Wise Team
1 Papers
Wise Team is an academic researcher. The author has contributed to research in topics: Mass ratio & Order (ring theory). The author has an hindex of 1, co-authored 1 publications.
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Papers
OGLE-2013-BLG-0911Lb: A Secondary on the Brown-dwarf Planet Boundary around an M Dwarf
Shota Miyazaki,Takahiro Sumi,David P. Bennett,David P. Bennett,Andrzej Udalski,Yossi Shvartzvald,Rachel Street,Valerio Bozza,Valerio Bozza,Jennifer C. Yee,Ian A. Bond,Nicholas J. Rattenbury,Naoki Koshimoto,Daisuke Suzuki,Akihiko Fukui,Akihiko Fukui,Fumio Abe,Aparna Bhattacharya,Aparna Bhattacharya,Richard K. Barry,Martin Donachie,Hirosane Fujii,Yuki Hirao,Yoshitaka Itow,Y. Kamei,Iona Kondo,Man Cheung Alex Li,C. H. Ling,Yutaka Matsubara,Taro Matsuo,Yasushi Muraki,Masayuki Nagakane,K. Ohnishi,Clément Ranc,To. Saito,A. Sharan,Hiroshi Shibai,Haruno Suematsu,Denis J. Sullivan,Paul J. Tristram,T. Yamakawa,Atsunori Yonehara,Jan Skowron,Radosław Poleski,P. Mróz,P. Mróz,Michał K. Szymański,Igor Soszyński,P. Pietrukowicz,S. KozŁowski,Krzysztof Ulaczyk,Łukasz Wyrzykowski,M. Friedmann,Shai Kaspi,Dan Maoz,Wise Team,Michael D. Albrow,G. W. Christie,Darren L. DePoy,Avishay Gal-Yam,Andrew Gould,Andrew Gould,Andrew Gould,C.-U. Lee,C.-U. Lee,Ilan Manulis,Jennie McCormick,Tim Natusch,H. Ngan,R. W. Pogge,I. Porritt,Yiannis Tsapras,Etienne Bachelet,Etienne Bachelet,M. Hundertmark,Martin Dominik,D. M. Bramich,Arnaud Cassan,R. Figuera Jaimes,R. Figuera Jaimes,Keith Horne,R. W. Schmidt,Colin Snodgrass,Joachim Wambsganss,Iain A. Steele,J. W. Menzies,Shude Mao,Shude Mao,Shude Mao,RoboNet Collabofratino,U. G. Jørgensen,Martin Burgdorf,Simona Ciceri,S. Calchi Novati,Giuseppe D'Ago,Giuseppe D'Ago,Giuseppe D'Ago,Daniel F. Evans,Tobias C. Hinse,N. Kains,Eamonn Kerins,Heidi Korhonen,Luigi Mancini,A. Popovas,Markus Rabus,Sohrab Rahvar,Gaetano Scarpetta,Gaetano Scarpetta,Jesper Skottfelt,Jesper Skottfelt,John Southworth,Nuno Peixinho,Nuno Peixinho,P. Verma +113 more
TL;DR: In this paper, the binary-lens microlensing event OGLE-2013-BLG-0911 was analyzed and two groups of solutions for the projected separation normalized by the Einstein radius of s ∼ 0.15 or s ∼ 7.2 were presented.