C
C. Vinter
Researcher at Niels Bohr Institute
Publications - 12
Citations - 1716
C. Vinter is an academic researcher from Niels Bohr Institute. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 10, co-authored 12 publications receiving 1643 citations. Previous affiliations of C. Vinter include Institut d'Astrophysique de Paris.
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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
One or more bound planets per Milky Way star from microlensing observations
Arnaud Cassan,Arnaud Cassan,D. Kubas,D. Kubas,J. P. Beaulieu,J. P. Beaulieu,Martin Dominik,Martin Dominik,Keith Horne,Keith Horne,J. G. Greenhill,J. G. Greenhill,Joachim Wambsganss,Joachim Wambsganss,J. W. Menzies,Andrew Williams,U. G. Jørgensen,U. G. Jørgensen,Andrzej Udalski,David P. Bennett,David P. Bennett,Michael D. Albrow,Michael D. Albrow,V. Batista,S. Brillant,S. Brillant,J. A. R. Caldwell,J. A. R. Caldwell,Andrew A. Cole,Andrew A. Cole,Ch. Coutures,K. H. Cook,K. H. Cook,S. Dieters,S. Dieters,D. Dominis Prester,D. Dominis Prester,J. Donatowicz,J. Donatowicz,Pascal Fouqué,Pascal Fouqué,K. Hill,K. Hill,N. Kains,N. Kains,Stephen R. Kane,Stephen R. Kane,J. B. Marquette,R. Martin,K. R. Pollard,K. R. Pollard,Kailash C. Sahu,Kailash C. Sahu,C. Vinter,C. Vinter,D. Warren,D. Warren,B. Watson,B. Watson,M. Zub,M. Zub,Takahiro Sumi,Michał K. Szymański,M. Kubiak,Radosław Poleski,Igor Soszyński,Krzysztof Ulaczyk,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Łukasz Wyrzykowski,Łukasz Wyrzykowski +70 more
TL;DR: It is concluded that stars are orbited by planets as a rule, rather than the exception, and that of stars host Jupiter-mass planets 0.5–10 au (Sun–Earth distance) from their stars.
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.
Journal ArticleDOI
Full characterization of binary-lens event OGLE-2002-BLG-069 from PLANET observations
D. Kubas,Arnaud Cassan,J. P. Beaulieu,Ch. Coutures,Ch. Coutures,Martin Dominik,Michael D. Albrow,S. Brillant,John A. R. Caldwell,D. Dominis,J. Donatowicz,Christian Fendt,P. Fouque,U. G. Jørgensen,J. G. Greenhill,K. Hill,Janine Heinmüller,Keith Horne,Stephen R. Kane,J. B. Marquette,Ralph Martin,J. W. Menzies,K. R. Pollard,Kailash C. Sahu,C. Vinter,Joachim Wambsganss,R. D. Watson,Andrew Williams,C. Thurl +28 more
TL;DR: In this article, the photometric data obtained by PLANET and OGLE on the caustic-crossing binary-lens microlensing event OGLE-2002-BLG-069 were analyzed.
Journal ArticleDOI
Limb-darkening measurements for a cool red giant in microlensing event OGLE 2004-BLG-482
M. Zub,M. Zub,Arnaud Cassan,Arnaud Cassan,David Heyrovský,Pascal Fouqué,H. C. Stempels,Michael D. Albrow,J. P. Beaulieu,S. Brillant,G. W. Christie,N. Kains,S. Kozłowski,D. Kubas,D. Kubas,Joachim Wambsganss,V. Batista,David P. Bennett,K. H. Cook,C. Coutures,S. Dieters,Martin Dominik,D. Dominis Prester,J. Donatowicz,J. G. Greenhill,Keith Horne,U. G. Jørgensen,S. R. Kane,J. B. Marquette,R. M. Martin,J. W. Menzies,K. R. Pollard,Kailash C. Sahu,C. Vinter,Andrew Williams,Andrew Gould,Darren L. DePoy,Avishay Gal-Yam,B. S. Gaudi,C. Han,Y. M. Lipkin,D. Maoz,Eran O. Ofek,Byeong-Gon Park,R. W. Pogge,Jennie McCormick,Andrzej Udalski,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Łukasz Wyrzykowski,Łukasz Wyrzykowski +54 more
TL;DR: In this article, the authors present a detailed analysis of OGLE 2004-BLG-482, a relatively high-magnification single-lens microlensing event that exhibits clear extended-source effects.