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.
Papers
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Journal ArticleDOI
OGLE-2015-BLG-0479LA,B: Binary Gravitational Microlens Characterized by Simultaneous Ground-based and Space-based Observation
C. Han,Andrzej Udalski,Andrew Gould,Wei Zhu,R. A. Street,Jennifer C. Yee,C. A. Beichman,C. Bryden,S. Calchi Novati,Sean Carey,Michael Fausnaugh,B. S. Gaudi,Calen B. Henderson,Yossi Shvartzvald,B. Wibking,Michał K. Szymański,Igor Soszyński,Jan Skowron,P. Mróz,R. Poleski,P. Pietrukowicz,S. Kozlowski,K. Ulaczyk,Łukasz Wyrzykowski,Michał Pawlak,Yiannis Tsapras,M. Hundertmark,Etienne Bachelet,Martin Dominik,D. M. Bramich,Arnaud Cassan,R. Figuera Jaimes,Keith Horne,C. Ranc,R. W. Schmidt,Colin Snodgrass,Joachim Wambsganss,Iain A. Steele,J. W. Menzies,Shude Mao,V. Bozza,U. G. Jørgensen,Khalid Al-Subai,Simona Ciceri,Giuseppe D'Ago,Troels Haugbølle,F. V. Hessman,Tobias C. Hinse,Diana Juncher,Heidi Korhonen,L. Mancini,A. Popovas,M. Rabus,S. Rahvar,Gaetano Scarpetta,J. Skottfelt,John Southworth,D. A. Starkey,Jean Surdej,Olivier Wertz,M. Zarucki,R. W. Pogge,Darren L. DePoy +62 more
TL;DR: In this paper, a combined analysis of the observations of the OGLE-2015-BLG-0479 taken both from the ground and by the Spitzer Space Telescope is presented.
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Microlensing events by proxima centauri in 2014 and 2016: Opportunities for mass determination and possible planet detection
TL;DR: In this article, it was shown that Proxima Centauri will pass close to a pair of faint background stars in the next few years and the relativistic deflection of light will cause shifts in the positions of the background stars of ∼0.5 and 1.5 mas, respectively.
Journal ArticleDOI
Microlensing binaries discovered through high-magnification channel
In-Gu Shin,J.-Y. Choi,S.-Y. Park,Chang S. Han,Andrew Gould,Takahiro Sumi,Andrzej Udalski,J. P. Beaulieu,Martin Dominik,William H. Allen,M. Bos,G. W. Christie,Darren L. DePoy,Subo Dong,Jack D. Drummond,Avishay Gal-Yam,B. S. Gaudi,Li-Wei Hung,J. Janczak,Shai Kaspi,C.-U. Lee,F. Mallia,D. Maoz,Alain Maury,Jennie McCormick,L. A. G. Monard,D. Moorhouse,J. A. Muñoz,Tim Natusch,C. Nelson,Byeong-Gon Park,Richard W. Pogge,David Polishook,Yossi Shvartzvald,Avi Shporer,G. Thornley,Jennifer C. Yee,Fumio Abe,David P. Bennett,Ian A. Bond,C. S. Botzler,Akihiko Fukui,K. Furusawa,F. Hayashi,John B. Hearnshaw,S. Hosaka,Yoshitaka Itow,Kisaku Kamiya,P. M. Kilmartin,S. Kobara,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,K. Omori,Y. C. Perrott,Nicholas J. Rattenbury,To. Saito,L. Skuljan,Denis J. Sullivan,Daisuke Suzuki,Winston L. Sweatman,P. J. Tristram,K. Wada,Philip Yock,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,Radosław Poleski,Krzysztof Ulaczyk,Łukasz Wyrzykowski,Łukasz Wyrzykowski,S. Kozlowski,P. Pietrukowicz,Michael D. Albrow,V. Batista,D. M. Bramich,S. Brillant,J. A. R. Caldwell,J. J. Calitz,Arnaud Cassan,Andrew A. Cole,K. H. Cook,E. Corrales,Ch. Coutures,S. Dieters,S. Dieters,D. Dominis Prester,J. Donatowicz,Pascal Fouqué,J. G. Greenhill,M. Hoffman,U. G. Jørgensen,U. G. Jørgensen,S. R. Kane,D. Kubas,D. Kubas,J. B. Marquette,R. M. Martin,P. J. Meintjes,J. W. Menzies,K. R. Pollard,Kailash C. Sahu,Joachim Wambsganss,Andrew Williams,C. Vinter,M. Zub,Alasdair Allan,P. Browne,Keith Horne,Colin Snodgrass,Colin Snodgrass,Iain A. Steele,Rachel Street,Yiannis Tsapras,Khalid Al-Subai,Valerio Bozza,Martin Burgdorf,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Stefan Dreizler,François Finet,T. Gerner,M. Glitrup,Frank Grundahl,S. Hardis,K. B. W. Harpsøe,K. B. W. Harpsøe,Frederic V. Hessman,Tobias C. Hinse,Tobias C. Hinse,Tobias C. Hinse,M. Hundertmark,M. Hundertmark,N. Kains,Eamonn Kerins,C. Liebig,C. Liebig,G. Maier,Luigi Mancini,Luigi Mancini,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,Jesper Skottfelt,Jean Surdej,John Southworth,F. Zimmer +163 more
TL;DR: In this paper, the light curves of eight binary-lensing events detected through the channel of high-magnification events during the seasons from 2007 to 2010 were analyzed, and the dependence of the degeneracy on the lensing parameters was consistent with a theoretical prediction that the degeneration becomes severe as the binary separation and the mass ratio deviate from the values of resonant caustics.
Journal ArticleDOI
Probing MACHOs by observation of M31 pixel lensing with the 1.5m Loiano telescope
S. Calchi Novati,Giovanni Covone,F. De Paolis,Martin Dominik,Y. Giraud-Heraud,G. Ingrosso,Ph. Jetzer,Luigi Mancini,A. A. Nucita,Gaetano Scarpetta,Francesco Strafella,Andrew Gould +11 more
TL;DR: In this paper, a series of pilot observations in order to study microlensing of (unresolved) stars in M31 with the 1.5m Loiano telescope, including observations on both identified variable source stars and reported micro-lensing events, were analyzed.
Journal ArticleDOI
MOA-2010-BLG-523: "Failed Planet" = RS CVn Star
Andrew Gould,Jennifer C. Yee,Ian A. Bond,Andrzej Udalski,C. Han,U. G. Jørgensen,J. G. Greenhill,Yiannis Tsapras,Marc H. Pinsonneault,Thomas Bensby,William H. Allen,Leonardo A. Almeida,M. Bos,G. W. Christie,Darren L. DePoy,Subo Dong,B. S. Gaudi,Li-Wei Hung,Francisco Jablonski,C.-U. Lee,Jennie McCormick,D. Moorhouse,J. A. Muñoz,Tim Natusch,M. Nola,Richard W. Pogge,Jan Skowron,G. Thornley,Fumio Abe,David P. Bennett,C. S. Botzler,P. Chote,M. Freeman,Akihiko Fukui,K. Furusawa,P. Harris,Yoshitaka Itow,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Kouji Ohnishi,Nicholas J. Rattenbury,To. Saito,Denis J. Sullivan,Takahiro Sumi,Daisuke Suzuki,Winston L. Sweatman,Paul J. Tristram,K. Wada,P. C. M. Yock,Michał K. Szymański,Igor Soszyński,M. Kubiak,Radosław Poleski,Krzysztof Ulaczyk,Grzegorz Pietrzyński,L. Wyrzykowski,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,F. V. Hessman,Tobias C. Hinse,M. Hundertmark,N. Kains,Eamonn Kerins,C. Liebig,Luigi Mancini,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Kailash C. Sahu,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,Colin Snodgrass,John Southworth,Jean Surdej,Joachim Wambsganss,Rachel Street,Keith Horne,D. M. Bramich,Iain A. Steele,Michael D. Albrow,Etienne Bachelet,V. Batista,Thomas G. Beatty,J. P. Beaulieu,C. S. Bennett,R. Bowens-Rubin,Stephane Brillant,John A. R. Caldwell,Arnaud Cassan,Andrew A. Cole,E. Corrales,C. Coutures,S. Dieters,D. Dominis Prester,J. Donatowicz,P. Fouque,Calen B. Henderson,D. Kubas,J. B. Marquette,R. Martin,J. W. Menzies,Benjamin J. Shappee,Andrew Williams,J. van Saders,M. Zub +118 more
TL;DR: In this article, the authors combine long-term photometric monitoring with a previously published high-resolution spectrum taken near peak to demonstrate that this is an RS CVn variable, so that planetary microlensing is not required to explain the lightcurve deviations.