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Institution

National Science Foundation

GovernmentAlexandria, Virginia, United States
About: National Science Foundation is a government organization based out in Alexandria, Virginia, United States. It is known for research contribution in the topics: Galaxy & Population. The organization has 4729 authors who have published 6040 publications receiving 298150 citations. The organization is also known as: NSF & N.S.F..
Topics: Galaxy, Population, Stars, LIGO, Gravitational wave


Papers
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Journal ArticleDOI
TL;DR: The first transneptunian object known to be on a retrograde orbit was reported in this paper, which was made during an outer solar system survey using the Canada-France-Hawaii Telescope (CFHT).
Abstract: We report the discovery of the first transneptunian object known to be on a retrograde orbit. The discovery was made during an outer solar system survey using the Canada–France–Hawaii Telescope (CFHT). After recovery observations on the MMT, CTIO-Blanco, Gemini-South, and CFHT telescopes, we can state with certainty that the object is both transneptunian and orbits the Sun in a retrograde sense, with an orbital inclination i = 104 deg. The object has IAU Minor Planet Center provisional designation 2008 KV42 and temporary nickname “Drac.” Numerical integration of a set of initial states consistent with the astrometry shows that the semimajor axis is a � 42 AU, the perihelion distance is q ∼21 AU, and that the object’s orbit evolves on ∼30 million year timescales via gravitational encounters with Uranus and Neptune. The object is unlikely to be primordial and thus needs a supply mechanism from a long-lived source. We outline several scenarios which could have emplaced the object on its current orbit, including a currently unobserved reservoir of large-inclination orbits beyond Neptune which may also supply the Halley-type comets.

82 citations

Journal ArticleDOI
TL;DR: In this article, the CTIO Argus multi-fiber system was used to detect giant star members of distant globular clusters Reticulum (C0435 -590) and NGC 1841 (C0444-840) based on spectroscopy with CTIOArgus.
Abstract: Velocities and metallicities for giant star members of the distant globular clusters Reticulum (C0435 -590) and NGC 1841 (C0444-840) based on spectroscopy with the CTIO Argus multi-fiber system show that these two clusters are likely members of the Large Magellanic Cloud (LMC). The velocity, [Fe/H] metallicity, and absolute visual magnitude for Reticulum are 241.5±1.5 km s −1 , −1.71, and −6.0±0,2, and for NGC 1841, 212.5±1.8 km s −1 , −2.11, and −7.9±0.2

82 citations

Journal ArticleDOI
TL;DR: In this paper, a comparison of the locations of the optical components of the rado-binary Wolf-Rayet stars WR 146 and WR 147 with high-resolution radio maps strikingly demonstrates that the nonthermal radio components arise between the optical binary components, closer to the OB component than the WR.
Abstract: Hubble Space Telescope (HST) Wide Field Planetary Camera 2 images of the rado-binary Wolf-Rayet stars WR 146 and WR 147, as well as the 02 visual binary WR 86, resolve each of them into two very close optical components. The colors of these optical pairs are similar, indicating that they are likely to be physically bound WR + OB systems at the same distance. Comparison of the locations of the optical components of WR 146 and WR 147 with high-resolution radio maps strikingly demonstrates that the nonthermal radio components arise between the optical binary components, closer to the OB component than the WR. This is as expected if the nonthermal radio emission results from the collision of the stellar winds of the binary components seen in the HST images. The similar magnitudes and colors determined for the components of WR 86 from our HST images, combined with an analysis of the unresolved, combined WC7 + OB optical spectrum, indicates an absolute magnitude for the WC7 component of about MV ~ -5.

82 citations

Journal ArticleDOI
TL;DR: It is demonstrated that sampling with synthesis can improve the quality of public use data relative to sampling followed by standard statistical disclosure limitation, and is illustrated on a population constructed with data from the U.S. Current Population Survey.
Abstract: Many statistical agencies disseminate samples of census microdata, that is, data on individual records, to the public. Before releasing the microdata, agencies typically alter identifying or sensitive values to protect data subjects’ confidentiality, for example by coarsening, perturbing, or swapping data. These standard disclosure limitation techniques distort relationships and distributional features in the original data, especially when applied with high intensity. Furthermore, it can be difficult for analysts of the masked public use data to adjust inferences for the effects of the disclosure limitation. Motivated by these shortcomings, we propose an approach to census microdata dissemination called sampling with synthesis. The basic idea is to replace the identifying or sensitive values in the census with multiple imputations, and release samples from these multiply-imputed populations. We demonstrate that sampling with synthesis can improve the quality of public use data relative to sampling followe...

82 citations


Authors

Showing all 4739 results

NameH-indexPapersCitations
Jie Zhang1784857221720
George M. Church172900120514
Timothy M. Heckman170754141237
Timothy C. Beers156934102581
Xiang Zhang1541733117576
Ian Smail15189583777
Robert Plomin151110488588
James M. Tiedje150688102287
Rajesh Kumar1494439140830
Charles C. Steidel14148672242
R. L. McCarthy1411238115696
Barry Blumenfeld1401909105694
Yasushi Fukazawa13588264424
Lee Hartmann13457957649
Jean-Luc Brédas134102685803
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20233
202211
2021150
2020168
2019173
2018164