M
M. Nola
Publications - 6
Citations - 173
M. Nola is an academic researcher. The author has contributed to research in topics: Gravitational microlensing & Planetary system. The author has an hindex of 6, co-authored 6 publications receiving 172 citations.
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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
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,To. Saito,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,Grzegorz Pietrzyński,Łukasz Wyrzykowski,Łukasz Wyrzykowski,J.-Y. Choi,G. W. Christie,Darren L. DePoy,Subo Dong,Jack D. Drummond,B. S. Gaudi,Chang S. Han,Li-Wei Hung,Li-Wei Hung,K.-H. Hwang,C.-U. Lee,Jennie McCormick,D. Moorhouse,Tim Natusch,M. Nola,Eran O. Ofek,Richard W. Pogge,In-Gu Shin,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,Tobias C. Hinse,Tobias C. Hinse,M. Hundertmark,M. Hundertmark,N. Kains,N. Kains,Eamonn Kerins,C. Liebig,C. Liebig,Luigi Mancini,Luigi Mancini,M. Mathiasen,Matthew T. Penny,Matthew T. Penny,S. Proft,Sohrab Rahvar,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,Yiannis Tsapras,Keith Horne,J. Donatowicz,Kailash C. Sahu,Etienne Bachelet,V. Batista,V. Batista,Thomas G. Beatty,J. P. Beaulieu,C. S. Bennett,Christine S. Black,R. Bowens-Rubin,S. 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,D. Kubas,J. B. Marquette,R. Martin,J. W. Menzies,B. J. Shappee,Andrew Williams,D. Wouters,J. van Saders,Robert T. Zellem,M. Zub +133 more
TL;DR: In this paper, 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 parlax.
Journal ArticleDOI
MOA-2010-BLG-311: A planetary candidate below the threshold of reliable detection
Jennifer C. Yee,Li-Wei Hung,Li-Wei Hung,Ian A. Bond,William H. Allen,L. A. G. Monard,Michael D. Albrow,Pascal Fouqué,Martin Dominik,Yiannis Tsapras,Yiannis Tsapras,Andrzej Udalski,Andrew Gould,Robert T. Zellem,M. Bos,G. W. Christie,Darren L. DePoy,Subo Dong,Jack D. Drummond,B. S. Gaudi,Evgeny Gorbikov,C. Han,Shai Kaspi,N. Klein,C.-U. Lee,D. Maoz,Jennie McCormick,D. Moorhouse,Tim Natusch,M. Nola,Byeong-Gon Park,R. W. Pogge,David Polishook,Avi Shporer,Yossi Shvartzvald,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,Takahiro Sumi,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,Grzegorz Pietrzyński,Łukasz Wyrzykowski,Łukasz Wyrzykowski,Etienne Bachelet,V. Batista,V. Batista,Thomas G. Beatty,J. P. Beaulieu,C. S. Bennett,R. Bowens-Rubin,S. Brillant,J. A. R. Caldwell,Arnaud Cassan,Andrew A. Cole,E. Corrales,C. Coutures,S. Dieters,D. Dominis Prester,J. Donatowicz,J. G. Greenhill,Calen B. Henderson,D. Kubas,D. Kubas,J. B. Marquette,R. Martin,J. W. Menzies,Benjamin J. Shappee,Andrew Williams,D. Wouters,J. van Saders,M. Zub,Rachel Street,Keith Horne,D. M. Bramich,Iain A. Steele,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,François Finet,T. Gerner,S. Hardis,K. B. W. Harpsøe,Frederic V. Hessman,Tobias C. Hinse,Tobias C. Hinse,Tobias C. Hinse,M. Hundertmark,M. Hundertmark,U. G. Jørgensen,N. Kains,Eamonn Kerins,C. Liebig,C. Liebig,Luigi Mancini,Luigi Mancini,M. Mathiasen,Matthew T. Penny,Matthew T. Penny,S. Proft,Sohrab Rahvar,Sohrab Rahvar,Davide Ricci,Kailash C. Sahu,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,Colin Snodgrass,John Southworth,Jean Surdej,Joachim Wambsganss +139 more
TL;DR: In this paper, the authors analyzed MOA-2010-BLG-311, a high magnification (A max > 600) microlensing event with complete data coverage over the peak, making it very sensitive to planetary signals.
Journal ArticleDOI
MOA-2010-BLG-311: A planetary candidate below the threshold of reliable detection
Jennifer C. Yee,Li-Wei Hung,Ian A. Bond,William H. Allen,L. A. G. Monard,Michael D. Albrow,P. Fouque,Martin Dominik,Yiannis Tsapras,Andrzej Udalski,Andrew Gould,Robert T. Zellem,M. Bos,G. W. Christie,Darren L. DePoy,Subo Dong,Jack D. Drummond,B. S. Gaudi,Evgeny Gorbikov,C. Han,Shai Kaspi,N. Klein,C.-U. Lee,D. Maoz,Jennie McCormick,D. Moorhouse,Tim Natusch,M. Nola,Byeong-Gon Park,R. W. Pogge,David Polishook,Avi Shporer,Yossi Shvartzvald,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,Philip Yock,Michał K. Szymański,Igor Soszyński,M. Kubiak,Radosław Poleski,Krzysztof Ulaczyk,Grzegorz Pietrzyński,L. Wyrzykowski,Etienne Bachelet,V. Batista,Thomas G. Beatty,J. P. Beaulieu,C. S. Bennett,R. Bowens-Rubin,Stephane Brillant,J. A. R. Caldwell,Arnaud Cassan,Andrew A. Cole,E. Corrales,C. Coutures,S. Dieters,D. Dominis Prester,J. Donatowicz,J. G. Greenhill,Calen B. Henderson,D. Kubas,J. B. Marquette,R. Martin,J. W. Menzies,Benjamin J. Shappee,Andrew Williams,D. Wouters,J. van Saders,M. Zub,Rachel Street,Keith Horne,D. M. Bramich,Iain A. Steele,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,François Finet,T. Gerner,S. Hardis,K. B. W. Harpsøe,F. V. Hessman,Tobias C. Hinse,M. Hundertmark,U. G. Jørgensen,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,J. Wambsganß +125 more
TL;DR: In this paper, the authors analyzed MOA-2010-BLG-311, a high magnification (A_max>600) microlensing event with complete data coverage over the peak, making it very sensitive to planetary signals.
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.