M
M. Kubiak
Researcher at University of Warsaw
Publications - 389
Citations - 22404
M. Kubiak is an academic researcher from University of Warsaw. The author has contributed to research in topics: Gravitational microlensing & Gravitational lens. The author has an hindex of 77, co-authored 389 publications receiving 21457 citations.
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Journal ArticleDOI
Limb-darkening measurements for a cool red giant in microlensing event OGLE 2004-BLG-482
M. Zub,Arnaud Cassan,D. Heyrovsky,P. Fouque,H. C. Stempels,Michael D. Albrow,J. P. Beaulieu,Stephane Brillant,G. W. Christie,N. Kains,S. Kozlowski,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,Igor Soszyński,O. Szewczyk,L. Wyrzykowski +49 more
TL;DR: In this article, a detailed analysis of OGLE 2004-BLG-482, a relatively high-magnification single-lens microlensing event which exhibits clear extended-source effects is presented.
Journal ArticleDOI
Super-massive Planets around Late-type Stars—the Case of OGLE-2012-BLG-0406Lb
Radosław Poleski,Radosław Poleski,Andrzej Udalski,Subo Dong,Michał K. Szymański,Igor Soszyński,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Szymon Kozłowski,Paweł Pietrukowicz,Krzysztof Ulaczyk,Jan Skowron,Łukasz Wyrzykowski,Łukasz Wyrzykowski,Andrew Gould +15 more
TL;DR: In this article, the authors presented a discovery of a 3.9 ± 1.2 M Jup mass planet orbiting the 0.59 ± 0.17 M ☉ star using the gravitational microlensing method.
Journal ArticleDOI
Massive stars exploding in a He-rich circumstellar medium – V. Observations of the slow-evolving SN Ibn OGLE-2012-SN-006
A. Pastorello,Łukasz Wyrzykowski,Łukasz Wyrzykowski,Stefano Valenti,Stefano Valenti,J. L. Prieto,J. L. Prieto,S. Kozlowski,Andrzej Udalski,Nancy Elias-Rosa,A. Morales-Garoffolo,Joseph P. Anderson,S. Benetti,Melina C. Bersten,Melina C. Bersten,Melina C. Bersten,M. T. Botticella,Enrico Cappellaro,Giovanni Fasano,Morgan Fraser,Avishay Gal-Yam,M. Gillone,Melissa L. Graham,Melissa L. Graham,Jochen Greiner,Stephan Hachinger,Stephan Hachinger,D. A. Howell,D. A. Howell,Cosimo Inserra,Jerod T. Parrent,Jerod T. Parrent,Arne Rau,Steve Schulze,Stephen J. Smartt,K. W. Smith,Massimo Turatto,O. Yaron,David Young,M. Kubiak,Michał K. Szymański,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,Krzysztof Ulaczyk,Radosław Poleski,Radosław Poleski,P. Pietrukowicz,Jan Skowron,P. Mróz +49 more
TL;DR: The OGLE-2012-SN-006 was discovered and monitored by the Optical Gravitational Lensing Experiment-IV survey, and spectroscopically followed by Public ESO Spectroscopic Survey of Transient Objects (PESSTO) at late phases as discussed by the authors.
Journal ArticleDOI
MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?
K. Furusawa,Andrzej Udalski,Takahiro Sumi,David P. Bennett,Ian A. Bond,Andrew Gould,U. G. Jørgensen,Colin Snodgrass,D. Dominis Prester,Michael D. Albrow,Fumio Abe,C. S. Botzler,P. Chote,M. Freeman,Akihiko Fukui,P. Harris,Yoshitaka Itow,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Yasushi Muraki,Kouji Ohnishi,Nicholas J. Rattenbury,Denis J. Sullivan,Daisuke Suzuki,Winston L. Sweatman,Paul J. Tristram,K. Wada,Philip Yock,Michał K. Szymański,Igor Soszyński,M. Kubiak,Radosław Poleski,Krzysztof Ulaczyk,Grzegorz Pietrzyński,L. Wyrzykowski,J.-Y. Choi,G. W. Christie,Darren L. DePoy,Subo Dong,Jack D. Drummond,B. S. Gaudi,Chang S. Han,Jennie McCormick,D. Moorhouse,Tim Natusch,M. Nola,Eran O. Ofek,Byeong-Gon Park,H. Park,Richard W. Pogge,Jan Skowron,G. Thornley,Jennifer C. Yee,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Martin Dominik,François Finet,T. Gerner,S. Hardis,K. B. W. Harpsøe,Tobias C. Hinse,M. Hundertmark,N. Kains,Eamonn Kerins,C. Liebig,Luigi Mancini,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,S. Schäfer,F. Schönebeck,John Southworth,Jean Surdej,Joachim Wambsganss,Rachel Street,D. M. Bramich,Iain A. Steele,Yiannis Tsapras,Keith Horne,J. Donatowicz,Kailash C. Sahu,Etienne Bachelet,V. Batista,Thomas G. Beatty,C. S. Bennett,Christine S. Black,R. Bowens-Rubin,Stephane Brillant,J. A. R. Caldwell,Arnaud Cassan,Andrew A. Cole,E. Corrales,C. Coutures,S. Dieters,P. Fouqué,J. G. Greenhill,Calen B. Henderson,D. Kubas,R. Martin,J. W. Menzies,B. J. Shappee,Andrew Williams,D. Wouters,J. van Saders,Robert T. Zellem,M. Zub +114 more
TL;DR: In this article, the authors analyzed the planetary microlensing event MOA-2010-BLG-328 and showed that the microlens parallax signal, which determines the host mass and distance, is actually due to xallarap (source orbital motion) that is being misinterpreted as paralax.
Journal ArticleDOI
OGLE-TR-211 – a new transiting inflated hot Jupiter from the OGLE survey and ESO LP666 spectroscopic follow-up program
Andrzej Udalski,Frederic Pont,Dominique Naef,C. Melo,François Bouchy,Nuno C. Santos,C. Moutou,Rodrigo F. Díaz,Wolfgang Gieren,Michaël Gillon,Sergio Hoyer,M. Mayor,Tsevi Mazeh,Dante Minniti,Grzegorz Pietrzyński,D. Queloz,S. Ramírez,Maria Teresa Ruiz,Avi Shporer,Omer Tamuz,Stéphane Udry,Manuela Zoccali,M. Kubiak,Michał K. Szymański,Igor Soszyński,O. Szewczyk,Krzysztof Ulaczyk,Lukasz Wyrzykowski +27 more
TL;DR: The OGLE-TR-211b candidate as mentioned in this paper is a hot Jupiter orbiting an F7-8 spectral type dwarf star with a period of 3.68 days and its mass is equal to 1.03± 0.20 M Jup, while its radius R Jup.