F
Fumio Abe
Researcher at Nagoya University
Publications - 549
Citations - 24812
Fumio Abe is an academic researcher from Nagoya University. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 79, co-authored 526 publications receiving 23567 citations. Previous affiliations of Fumio Abe include University of Auckland & Osaka University.
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Journal ArticleDOI
Observation of top quark production in p̄p collisions with the collider detector at fermilab
Fumio Abe,H. Akimoto,A. Akopian,M. G. Albrow,S. R. Amendolia,D. Amidei,J. Antos,C. Anway-Wiese,S. Aota,Giorgio Apollinari,T. Asakawa,W. Ashmanskas,M. Atac,P. Auchincloss,F. Azfar,P. Azzi-Bacchetta,Nicola Bacchetta,W. Badgett,S. Bagdasarov,M. W. Bailey,J. Bao,P. de Barbaro,A. Barbaro-Galtieri,Virgil E Barnes,B. A. Barnett,P. Bartalini,G. Bauer,T. Baumann,F. Bedeschi,S. Behrends,Stefano Belforte,G. Bellettini,J. N. Bellinger,Douglas Benjamin,Jose M. Benlloch,James Bensinger,D. Benton,Andrew Beretvas,J. P. Berge,S. Bertolucci,A. Bhatti,K. Biery,K. Biery,M. Binkley,Dario Bisello,R. E. Blair,Craig Blocker,A. Bodek,W. Bokhari,V. Bolognesi,Daniela Bortoletto,J. Boudreau,G. W. Brandenburg,L. Breccia,C. Bromberg,E. Buckley-Geer,H. S. Budd,Kevin Burkett,G. Busetto,A. Byon-Wagner,K. L. Byrum,J. Cammerata,C. Campagnari,M. Campbell,A. Caner,W. Carithers,Duncan Carlsmith,Andrea Castro,G. Cauz,Y. Cen,F. Cervelli,H. Y. Chao,J. W. Chapman,M. T. Cheng,G. Chiarelli,T. Chikamatsu,C. N. Chiou,L. Christofek,S. Cihangir,Allan G Clark,Marina Cobal,M. Contreras,J. Conway,J. Cooper,M. Cordelli,C. Couyoumtzelis,D. Crane,Daniel P Cronin-Hennessy,R. Culbertson,J. D. Cunningham,T. Daniels,F. DeJongh,S. Delchamps,S. Dell'Agnello,M. Dell'Orso,L. Demortier,B. Denby,M. M. Deninno,P. F. Derwent,T. Devlin,M. Dickson,Jay Dittmann,S. Donati,R. B. Drucker,A. Dunn,N. Eddy,Kevin Einsweiler,J. E. Elias,R. Ely,E. Engels,D. Errede,S. Errede,Q. Fan,I. Fiori,B. Flaugher,G. W. Foster,M. Franklin,M. Frautschi,J. C. Freeman,J.I. Friedman,Henry J. Frisch,T. A. Fuess,Yasuo Fukui,S. Funaki,G. Gagliardi,S. Galeotti,Michele Gallinaro,Maurice Garcia-Sciveres,Alan Garfinkel,S. Geer,D. W. Gerdes,P. Giannetti,Nikos Giokaris,P. Giromini,L. Gladney,D. Glenzinski,M. Gold,J. Gonzalez,A. Gordon,A. T. Goshaw,K. Goulianos,H. Grassmann,L. Groer,C. Grosso-Pilcher,G. Guillian,R. S. Guo,C. Haber,S. R. Hahn,R. Hamilton,R. Handler,R. M. Hans,Kazuhiko Hara,B. Harral,Robert M Harris,S. A. Hauger,Jay Hauser,C. Hawk,E. Hayashi,Jochen Jens Heinrich,Marcus Hohlmann,Marcus Hohlmann,C. Holck,R. J. Hollebeek,L. Holloway,A. Hölscher,A. Hölscher,Hong Sj,G. Houk,P. Hu,B. T. Huffman,R. E. Hughes,J. Huston,John Huth,J. Hylen,Hiroshi Ikeda,M. Incagli,J. Incandela,J. Iwai,Y. Iwata,Henrik Jeldtoft Jensen,Umesh Joshi,R. W. Kadel,E. Kajfasz,Teruki Kamon,T. Kaneko,K. Karr,H. Kasha,Y. Kato,L. Keeble,K. Kelley,R. D. Kennedy,R. Kephart,P. Kesten,D. Kestenbaum,R. M. Keup,H. Keutelian,F. Keyvan,Bj Kim,Doyeong Kim,Hyun-Chul Kim,Hyun-Chul Kim,S. B. Kim,S. H. Kim,Yongsun Kim,L. E. Kirsch,P. Koehn,Kiminori Kondo,J. Konigsberg,Sacha E Kopp,Kostantinos Kordas,Kostantinos Kordas,W. Koska,E. Kovacs,W. Kowald,M. Krasberg,J. Kroll,Mark Kruse,T. Kuwabara,Steve Kuhlmann,E. Kuns,A. T. Laasanen,Nicola Labanca,Stephan Lammel,J. I. Lamoureux,T. LeCompte,S. Leone,J. D. Lewis,P. Limon,M. Lindgren,Tony Liss,N. S. Lockyer,O. Long,C. Loomis,M. Loreti,Jun Lu,D. Lucchesi,P. Lukens,S. Lusin,J. Lys,Kaori Maeshima,A. Maghakian,Petar Maksimovic,M. Mangano,J. Mansour,Mosè Mariotti,J. P. Marriner,A. Martin,J. A.J. Matthews,R. Mattingly,P. McIntyre,P. Melese,A. Menzione,E. Meschi,Scott D. Metzler,C. Miao,G. Michail,S. Mikamo,R. J. Miller,H. Minato,S. Miscetti,M. Mishina,H. Mitsushio,T. Miyamoto,S. Miyashita,Y. Morita,James Mueller,A. Mukherjee,T. Muller,P. Murat,H. Nakada,I. Nakano,C. Nelson,D. Neuberger,Catherine Newman-Holmes,M. Ninomiya,Lawrence Nodulman,S. Ogawa,S. H. Oh,K. E. Ohl,T. Ohmoto,T. Ohsugi,R. Oishi,M. Okabe,T. Okusawa,Rachel A. Oliver,James D. Olsen,C. Pagliarone,Riccardo Paoletti,V. Papadimitriou,S. P. Pappas,Sung Keun Park,J. Patrick,G. Pauletta,Manfred Paulini,L. Pescara,M. D. Peters,T. J. Phillips,G. Piacentino,M. Pillai,K. T. Pitts,R. K. Plunkett,L. Pondrom,James Proudfoot,F. Ptohos,G. Punzi,K. Ragan,K. Ragan,A. Ribon,F. Rimondi,L. Ristori,W. J. Robertson,T. Rodrigo,J. Romano,L. Rosenson,R. Roser,W. K. Sakumoto,D. Saltzberg,Andrea Sansoni,L. Santi,H. Sato,V. Scarpine,P. Schlabach,E. E. Schmidt,M. P. Schmidt,G. F. Sciacca,A. Scribano,S. Segler,Sally Seidel,Y. Seiya,G. Sganos,G. Sganos,A. Sgolacchia,Marjorie Shapiro,N. M. Shaw,Q. Shen,P. F. Shepard,M. Shimojima,M. J. Shochet,J. Siegrist,Alan Sill,P.K. Sinervo,P.K. Sinervo,P. Singh,J. Skarha,K. Sliwa,D. A. Smith,F. D. Snider,T. Song,J. Spalding,P. Sphicas,Leonard Spiegel,A. Spies,Luca Stanco,J. Steele,A. Stefanini,K. Strahl,K. Strahl,James Strait,David Stuart,G. Sullivan,A. Soumarokov,Konstanty Sumorok,J. Suzuki,T. Takada,T. Takahashi,T. Takano,K. Takikawa,N. Tamura,F. Tartarelli,Wendy Taylor,Wendy Taylor,P. K. Teng,Y. Teramoto,S. Tether,D. Theriot,T. L. Thomas,R. P. Thun,M. Timko,Paul Tipton,A. Titov,S. Tkaczyk,D. Toback,K. Tollefson,A. Tollestrup,J. Tonnison,J. F. de Troconiz,S. Truitt,J. Tseng,Nicola Turini,T. Uchida,N. Uemura,F. Ukegawa,G. Unal,S. C. van den Brink,S. Vejcik,G. Velev,R. Vidal,M. Vondracek,D. Vucinic,R. G. Wagner,R. L. Wagner,J. Wahl,R. C. Walker,C. H. Wang,C. H. Wang,G. Wang,Jing Wang,M. J. Wang,Q. F. Wang,Andreas Warburton,Andreas Warburton,Gordon Watts,T. L. Watts,R. C. Webb,C. Wei,Chris Wendt,H. Wenzel,W. C. Wester,A. B. Wicklund,E. Wicklund,R. Wilkinson,H. H. Williams,P. Wilson,B. L. Winer,D. Wolinski,J. Wolinski,X. Wu,J. Wyss,Avraham Yagil,W-M. Yao,K. Yasuoka,Y. Ye,Y. Ye,G. P. Yeh,P. Yeh,M. Yin,J. Yoh,C. Yosef,T. Yoshida,D. D. Yovanovitch,I. Yu,J. C. Yun,A. Zanetti,F. Zetti,Le Zhang,Weiya Zhang,S. Zucchelli +446 more
TL;DR: In this paper, the existence of the top quark was established using a data sample of collisions at the Fermilab National Ensemble (CDF) collected with the Collider Detector.
Journal ArticleDOI
Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing
J. P. Beaulieu,David P. Bennett,Pascal Fouqué,Andrew Williams,Martin Dominik,U. G. Jørgensen,D. Kubas,Arnaud Cassan,C. Coutures,J. G. Greenhill,K. M. Hill,J. W. Menzies,Penny D. Sackett,Michael D. Albrow,S. Brillant,J. A. R. Caldwell,J. J. Calitz,K. H. Cook,E. Corrales,M. Desort,S. Dieters,D. Dominis,J. Donatowicz,M. Hoffman,Stephen R. Kane,J. B. Marquette,R. M. Martin,P. J. Meintjes,K. R. Pollard,Kailash C. Sahu,C. Vinter,Joachim Wambsganss,K. Woller,Keith Horne,Iain A. Steele,D. M. Bramich,D. M. Bramich,Martin Burgdorf,Colin Snodgrass,M. F. Bode,Andrzej Udalski,Michał K. Szymański,M. Kubiak,T. Wiȩckowski,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Łukasz Wyrzykowski,Bohdan Paczynski,Fumio Abe,Ian A. Bond,T. R. Britton,T. R. Britton,A. C. Gilmore,John B. Hearnshaw,Yoshitaka Itow,Kisaku Kamiya,P. M. Kilmartin,A. V. Korpela,Kimiaki Masuda,Yutaka Matsubara,M. Motomura,Yasushi Muraki,Shota Nakamura,C. Okada,Kouji Ohnishi,Nicholas J. Rattenbury,Takashi Sako,Susumu Sato,Misao Sasaki,T. Sekiguchi,Denis J. Sullivan,P. J. Tristram,Philip Yock,T. Yoshioka +74 more
TL;DR: The detection of a cool, sub-Neptune-mass planets may be more common than gas giant planets, as predicted by the core accretion theory, and is suggested to name OGLE-2005-BLG-390Lb, indicating a planetary mass companion to the lens star of the microlensing event.
Journal ArticleDOI
Unbound or distant planetary mass population detected by gravitational microlensing
Takahiro Sumi,Kisaku Kamiya,David P. Bennett,Ian A. Bond,Fumio Abe,C. S. Botzler,Akihiko Fukui,K. Furusawa,John B. Hearnshaw,Yoshitaka Itow,P. M. Kilmartin,A. V. Korpela,W. Lin,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,M. Motomura,Yasushi Muraki,M. Nagaya,Shota Nakamura,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,Nicholas J. Rattenbury,To. Saito,T. K. Sako,Denis J. Sullivan,Winston L. Sweatman,P. J. Tristram,P. C. M. Yock,Andrzej Udalski,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Radosław Poleski,Igor Soszyński,Łukasz Wyrzykowski,K. Ulaczyk +38 more
TL;DR: The discovery of a population of unbound or distant Jupiter-mass objects is reported, which are almost twice as common as main-sequence stars, based on two years of gravitational microlensing survey observations towards the Galactic Bulge.
Journal ArticleDOI
Real-time difference imaging analysis of moa galactic bulge observations during 2000
Ian A. Bond,Ian A. Bond,Fumio Abe,R. J. Dodd,R. J. Dodd,R. J. Dodd,John B. Hearnshaw,Morihiro Honda,Jun Jugaku,P. M. Kilmartin,P. M. Kilmartin,A. Marles,Kimiaki Masuda,Yutaka Matsubara,Yasushi Muraki,Takashi Nakamura,G. Nankivell,S. Noda,C. Noguchi,Kouji Ohnishi,Nicholas J. Rattenbury,M. Reid,To. Saito,Hiroshi Sato,Maki Sekiguchi,J. Skuljan,D. J. Sullivan,Takahiro Sumi,Mine Takeuti,Yoshiyuki Watase,S. Wilkinson,R. Yamada,T. Yanagisawa,Philip Yock +33 more
TL;DR: In this paper, the authors describe observations carried out by the MOA group of the Galactic bulge during 2000 that were designed to detect efficiently gravitational microlensing of faint stars in which the magnification is high and/or of short duration.
Journal ArticleDOI
OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event
Ian A. Bond,Andrzej Udalski,M. Jaroszyński,M. Jaroszyński,Nicholas J. Rattenbury,Bohdan Paczynski,Igor Soszyński,Lukasz Wyrzykowski,Michał K. Szymański,M. Kubiak,O. Szewczyk,O. Szewczyk,K. Żebruń,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Fumio Abe,David P. Bennett,S. Eguchi,Y. Furuta,John B. Hearnshaw,Koki Kamiya,P. M. Kilmartin,Y. Kurata,Kimiaki Masuda,Yutaka Matsubara,Yasushi Muraki,S. Noda,K. Okajima,Takashi Sako,T. Sekiguchi,Denis J. Sullivan,Takahiro Sumi,P. J. Tristram,T. Yanagisawa,Philip Yock +34 more
TL;DR: In this paper, a short-duration (~7 days) low-amplitude deviation in the light curve due to a single-lens profile was observed in both the MOA (Microlensing Observations in Astrophysics) and OGLE (Optical Gravitational Lensing Experiment) survey observations.