M
Martin Dominik
Researcher at University of St Andrews
Publications - 414
Citations - 17326
Martin Dominik is an academic researcher from University of St Andrews. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 62, co-authored 399 publications receiving 16221 citations. Previous affiliations of Martin Dominik include Max Planck Society & University of Groningen.
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Journal ArticleDOI
OGLE-2009-BLG-092/MOA-2009-BLG-137: A Dramatic Repeating Event With the Second Perturbation Predicted by Real-Time Analysis
Yoon-Hyun Ryu,C. Han,K.-H. Hwang,R. Street,Andrzej Udalski,Takahiro Sumi,Akihiko Fukui,J. P. Beaulieu,Andrew Gould,Martin Dominik,Fumio Abe,D. P. Bennett,Ian A. Bond,C. S. Botzler,K. Furusawa,F. Hayashi,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,K. Nishimoto,Kouji Ohnishi,Y. C. Perrott,N. J. Rattenbury,To. Saito,L. Skuljan,D. J. Sullivan,Daisuke Suzuki,Winston L. Sweatman,P. J. Tristram,K. Wada,P. C. M. Yock,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Łukasz Wyrzykowski,K. Ulaczyk,M. Bos,G. W. Christie,Darren L. DePoy,Avishay Gal-Yam,B. S. Gaudi,Shai Kaspi,C.-U. Lee,D. Maoz,Jennie McCormick,B. Monard,D. Moorhouse,R. W. Pogge,David Polishook,Yossi Shvartzvald,Avi Shporer,G. Thornley,Jennifer C. Yee,Michael D. Albrow,V. Batista,Stephane Brillant,Arnaud Cassan,Andrew A. Cole,E. Corrales,Ch. Coutures,S. Dieters,P. Fouque,J. G. Greenhill,J. W. Menzies,Alasdair Allan,D. M. Bramich,P. Browne,Keith Horne,N. Kains,Colin Snodgrass,Iain A. Steele,Yiannis Tsapras,Valerio Bozza,Martin Burgdorf,S. Calchi Novati,S. Dreizler,F. Finet,M. Glitrup,Frank Grundahl,Kasper Harpsøe,F. V. Hessman,Tobias C. Hinse,M. Hundertmark,U. G. Jørgensen,C. Liebig,Gernot Maier,Luigi Mancini,M. Mathiasen,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,Jesper Skottfelt,Jean Surdej,John Southworth,Joachim Wambsganss,F. Zimmer +107 more
TL;DR: In this article, the authors report the results of the analysis of a dramatic repeating gravitational microlensing event OGLE-2009-BLG-092/MOA-2009 -BLG137, for which the light curve is characterized by two distinct peaks with perturbations near both peaks.
Journal ArticleDOI
Microlensing constraints on the mass of single stars from HST astrometric measurements
N. Kains,Annalisa Calamida,Kailash C. Sahu,Stefano Casertano,Jonathan Anderson,Andrzej Udalski,Manuela Zoccali,Manuela Zoccali,Michael D. Albrow,Ian A. Bond,Thomas M. Brown,Martin Dominik,Chris L. Fryer,Mario Livio,Shude Mao,Marina Rejkuba +15 more
TL;DR: The first results from a large-scale observing campaign aiming to use astrometric microlensing to detect and place limits on the mass of single objects, including stellar remnants, were reported in this paper.
Journal ArticleDOI
Discovery of a Gas Giant Planet in Microlensing Event Ogle-2014-BLG-1760
Aparna Bhattacharya,David P. Bennett,Ian A. Bond,Takahiro Sumi,Andrzej Udalski,Rachel Street,Yiannis Tsapras,Fumio Abe,M. Freeman,Akihiko Fukui,Yuki Hirao,Yoshitaka Itow,Naoki Koshimoto,Man Cheung Alex Li,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,Yasushi Muraki,Masayuki Nagakane,Kouji Ohnishi,Nicholas J. Rattenbury,To. Saito,A. Sharan,Denis J. Sullivan,Daisuke Suzuki,Paul J. Tristram,Jan Skowron,Michał K. Szymański,Igor Soszyński,Radosław Poleski,P. Mróz,Szymon Kozłowski,P. Pietrukowicz,Krzysztof Ulaczyk,Lukasz Wyrzykowski,Etienne Bachelet,D. M. Bramich,Giuseppe D'Ago,Martin Dominik,R. Figuera Jaimes,Keith Horne,M. Hundertmark,N. Kains,J. W. Menzies,R. W. Schmidt,Colin Snodgrass,Iain A. Steele,Joachim Wambsganss +47 more
TL;DR: In this paper, the authors present the analysis of the planetary microlensing event OGLE-2014-BLG-1760, which shows a strong light curve signal due to the presence of a Jupiter mass-ratio planet.
Journal ArticleDOI
OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensing
P. Fouque,D. Heyrovsky,S. Dong,Andrew Gould,Andrzej Udalski,Michael D. Albrow,V. Batista,J. P. Beaulieu,D. P. Bennett,Ian A. Bond,D. M. Bramich,S. Calchi Novati,Arnaud Cassan,C. Coutures,S. Dieters,Martin Dominik,D. Dominis Prester,J. G. Greenhill,Keith Horne,U. G. Jørgensen,S. Kozlowski,D. Kubas,Chien-Hsiu Lee,J. B. Marquette,M. Mathiasen,J. W. Menzies,L. A. G. Monard,Shogo Nishiyama,I. E. Papadakis,R. Street,Takahiro Sumi,Andrew Williams,Jennifer C. Yee,Stephane Brillant,J. A. R. Caldwell,Andrew A. Cole,K. H. Cook,J. Donatowicz,N. Kains,S. R. Kane,R. M. Martin,K. R. Pollard,Kailash C. Sahu,Yiannis Tsapras,Joachim Wambsganss,M. Zub,Darren L. DePoy,B. S. Gaudi,C. Han,C.-U. Lee,Byeong-Gon Park,R. W. Pogge,M. Kubiak,Michał K. Szymański,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,K. Ulaczyk,L. Wyrzykowski,Fumio Abe,Akihiko Fukui,K. Furusawa,A. C. Gilmore,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,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,N. J. Rattenbury,To. Saito,Takashi Sako,Susumu Sato,L. Skuljan,D. J. Sullivan,Winston L. Sweatman,P. J. Tristram,P. C. M. Yock,Alasdair Allan,M. F. Bode,Martin Burgdorf,N. R. Clay,S. N. Fraser,E. Hawkins,Eamonn Kerins,T. A. Lister,C. J. Mottram,E. S. Saunders,Colin Snodgrass,Iain A. Steele,P. J. Wheatley,Timo Anguita,Valerio Bozza,Kasper Harpsøe,Tobias C. Hinse,M. Hundertmark,Per Kjaergaard,C. Liebig,Luigi Mancini,G. Masi,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,John Southworth,Jean Surdej,Christina C. Thöne,A. Riffeser,Stella Seitz,R. Bender +117 more
TL;DR: In the case of OGLE 2008-BLG-290, the K giant source star reached a peak magnification of about 100 as mentioned in this paper, and 13 different telescopes have covered this event in eight different photometric bands, and the best-measured coefficients lead to an estimate of the source effective temperature of about 4700 +100-200 K.
Journal ArticleDOI
Theory and practice of microlensing light curves around fold singularities
TL;DR: In this paper, a general, consistent and optimal choice of parameters provides a deep understanding of the involved features, avoids numerical difficulties and minimizes correlations between model parameters, while the photometric data of a microlensing event around a caustic passage itself do not provide constraints on the characteristics of the underlying binary lens and do not allow predictions of the behaviour of other regions of the light curve, vital constraints can be obtained in an efficient way if these are combined with a few simple characteristics of data outside the Caustic passages.