Institution
Vaughn College of Aeronautics and Technology
Education•New 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.
Papers published on a yearly basis
Papers
More filters
••
Las Cumbres Observatory Global Telescope Network1, Queen Mary University of London2, Chungbuk National University3, University of Salerno4, Ohio State University5, Institut d'Astrophysique de Paris6, University of Warsaw7, Niels Bohr Institute8, Osaka University9, European Southern Observatory10, Qatar Foundation11, University of St Andrews12, Max Planck Society13, Liverpool John Moores University14, Boston University15, University of Hamburg16, Heidelberg University17, National Academy of Sciences of Ukraine18, Geological Museum19, Korea Astronomy and Space Science Institute20, Armagh Observatory21, University of Manchester22, Pontifical Catholic University of Chile23, Sharif University of Technology24, International Institute of Minnesota25, Keele University26, University of Concepción27, University of Canterbury28, University of Toulouse29, Centre national de la recherche scientifique30, Goddard Space Flight Center31, University of Notre Dame32, University of Tasmania33, University of Rijeka34, University of Vienna35, San Francisco State University36, Texas A&M University37, Peking University38, Tel Aviv University39, Nagoya University40, Massey University41, University of Auckland42, Vaughn College of Aeronautics and Technology43, Victoria University of Wellington44, Kyoto Sangyo University45
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
••
Nagoya University1, University of Warsaw2, Osaka University3, University of Notre Dame4, Massey University5, Ohio State University6, University of Copenhagen7, University of Rijeka8, University of Canterbury9, University of Auckland10, Victoria University of Wellington11, National Institutes of Natural Sciences, Japan12, Vaughn College of Aeronautics and Technology13, University of Concepción14, University of Cambridge15, Chungbuk National University16, Texas A&M University17, University of California, Los Angeles18, Korea Astronomy and Space Science Institute19, Auckland University of Technology20, Tel Aviv University21, Qatar Foundation22, University of Salerno23, University of St Andrews24, University of Liège25, Heidelberg University26, Armagh Observatory27, University of Göttingen28, European Southern Observatory29, University of Manchester30, Max Planck Society31, Sharif University of Technology32, Perimeter Institute for Theoretical Physics33, Keele University34, Las Cumbres Observatory Global Telescope Network35, Liverpool John Moores University36, Queen Mary University of London37, Vienna University of Technology38, Space Telescope Science Institute39, University of Toulouse40, Institut d'Astrophysique de Paris41, Massachusetts Institute of Technology42, University of Tasmania43, University of Arizona44
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
••
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
••
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
••
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
Name | H-index | Papers | Citations |
---|---|---|---|
Xiang Zhang | 154 | 1733 | 117576 |
Denis J. Sullivan | 61 | 332 | 14092 |
To. Saito | 51 | 183 | 9392 |
Arthur H. Lefebvre | 41 | 123 | 4896 |
Michele Meo | 40 | 223 | 5557 |
Robin S. Langley | 40 | 263 | 5601 |
Ning Qin | 37 | 283 | 5011 |
Holger Babinsky | 33 | 242 | 4068 |
B. S. Gaudi | 31 | 64 | 2560 |
Philip J. Longhurst | 29 | 80 | 2578 |
Michael Gaster | 27 | 66 | 3998 |
Don Harris | 26 | 129 | 2537 |
To. Saito | 25 | 56 | 2362 |
John F. O'Connell | 22 | 89 | 1763 |
Rade Vignjevic | 21 | 84 | 1563 |