Z.R. Dong,P. Emonet,J. Engelberg,F. J. Eppling,T. Eronen,G. Esposito,P. Extermann,J. Favier,E. Fiandrini,Peter H. Fisher,Günter Flügge,N. Fouque,Yu. Galaktionov,Henning Gast,Massimo Gervasi,P. Giusti,D. Grandi,O. Grimm,W.Q. Gu,K. Hangarter,A. Hasan,V. Hermel,H. Hofer,W. Hungerford,M. Jongmanns,K. Karlamaa,Waclaw Karpinski,G. Kenney,Daijin Kim,G. N. Kim,K.S. Kim,M.Y. Kim,A. Klimentov,R. Kossakowski,Andrei Kounine,V. Koutsenko,M. Kraeber,G. Laborie,Timo Laitinen,G. Lamanna,E. Lanciotti,G. Laurenti,A. Lebedev,C. Lechanoine-Leluc,M.W. Lee,Shih-Chang Lee,Giuseppe Levi,C.L. Liu,Hengchang Liu,G. Lu,Y.S. Lu,K. Lübelsmeyer,D. Luckey,Werner Lustermann,C. Maña,Anselmo Margotti,F. Mayet,R. R. McNeil,B. Meillon,Mauro Menichelli,A. Mihul,Ari Mujunen,A. Oliva,J. Olzem,F. Palmonari,H. Park,W.H. Park,M. Pauluzzi,Felicitas Pauss,E. Perrin,A. Pesci,A. Pevsner,Fabrizio Giulio Luca Pilo,M. Pimenta,V. Plyaskin,V. Pojidaev,M. Pohl,N. Produit,P. G. Rancoita,D. Rapin,Frank Raupach,D. Ren,Z. L. Ren,M. Ribordy,J.P. Richeux,E. Riihonen,Jouko Ritakari,S. R. Ro,U. Roeser,C. Rossin,Roald Z. Sagdeev,D. Santos,G. Sartorelli,C. Sbarra,S. Schael,A. Schultz von Dratzig,G. Schwering,Eun-Suk Seo,Jungwook Shin,E. Shoumilov,V. Shoutko,T. Siedenburg,R. Siedling,Dong-Chul Son,Tao Song,F. Spinella,M. Steuer,G.S. Sun,H. Suter,X.W. Tang,Samuel C.C. Ting,Samuel C.C. Ting,Merja Tornikoski,J. J. Torsti,J. Trümper,J. Ulbricht,S. Urpo,Eino Valtonen,J. Vandenhirtz,E. P. Velikhov,B. Verlaat,I. Vetlitsky,F. Vezzu,J. P. Vialle,G. Viertel,D. Vité,H. von Gunten,S. Waldmeier Wicki,W. Wallraff,B.C. Wang,Jing Wang,K. Wiik,Ciaran Williams,S. X. Wu,S. X. Wu,P.C. Xia,S. Xu,J.L. Yan,L.G. Yan,Changgen Yang,J. Yang,Ming Yang,S.W. Ye,Zhenghao Xu,Hao Zhang,Zhidong Zhang,Dawei Zhao,You Zhou,Guohuai Zhu,W.Z. Zhu,H. L. Zhuang,Antonino Zichichi,B. Zimmermann,Paolo Zuccon +214 more
TL;DR: In this article, a measurement of the cosmic ray positron fraction in the energy range of 1 −30 GeV was presented, based on data taken by the AMS-01 experiment during its 10-day Space Shuttle flight in June 1998.
Journal ArticleDOI
Leptons in near earth orbit
J. Alcaraz,Behcet Alpat,Giovanni Ambrosi,H. Anderhub,L. Ao,A. Arefiev,P. Azzarello,E. Babucci,L. Baldini,M. Basile,D. Barancourt,F. Barao,G. Barbier,G.P. Barreira,Roberto Battiston,R. Becker,U. Becker,L. Bellagamba,P. Bene,J. Berdugo,P. Berges,B. Bertucci,Adrian Biland,S. Bizzaglia,S. Blasko,G. Boella,M. J. Boschini,M. Bourquin,L. Brocco,Giovanna Bruni,M. Buenerd,J. D. Burger,W. J. Burger,X. D. Cai,C. Camps,P. Cannarsa,M. Capell,Diego Casadei,J. Casaus,G. Castellini,Claudia Cecchi,Y. H. Chang,H. F. Chen,H. S. Chen,Z.G. Chen,N.A. Chernoplekov,Tzihong Chiueh,Y.L. Chuang,Federico Cindolo,V. Commichau,A. Contin,P. Crespo,Markus Cristinziani,J. P. Da Cunha,T. S. Dai,J.D. Deus,N. Dinu,L. Djambazov,I. D'Antone,Z.R. Dong,P. Emonet,J. Engelberg,F. J. Eppling,T. Eronen,G. Esposito,P. Extermann,J. Favier,E. Fiandrini,Peter H. Fisher,G. Fluegge,N. Fouque,Yu. Galaktionov,Massimo Gervasi,P. Giusti,D. Grandi,O. Grimm,W.Q. Gu,K. Hangarter,A. Hasan,V. Hermel,H. Hofer,M. A. Huang,W. Hungerford,M. Ionica,R. Ionica,M. Jongmanns,K. Karlamaa,Waclaw Karpinski,G. Kenney,Jose Maria Kenny,W. Kim,A. Klimentov,R. Kossakowski,V. Koutsenko,M. Kraeber,G. Laborie,Timo Laitinen,G. Lamanna,G. Laurenti,A. Lebedev,S.C. Lee,Giuseppe Levi,P. Levtchenko,C.L. Liu,H. T. Liu,I. Lopes,G. Lu,Lu Yuzhang,K. Lübelsmeyer,D. Luckey,Werner Lustermann,C. Maña,Anselmo Margotti,F. Mayet,R. R. McNeil,B. Meillon,Mauro Menichelli,A. Mihul,A. Mourao,Ari Mujunen,F. Palmonari,A. Papi,Inkyu Park,M. Pauluzzi,Felicitas Pauss,E. Perrin,A. Pesci,A. Pevsner,M. Pimenta,V. Plyaskin,V. Pojidaev,V. Postolache,N. Produit,P. G. Rancoita,D. Rapin,Frank Raupach,D. Ren,Z. L. Ren,M. Ribordy,J.P. Richeux,E. Riihonen,J. Ritakari,U. Roeser,C. Roissin,Roald Z. Sagdeev,G. Sartorelli,A. Schultz von Dratzig,G. Schwering,G. Scolieri,Eun-Suk Seo,V. Shoutko,E. Shoumilov,R. Siedling,Dong-Chul Son,Tengfei Song,M. Steuer,G.S. Sun,H. Suter,Xiao-Dong Tang,Samuel C.C. Ting,S. M. Ting,Merja Tornikoski,J. J. Torsti,J. Trümper,J. Ulbricht,S. Urpo,Ilya Usoskin,Eino Valtonen,J. Vandenhirtz,F. Velcea,E. P. Velikhov,B. Verlaat,I. Vetlitsky,F. Vezzu,J. P. Vialle,G. Viertel,D. Vité,H. von Gunten,S. Waldmeier Wicki,W. Wallraff,B.C. Wang,Jing Wang,Yun Wang,K. Wiik,Ciaran Williams,S. X. Wu,S. X. Wu,P.C. Xia,J.L. Yan,L.G. Yan,Changgen Yang,Mao-Zhi Yang,S.W. Ye,P. Yeh,Z. Z. Xu,Hao Zhang,Zhenyu Zhang,Dawei Zhao,Guohuai Zhu,W.Z. Zhu,H.L. Zhuang,Antonino Zichichi,B. Zimmermann +202 more
TL;DR: The lepton kinetic energy ranges from 0.2 to 40 GeV for e − and from 3 GeV to 6 GeVs for e + were measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at altitudes near 380 km.
Journal ArticleDOI
Cosmological constraints from archeops
Alain Benoit,Peter A. R. Ade,Alexandre Amblard,R. Ansari,Éric Aubourg,S. Bargot,James G. Bartlett,J.-Ph. Bernard,R. S. Bhatia,Alain Blanchard,James J. Bock,A. Boscaleri,A. Boscaleri,François R. Bouchet,A. Bourrachot,Philippe Camus,F. Couchot,P. de Bernardis,Jacques Delabrouille,Francois-Xavier Désert,O. Doré,Marian Douspis,L. Dumoulin,X. Dupac,P. Filliatre,Pablo Fosalba,K. Ganga,Fred Gannaway,B. Gautier,M. Giard,Y. Giraud-Héraud,R. Gispert,L. Guglielmi,J.-Ch. Hamilton,Shaul Hanany,Sophie Henrot-Versille,J. Kaplan,Guilaine Lagache,J.-M. Lamarre,Andrew E. Lange,J. F. Macías-Pérez,K. Madet,Bruno Maffei,Ch. Magneville,Daniel P. Marrone,Silvia Masi,F. Mayet,Anthony Murphy,F. Naraghi,Federico Nati,Guillaume Patanchon,Guy Perrin,M. Piat,Nicolas Ponthieu,Simon Prunet,Jean-Loup Puget,C. Renault,C. Rosset,D. Santos,Alexei A. Starobinsky,I. Strukov,Rashmikant V. Sudiwala,Romain Teyssier,Romain Teyssier,M. Tristram,Carole Tucker,Jean-Charles Vanel,D. Vibert,E. Wakui,D. Yvon +69 more
TL;DR: In this paper, the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations were analyzed, and the spectral index n was measured to be 1.04 (+0.10, 0.12) when the optical depth to reionization, tau, is allowed to vary as a free parameter, and 0.96 (+ 0.03,0.04) when tau is fixed to zero, both in good agreement with inflation.