J
J. W. Menzies
Researcher at University of Canterbury
Publications - 114
Citations - 6401
J. W. Menzies is an academic researcher from University of Canterbury. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 43, co-authored 107 publications receiving 6210 citations.
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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
A COLD NEPTUNE-MASS PLANET OGLE-2007-BLG-368Lb: COLD NEPTUNES ARE COMMON
Takahiro Sumi,D. P. Bennett,Ian A. Bond,Andrzej Udalski,V. Batista,Martin Dominik,Martin Dominik,P. Fouqué,D. Kubas,Andrew Gould,Bruce Macintosh,K. H. Cook,Subo Dong,L. Skuljan,Arnaud Cassan,Fumio Abe,C. S. Botzler,Akihiko Fukui,K. Furusawa,John B. Hearnshaw,Yoshitaka Itow,Kisaku Kamiya,P. M. Kilmartin,A. V. Korpela,W. Lin,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Yasushi Muraki,M. Nagaya,Takahiro Nagayama,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,Nicholas J. Rattenbury,To. Saito,Takashi Sako,D. J. Sullivan,Winston L. Sweatman,P. J. Tristram,Philip Yock,J. P. Beaulieu,Andrew A. Cole,Ch. Coutures,M. F. Duran,J. G. Greenhill,Francisco Jablonski,U. Marboeuf,Eder Martioli,Ettore Pedretti,Ondřej Pejcha,Patricio Rojo,Michael D. Albrow,S. Brillant,M. F. Bode,D. M. Bramich,Martin Burgdorf,Martin Burgdorf,J. A. R. Caldwell,H. Calitz,E. Corrales,S. Dieters,S. Dieters,D. Dominis Prester,J. Donatowicz,K. M. Hill,K. M. Hill,M. Hoffman,Keith Horne,U. G. Jørgensen,N. Kains,Stephen R. Kane,J. B. Marquette,R. M. Martin,P. J. Meintjes,J. W. Menzies,K. R. Pollard,Kailash C. Sahu,Colin Snodgrass,Iain A. Steele,Rachel Street,Yiannis Tsapras,Joachim Wambsganss,Andrew Williams,M. Zub,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Łukasz Wyrzykowski,Krzysztof Ulaczyk,William H. Allen,G. W. Christie,Darren L. DePoy,B. S. Gaudi,C. Han,J. Janczak,C.-U. Lee,Jennie McCormick,F. Mallia,B. Monard,Tim Natusch,Byeong-Gon Park,Richard W. Pogge,R. Santallo +107 more
TL;DR: The OGLE-2007-BLG-368Lb with a planet-star mass ratio of q = [9.5 ± 2.1] × 10^(-5] via gravitational microlensing was discovered in real-time thanks to the high cadence of the Microlensing Observations in Astrophysics survey and intensive followup observations.
Journal ArticleDOI
A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common
Takahiro Sumi,D. P. Bennett,Ian A. Bond,Andrzej Udalski,V. Batista,Martin Dominik,P. Fouque,D. Kubas,Andrew Gould,Bruce Macintosh,K. H. Cook,Subo Dong,L. Skuljan,Arnaud Cassan,Fumio Abe,C. S. Botzler,Akihiko Fukui,K. Furusawa,John B. Hearnshaw,Yoshitaka Itow,Kisaku Kamiya,P. M. Kilmartin,A. V. Korpela,W. Lin,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Yasushi Muraki,M. Nagaya,Takahiro Nagayama,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,Nicholas J. Rattenbury,To. Saito,Takashi Sako,D. J. Sullivan,Winston L. Sweatman,Philip Yock,J. P. Beaulieu,Andrew A. Cole,Ch. Coutures,M. F. Duran,J. G. Greenhill,Francisco Jablonski,U. Marboeuf,Eder Martioli,Ettore Pedretti,Ondřej Pejcha,Patricio Rojo,Michael D. Albrow,S. Brillant,M. F. Bode,D. M. Bramich,Martin Burgdorf,J. A. R. Caldwell,H. Calitz,E. Corrales,S. Dieters,D. Dominis Prester,J. Donatowicz,K. M. Hill,M. Hoffman,Keith Horne,N. Kains,Stephen R. Kane,J. B. Marquette,R. M. Martin,P. J. Meintjes,J. W. Menzies,K. R. Pollard,Kailash C. Sahu,Colin Snodgrass,Iain A. Steele,Rachel Street,Yiannis Tsapras,Joachim Wambsganss,Andrew Williams,M. Zub,M.K. Szyma,M. Kubiak,G. Pietrzy,I. Soszy,O. Szewczyk,K. Ulaczyk,William H. Allen,G. W. Christie,Darren L. DePoy,B. S. Gaudi,C. Han,J. Janczak,C.-U. Lee,Jennie McCormick,F. Mallia,B. Monard,Tim Natusch,Byeong-Gon Park,Richard W. Pogge,R. Santallo +99 more
TL;DR: A Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q=[9.5 +/- 2.1] x 10^{-5} via gravitational microlensing was discovered in real-time thanks to the high cadence of the MOA survey and intensive follow-up observations as mentioned in this paper.
Journal ArticleDOI
OGLE-2005-BLG-071Lb, THE MOST MASSIVE M DWARF PLANETARY COMPANION?
Subo Dong,Andrew Gould,Andrzej Udalski,Jay Anderson,G. W. Christie,B. S. Gaudi,M. Jaroszynski,M. Kubiak,Michał K. Szymański,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,O. Szewczyk,Krzysztof Ulaczyk,Łukasz Wyrzykowski,Łukasz Wyrzykowski,Darren L. DePoy,D. B. Fox,Avishay Gal-Yam,C. Han,Sébastien Lépine,Jennie McCormick,Eran O. Ofek,Byeong-Gon Park,Richard W. Pogge,Fumio Abe,David P. Bennett,Ian A. Bond,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,Kouji Ohnishi,C. Okada,Nicholas J. Rattenbury,To. Saito,Takashi Sako,Misao Sasaki,Denis J. Sullivan,Takahiro Sumi,P. J. Tristram,T. Yanagisawa,P. C. M. Yock,T. Yoshoika,robo Net Collaborations,Michael D. Albrow,J. P. Beaulieu,S. Brillant,H. Calitz,A. Cassan,K. H. Cook,Ch. Coutures,S. Dieters,D. Dominis Prester,J. Donatowicz,P. Fouqué,J. G. Greenhill,K. M. Hill,M. Hoffman,Keith Horne,U. G. Jørgensen,Stephen R. Kane,D. Kubas,J. B. Marquette,Roland Martin,P. J. Meintjes,J. W. Menzies,K. R. Pollard,K. C. Sahu,C. Vinter,Joachim Wambsganss,Andrew Williams,M. F. Bode,D. M. Bramich,Martin Burgdorf,Colin Snodgrass,Iain A. Steele,V. Doublier,Cedric Foellmi +87 more
TL;DR: The OGLE-2005-BLG-071Lb was discovered by microlensing and the first in a high-magnification event as discussed by the authors, and the second largest known planet.
Journal ArticleDOI
MOA-2009-BLG-387Lb: a massive planet orbiting an M dwarf
V. Batista,Andrew Gould,S. Dieters,Subo Dong,Ian A. Bond,J. P. Beaulieu,D. Maoz,B. Monard,G. W. Christie,Jennie McCormick,Michael D. Albrow,Keith Horne,Yiannis Tsapras,Martin Burgdorf,Martin Burgdorf,S. Calchi Novati,Jesper Skottfelt,J. A. R. Caldwell,Szymon Kozłowski,D. Kubas,D. Kubas,B. S. Gaudi,Chang S. Han,David P. Bennett,J. An,Fumio Abe,C. S. Botzler,D. Douchin,M. Freeman,Akihiko Fukui,K. Furusawa,John B. Hearnshaw,S. Hosaka,Yoshitaka Itow,Kisaku Kamiya,P. M. Kilmartin,A. V. Korpela,W. Lin,C. H. Ling,S. Makita,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Yasushi Muraki,M. Nagaya,K. Nishimoto,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,Nicholas J. Rattenbury,To. Saito,Denis J. Sullivan,Takahiro Sumi,Winston L. Sweatman,P. J. Tristram,E. von Seggern,Philip Yock,S. Brillant,J. J. Calitz,Arnaud Cassan,Andrew A. Cole,K. H. Cook,C. Coutures,D. Dominis Prester,J. Donatowicz,J. G. Greenhill,M. Hoffman,Francisco Jablonski,Stephen R. Kane,N. Kains,N. Kains,J. B. Marquette,R. M. Martin,Eder Martioli,P. J. Meintjes,J. W. Menzies,Ettore Pedretti,K. R. Pollard,Kailash C. Sahu,C. Vinter,Joachim Wambsganss,R. D. Watson,Andrew Williams,M. Zub,M. Zub,William H. Allen,Greg Bolt,M. Bos,Darren L. DePoy,Jack D. Drummond,Jason D. Eastman,Avishay Gal-Yam,E. Gorbikov,E. Gorbikov,D. Higgins,J. Janczak,Shai Kaspi,Shai Kaspi,C.-U. Lee,F. Mallia,Anaëlle Maury,L. A. G. Monard,D. Moorhouse,N. D. Morgan,Tim Natusch,Eran O. Ofek,Byeong-Gon Park,Richard W. Pogge,David Polishook,R. Santallo,Avi Shporer,O. Spector,G. Thornley,Jennifer C. Yee,Valerio Bozza,P. Browne,Martin Dominik,Martin Dominik,Stefan Dreizler,F. Finet,M. Glitrup,Frank Grundahl,K. B. W. Harpsøe,Frederic V. Hessman,Tobias C. Hinse,Tobias C. Hinse,M. Hundertmark,U. G. Jørgensen,U. G. Jørgensen,C. Liebig,C. Liebig,G. Maier,Luigi Mancini,Luigi Mancini,M. Mathiasen,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,John Southworth,Jean Surdej,F. Zimmer,F. Zimmer,Alasdair Allan,D. M. Bramich,Colin Snodgrass,Colin Snodgrass,Iain A. Steele,Rachel Street,Rachel Street +148 more
TL;DR: In this article, the authors reported the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval.