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Institution

Vaughn College of Aeronautics and Technology

EducationNew York, New York, United States
About: Vaughn College of Aeronautics and Technology is a education organization based out in New York, New York, United States. It is known for research contribution in the topics: Gravitational microlensing & Planetary system. The organization has 727 authors who have published 708 publications receiving 14082 citations. The organization is also known as: College of Aeronautics.


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Journal ArticleDOI
Yiannis Tsapras1, Yiannis Tsapras2, J.-Y. Choi3, Rachel Street1, C. Han3, Valerio Bozza4, Andrew Gould5, Martin Dominik, J. P. Beaulieu6, Andrzej Udalski7, U. G. Jørgensen8, Takahiro Sumi9, D. M. Bramich10, D. M. Bramich11, P. Browne12, Keith Horne12, M. Hundertmark12, Sergei I. Ipatov11, N. Kains10, Colin Snodgrass13, Iain A. Steele14, Khalid Al-Subai11, J. M. Andersen15, S. Calchi Novati4, Yassine Damerdji, C. Diehl16, C. Diehl17, Andrii Elyiv18, E. Giannini17, S. Hardis8, K. B. W. Harpsøe19, Tobias C. Hinse20, Tobias C. Hinse21, Tobias C. Hinse8, Diana Juncher8, Eamonn Kerins22, Heidi Korhonen8, C. Liebig12, Luigi Mancini13, M. Mathiasen8, Matthew T. Penny5, Markus Rabus23, Sohrab Rahvar24, Gaetano Scarpetta25, Gaetano Scarpetta4, Jesper Skottfelt19, Jesper Skottfelt8, John Southworth26, Jean Surdej, J. Tregloan-Reed26, C. Vilela26, Joachim Wambsganss17, Jan Skowron7, Radosław Poleski7, Radosław Poleski5, S. Kozllowski7, E. Wyrzykowski5, E. Wyrzykowski7, Michał K. Szymański7, M. Kubiak7, P. Pietrukowicz7, Grzegorz Pietrzyński7, Grzegorz Pietrzyński27, Igor Soszyński7, Krzysztof Ulaczyk7, Michael D. Albrow28, Etienne Bachelet29, Etienne Bachelet30, Richard K. Barry31, V. Batista6, Aparna Bhattacharya32, S. Brillant10, J. A. R. Caldwell, Arnaud Cassan6, Andrew A. Cole33, E. Corrales6, Ch. Coutures6, S. Dieters29, D. Dominis Prester34, J. Donatowicz35, Pascal Fouqué29, Pascal Fouqué30, J. G. Greenhill33, Stephen R. Kane36, D. Kubas6, D. Kubas10, J. B. Marquette6, J. W. Menzies, C. P. Ere6, C. P. Ere10, K. R. Pollard28, M. Zub17, G. W. Christie, Darren L. DePoy37, S. Dong38, Jack D. Drummond, B. S. Gaudi5, Calen B. Henderson5, K.-H. Hwang3, Youn Kil Jung3, A. Kavka5, J.-R. Koo20, C.-U. Lee20, D. Maoz39, L. A. G. Monard, Tim Natusch, H. Ngan, H. Park3, R. W. Pogge5, I. Porritt, In-Gu Shin3, Yossi Shvartzvald39, Thiam-Guan Tan, Jennifer C. Yee5, Fumio Abe40, David P. Bennett32, Ian A. Bond41, C. S. Botzler42, M. Freeman42, Akihiko Fukui, D. Fukunaga40, Yoshitaka Itow40, Naoki Koshimoto9, C. H. Ling41, Kimiaki Masuda40, Yutaka Matsubara40, Yasushi Muraki40, S. Namba9, K. Ohnishi, Nicholas J. Rattenbury42, To. Saito43, Denis J. Sullivan44, Winston L. Sweatman41, Daisuke Suzuki9, P. J. Tristram, N. Tsurumi40, K. Wada9, N. Yamai45, P. C. M. Yock42, Atsunori Yonehara45 
TL;DR: In this paper, a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories is presented.
Abstract: We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the light curve, especially the perturbation part, allowed us to accurately measure the parallax effect and lens orbital motion. Combining our measurement of the lens parallax with the angular Einstein radius determined from finite-source effects, we estimate the physical parameters of the lens system. We find that the event was caused by a 2.73 ± 0.43 M J planet orbiting a 0.44 ± 0.07 M ☉ early M-type star. The distance to the lens is 4.97 ± 0.29 kpc and the projected separation between the host star and its planet at the time of the event is 3.45 ± 0.26 AU. We find that the additional coverage provided by follow-up observations, especially during the planetary perturbation, leads to a more accurate determination of the physical parameters of the lens.

36 citations

Journal ArticleDOI
K. Furusawa1, Andrzej Udalski2, Takahiro Sumi3, David P. Bennett4, Ian A. Bond5, Andrew Gould6, U. G. Jørgensen7, Colin Snodgrass, D. Dominis Prester8, Michael D. Albrow9, Fumio Abe1, C. S. Botzler10, P. Chote11, M. Freeman10, Akihiko Fukui12, P. Harris11, Yoshitaka Itow1, C. H. Ling5, Kimiaki Masuda1, Yutaka Matsubara1, N. Miyake1, Yasushi Muraki1, Kouji Ohnishi, Nicholas J. Rattenbury10, To. Saito13, Denis J. Sullivan11, Daisuke Suzuki3, Winston L. Sweatman5, Paul J. Tristram, K. Wada3, Philip Yock10, Michał K. Szymański2, Igor Soszyński2, M. Kubiak2, Radosław Poleski2, Krzysztof Ulaczyk2, Grzegorz Pietrzyński14, Grzegorz Pietrzyński2, Łukasz Wyrzykowski2, Łukasz Wyrzykowski15, J.-Y. Choi16, G. W. Christie, Darren L. DePoy17, Subo Dong, Jack D. Drummond, B. S. Gaudi6, Chang S. Han16, Li-Wei Hung18, Li-Wei Hung6, K.-H. Hwang16, C.-U. Lee19, Jennie McCormick, D. Moorhouse, Tim Natusch20, M. Nola, Eran O. Ofek21, Richard W. Pogge6, In-Gu Shin16, Jan Skowron6, G. Thornley, Jennifer C. Yee6, Khalid Al-Subai22, Valerio Bozza23, P. Browne24, Martin Burgdorf, S. Calchi Novati23, Peter N. Dodds24, Martin Dominik24, François Finet25, T. Gerner26, S. Hardis7, K. B. W. Harpsøe7, Tobias C. Hinse19, Tobias C. Hinse27, Tobias C. Hinse7, M. Hundertmark28, M. Hundertmark24, N. Kains29, N. Kains24, Eamonn Kerins30, C. Liebig26, C. Liebig24, Luigi Mancini31, Luigi Mancini23, M. Mathiasen7, Matthew T. Penny30, Matthew T. Penny6, S. Proft26, Sohrab Rahvar32, Sohrab Rahvar33, Davide Ricci25, Gaetano Scarpetta23, S. Schäfer28, F. Schönebeck26, John Southworth34, Jean Surdej28, Joachim Wambsganss26, Rachel Street35, D. M. Bramich29, Iain A. Steele36, Yiannis Tsapras37, Yiannis Tsapras35, Keith Horne24, J. Donatowicz38, Kailash C. Sahu39, Etienne Bachelet40, V. Batista6, V. Batista41, Thomas G. Beatty6, J. P. Beaulieu41, C. S. Bennett42, Christine S. Black43, R. Bowens-Rubin42, S. Brillant29, J. A. R. Caldwell, Arnaud Cassan41, Andrew A. Cole43, E. Corrales41, C. Coutures41, S. Dieters43, P. Fouqué40, J. G. Greenhill43, Calen B. Henderson6, D. Kubas41, D. Kubas29, J. B. Marquette41, R. Martin, J. W. Menzies, B. J. Shappee6, Andrew Williams, D. Wouters, J. van Saders6, Robert T. Zellem44, M. Zub25 
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.
Abstract: We analyze the planetary microlensing event MOA-2010-BLG-328 The best fit yields host and planetary masses of M h = 011 ± 001 M ☉ and M p = 92 ± 22 M ⊕, corresponding to a very late M dwarf and sub-Neptune-mass planet, respectively The system lies at D L = 081 ± 010 kpc with projected separation r ⊥ = 092 ± 016 AU Because of the host's a priori unlikely close distance, as well as the unusual nature of the system, we consider the possibility 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 parallax We show a result that favors the parallax solution, even given its close host distance We show that future high-resolution astrometric measurements could decisively resolve the remaining ambiguity of these solutions

36 citations

Journal ArticleDOI
TL;DR: In this article, an analytical solution for the natural frequencies, mode shapes and orthogonality condition, of a free-free beam with large offset masses connected to the beam by torsion springs is presented.

35 citations

Journal ArticleDOI
TL;DR: In this paper, a surface ablation model considering the oxidation and sublimation ablation process is coupled with a Navier-Stokes solver by a gas-solid interaction method to simulate the ablation plasma flows.

35 citations

Journal ArticleDOI
TL;DR: The nonclassical reduction of the Navier-Stokes equations of fluid mechanics has been applied to a system of partial differential equations, yielding reduced sets of equations with one fewer independent variables as discussed by the authors.
Abstract: The nonclassical reduction method as pioneered by Bluman and Cole ( J. Meth. Mech. 18 1025-42) is used to examine symmetries of the full three-dimensional, unsteady, incompressible Navier-Stokes equations of fluid mechanics. The procedure, when applied to a system of partial differential equations, yields reduced sets of equations with one fewer independent variables. We find eight possibilities for reducing the Navier-Stokes equations in the three spatial and one temporal dimensions to sets of partial differential equations in three independent variables. Some of these reductions are derivable using the Lie-group method of classical symmetries but the remainder are genuinely nonclassical. Further investigations of one of our eight forms shows how it is possible to derive novel exact solutions of the Navier-Stokes equations by the nonclassical method.

35 citations


Authors

Showing all 732 results

NameH-indexPapersCitations
Xiang Zhang1541733117576
Denis J. Sullivan6133214092
To. Saito511839392
Arthur H. Lefebvre411234896
Michele Meo402235557
Robin S. Langley402635601
Ning Qin372835011
Holger Babinsky332424068
B. S. Gaudi31642560
Philip J. Longhurst29802578
Michael Gaster27663998
Don Harris261292537
To. Saito25562362
John F. O'Connell22891763
Rade Vignjevic21841563
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20236
20223
202145
202033
201934
201841