M
Marco Grassi
Researcher at Federal University of Paraná
Publications - 236
Citations - 5631
Marco Grassi is an academic researcher from Federal University of Paraná. The author has contributed to research in topics: CMOS & Detector. The author has an hindex of 31, co-authored 236 publications receiving 4805 citations. Previous affiliations of Marco Grassi include University of Delaware & University of Pavia.
Papers
More filters
Journal ArticleDOI
Search for the lepton flavour violating decay μ + → e + γ with the full dataset of the MEG experiment
A. M. Baldini,Yu Bao,E. Baracchini,C. Bemporad,F. Berg,F. Berg,Michele Biasotti,G. Boca,Michele Cascella,P. W. Cattaneo,G. Cavoto,Fabrizio Cei,C. Cerri,G. Chiarello,C. Chiri,A. Corvaglia,A. de Bari,M. De Gerone,Tadayoshi Doke,A. D’Onofrio,S. Dussoni,J. Egger,Yasunori Fujii,L. Galli,Flavio Gatti,Francesco Grancagnolo,Marco Grassi,A. Graziosi,D. N. Grigoriev,D. N. Grigoriev,D. N. Grigoriev,Tomiyoshi Haruyama,M. Hildebrandt,Z. Hodge,Z. Hodge,K. Ieki,F. Ignatov,F. Ignatov,T. Iwamoto,D. Kaneko,T. I. Kang,P.R. Kettle,B.I. Khazin,B.I. Khazin,N. V. Khomutov,A. S. Korenchenko,N. Kravchuk,G. M. A. Lim,A. Maki,Satoshi Mihara,W. R. Molzon,Toshinori Mori,Fabio Morsani,A. Mtchedilishvili,D. Mzavia,S. Nakaura,Roberto Di Nardo,Donato Nicolo,Hajime Nishiguchi,M. Nishimura,S. Ogawa,Wataru Ootani,S. Orito,M. Panareo,Angela Papa,Roberto Pazzi,A. Pepino,G. Piredda,G. Pizzigoni,A. Popov,A. Popov,F. Raffaelli,F. Renga,F. Renga,E. Ripiccini,Stefan Ritt,M. Rossella,G. Rutar,G. Rutar,Ryu Sawada,F. Sergiampietri,G. Signorelli,M. Simonetta,G. Tassielli,F. Tenchini,Yusuke Uchiyama,M. Venturini,C. Voena,Akira Yamamoto,Kayo Yoshida,Z. You,Yury V. Yudin,Yury V. Yudin,D. Zanello +93 more
TL;DR: The final results of the search for the lepton flavour violating decay were presented in this paper, based on the full dataset collected by the MEG experiment at the Paul Scherrer Institut in the period 2009-2013.
Journal ArticleDOI
New Constraint on the Existence of the μ + → e + γ Decay
J. Adam,J. Adam,X. Bai,A. M. Baldini,E. Baracchini,E. Baracchini,C. Bemporad,G. Boca,P. W. Cattaneo,G. Cavoto,Fabrizio Cei,C. Cerri,A. de Bari,M. De Gerone,Tadayoshi Doke,S. Dussoni,J. Egger,Yasunori Fujii,L. Galli,Flavio Gatti,B. Golden,Marco Grassi,A. Graziosi,D.N. Grigoriev,D.N. Grigoriev,Tomiyoshi Haruyama,M. Hildebrandt,Y. Hisamatsu,F.V. Ignatov,T. Iwamoto,D. Kaneko,P.R. Kettle,B.I. Khazin,N. Khomotov,O. Kiselev,A. S. Korenchenko,N. Kravchuk,G. M. A. Lim,A. Maki,Satoshi Mihara,W. R. Molzon,Takehiko Mori,D. Mzavia,Roberto Di Nardo,H. Natori,H. Natori,Donato Nicolo,Hajime Nishiguchi,Y. Nishimura,Wataru Ootani,M. Panareo,Angela Papa,G. Piredda,A.S. Popov,F. Renga,F. Renga,E. Ripiccini,Stefan Ritt,M. Rossella,Ryu Sawada,F. Sergiampietri,Giovanni Signorelli,S. Suzuki,F. Tenchini,C. Topchyan,Yusuke Uchiyama,Yusuke Uchiyama,C. Voena,F. Xiao,S. Yamada,Akira Yamamoto,Satoru Yamashita,Z. You,Yu.V. Yudin,D. Zanello +74 more
TL;DR: The data collected by the MEG experiment at the Paul Scherrer Institut show no excess of events compared to background expectations and yield a new upper limit on the branching ratio of this decay of 5.7 × 10(-13) (90% confidence level).
Journal ArticleDOI
New limit on the lepton-flavor-violating decay μ+→e+γ.
J. Adam,J. Adam,X. Bai,A. M. Baldini,E. Baracchini,C. Bemporad,G. Boca,P. W. Cattaneo,G. Cavoto,Fabrizio Cei,C. Cerri,A. de Bari,M. De Gerone,Tadayoshi Doke,S. Dussoni,J. Egger,K. Fratini,Yasunori Fujii,Luca Galli,G. Gallucci,Flavio Gatti,B. Golden,Marco Grassi,D.N. Grigoriev,Tomiyoshi Haruyama,M. Hildebrandt,Y. Hisamatsu,F.V. Ignatov,T. Iwamoto,P.R. Kettle,B.I. Khazin,O. Kiselev,A. S. Korenchenko,N. Kravchuk,A. Maki,Satoshi Mihara,W. R. Molzon,Takehiko Mori,D. Mzavia,H. Natori,H. Natori,Donato Nicolo,Hajime Nishiguchi,Y. Nishimura,Wataru Ootani,M. Panareo,Angela Papa,R. Pazzi,G. Piredda,A.S. Popov,F. Renga,Stefan Ritt,M. Rossella,Ryu Sawada,F. Sergiampietri,Giovanni Signorelli,S. Suzuki,F. Tenchini,C. Topchyan,Yusuke Uchiyama,Yusuke Uchiyama,R. Valle,C. Voena,F. Xiao,S. Yamada,Akira Yamamoto,Satoru Yamashita,Yu.V. Yudin,D. Zanello +68 more
TL;DR: In this article, the authors presented a new result based on an analysis of the data collected by the MEG detector at the Paul Scherrer Institut in 2009 and 2010, in search of the lepton-flavor-violating decay.
Journal ArticleDOI
The Large Observatory For X-ray Timing: LOFT
Marco Feroci,Luigi Stella,M. van der Klis,T. J.-L. Courvoisier,Margarita Hernanz,René Hudec,Andrea Santangelo,Dom Walton,A. A. Zdziarski,Didier Barret,Tomaso Belloni,João Braga,Søren Brandt,Carl Budtz-Jørgensen,Sergio Campana,J. W. den Herder,Juhani Huovelin,G. L. Israel,Martin Pohl,Paul S. Ray,A. Vacchi,Silvia Zane,A. Argan,Primo Attina,Giuseppe Bertuccio,Enrico Bozzo,Riccardo Campana,Deepto Chakrabarty,Enrico Costa,A. de Rosa,E. Del Monte,S. Di Cosimo,I. Donnarumma,Y. Evangelista,D. Haas,Peter G. Jonker,S. Korpela,Claudio Labanti,Piero Malcovati,Roberto Mignani,Fabio Muleri,Massimo Rapisarda,Massimo Rapisarda,Alexander Rashevsky,Nanda Rea,Alda Rubini,C. Tenzer,Colleen A. Wilson-Hodge,Berend Winter,K. S. Wood,G. Zampa,N. Zampa,Marek A. Abramowicz,M. A. Alpar,Diego Altamirano,Diego Altamirano,J. M. Alvarez,Lorenzo Amati,C. Amoros,Louis Antonelli,R. Artigue,P. Azzarello,Matteo Bachetti,Giuseppe Baldazzi,Marco Barbera,Cesare Barbieri,Stéphane Basa,Altan Baykal,R. Belmont,L. Boirin,V. Bonvicini,Luciano Burderi,M. Bursa,C. Cabanac,Edward M. Cackett,G. A. Caliandro,Piergiorgio Casella,Sylvain Chaty,Jérôme Chenevez,M. J. Coe,Alfonso Collura,Alessandro Corongiu,Stefano Covino,Giancarlo Cusumano,Flavio D'Amico,S. Dall'Osso,D. de Martino,G. De Paris,G. Di Persio,T. Di Salvo,Chris Done,M. Dovčiak,Alessandro Drago,Ünal Ertan,Sergio Fabiani,M. Falanga,Rob Fender,P. Ferrando,Desiree Della Monica Ferreira,G.W. Fraser,Filippo Frontera,F. Fuschino,J. L. Galvez,Poshak Gandhi,P. Giommi,O. Godet,E. Göǧüş,Andrea Goldwurm,D. Gotz,Marco Grassi,P. Guttridge,Pasi Hakala,Gilles Henri,W. Hermsen,J. Horak,Allan Hornstrup,J. J. M. in 't Zand,Jordi Isern,Emrah Kalemci,Gottfried Kanbach,V. Karas,Dhiren Kataria,T. Kennedy,D. Klochkov,W. Kluźniak,Kostas D. Kokkotas,I. Kreykenbohm,Julian H. Krolik,L. Kuiper,Irfan Kuvvetli,Nikolaos D. Kylafis,James M. Lattimer,Francesco Lazzarotto,Denis Leahy,Francois Lebrun,Dacheng Lin,Niels Lund,Thomas J. Maccarone,Julien Malzac,Martino Marisaldi,Adrian Martindale,M. Mastropietro,Jeffrey E. McClintock,I. M. McHardy,Mariano Mendez,Sandro Mereghetti,M. C. Miller,Teresa Mineo,Ennio Morelli,Sharon M. Morsink,C. Motch,S. Motta,T. Muñoz-Darias,Giampiero Naletto,Vitaly Neustroev,Jukka Nevalainen,J. F. Olive,Marina Orio,Mauro Orlandini,Piotr Orleanski,Feryal Özel,Luigi Pacciani,Stéphane Paltani,I. E. Papadakis,Alessandro Papitto,Alessandro Patruno,A. Pellizzoni,V. Petracek,J. Petri,P.-O. Petrucci,B. F. Phlips,L. Picolli,A. Possenti,Dimitrios Psaltis,Damien Rambaud,Pablo Reig,Ron Remillard,J. L. Rodriguez,P. Romano,Marina M. Romanova,Thomas Schanz,Christian Schmid,A. Segreto,Andrew Shearer,Alan Smith,Philip J. Smith,Paolo Soffitta,Nikolaos Stergioulas,Marcin Stolarski,Zdeněk Stuchlík,Andrea Tiengo,Diego F. Torres,Gabriel Török,R. Turolla,Phil Uttley,Simon Vaughan,S. Vercellone,R. Waters,Anna L. Watts,Roman Wawrzaszek,N. A. Webb,Jörn Wilms,Luca Zampieri,Andreas Zezas,J. Ziolkowski +204 more
TL;DR: The Large Observatory For X-ray Timing (LOFT) was selected by the European Space Agency (ESA) Cosmic Vision Theme "Matter under extreme conditions", namely: does matter orbiting close to the event horizon follow the predictions of general relativity? What is the equation of state of matter in neutron stars? LOFT, selected by ESA as one of the four Cosmic Vision M3 candidate missions to undergo an assessment phase, will revolutionise the study of collapsed objects in our galaxy and of the brightest supermassive black holes in active galactic nuclei.
Journal ArticleDOI
The enhanced X-ray Timing and Polarimetry mission—eXTP
Shuang-Nan Zhang,Andrea Santangelo,Andrea Santangelo,Marco Feroci,Yupeng Xu,Fangjun Lu,Yong Chen,Hua Feng,Shu Zhang,Søren Brandt,Margarita Hernanz,Luca Baldini,Enrico Bozzo,Riccardo Campana,Alessandra De Rosa,Yongwei Dong,Y. Evangelista,Vladimir Karas,Norbert Meidinger,A. Meuris,Kirpal Nandra,Teng Pan,Giovanni Pareschi,Piotr Orleanski,Qiushi Huang,Stéphane Schanne,G. Sironi,Daniele Spiga,Jiri Svoboda,Gianpiero Tagliaferri,C. Tenzer,Andrea Vacchi,Andrea Vacchi,Silvia Zane,D. Walton,Zhanshan Wang,Berend Winter,Xin Wu,Jean J. M. in't Zand,M. Ahangarianabhari,G. Ambrosi,Filippo Ambrosino,Marco Barbera,Stefano Basso,Jörg Bayer,Ronaldo Bellazzini,Pierluigi Bellutti,Bruna Bertucci,Giuseppe Bertuccio,Giacomo Borghi,X. L. Cao,Franck Cadoux,F. Ceraudo,Tian-Xiang Chen,Yu-Peng Chen,Jerome Chevenez,Marta Civitani,Wei Cui,Wei-Wei Cui,Thomas Dauser,Ettore Del Monte,Sergio Di Cosimo,Sebastian Diebold,Victor Doroshenko,Michal Dovciak,Yuan-Yuan Du,Lorenzo Ducci,Qingmei Fan,Yannick Favre,F. Fuschino,J. L. Galvez,M. Gao,Ming-Yu Ge,O. Gevin,Marco Grassi,QuanYing Gu,Yu-Dong Gu,Da-Wei Han,Bin Hong,Wei Hu,Long Ji,Shu-Mei Jia,W. C. Jiang,T. Kennedy,I. Kreykenbohm,Irfan Kuvvetli,Claudio Labanti,Luca Latronico,Gang Li,Mao-Shun Li,Xian Li,Wei Li,Zheng-Wei Li,Olivier Limousin,H. T. Liu,Xiao-Jing Liu,Bo Lu,T. Luo,D. Macera,Piero Malcovati,Adrian Martindale,M. Michalska,Bin Meng,Massimo Minuti,Alfredo Morbidini,Fabio Muleri,Stéphane Paltani,Emanuele Perinati,Antonino Picciotto,Claudio Piemonte,Jin-Lu Qu,A. Rachevski,Irina Rashevskaya,Jerome Rodriguez,Thomas Schanz,Zhengxiang Shen,LiZhi Sheng,JiangBo Song,Li-Ming Song,Carmelo Sgrò,Liang Sun,Ying Tan,Phil Uttley,Bo Wang,Dianlong Wang,G. F. Wang,Juan Wang,LangPing Wang,Yu-Sa Wang,Anna L. Watts,XiangYang Wen,Jörn Wilms,Shaolin Xiong,J. W. Yang,Sheng Yang,Yanji Yang,Nian Yu,Wenda Zhang,G. Zampa,N. Zampa,Andrzej A. Zdziarski,Aimei Zhang,C. L. Zhang,Fan Zhang,Long Zhang,Tong Zhang,Yi Zhang,Xiaoli Zhang,Zi-Liang Zhang,Baosheng Zhao,ShiJie Zheng,Yupeng Zhou,Nicola Zorzi,J. Frans Zwart +153 more
TL;DR: The enhanced X-ray Timing and Polarimetry mission—eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism and will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects.