Institution
Pierre-and-Marie-Curie University
Education•Paris, France•
About: Pierre-and-Marie-Curie University is a education organization based out in Paris, France. It is known for research contribution in the topics: Population & Raman spectroscopy. The organization has 34448 authors who have published 56139 publications receiving 2392398 citations.
Topics: Population, Raman spectroscopy, Catalysis, Context (language use), Gene
Papers published on a yearly basis
Papers
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University of Birmingham1, University of Victoria2, University of Sydney3, INAF4, University of Liège5, Yale University6, International School for Advanced Studies7, Aarhus University8, Ohio State University9, Spanish National Research Council10, University of Amsterdam11, University of British Columbia12, Pierre-and-Marie-Curie University13, Max Planck Society14, Hungarian Academy of Sciences15, Ames Research Center16
TL;DR: In this article, the authors measured the masses of 40 stars on the RGB and 19 in the RC of the old metal-rich cluster NGC 6791 and showed that the difference between the average mass of RGB and RC stars is small but significant.
Abstract: Mass-loss of red giant branch (RGB) stars is still poorly determined, despite its crucial role in the chemical enrichment of galaxies. Thanks to the recent detection of solar-like oscillations in G–K giants in open clusters with Kepler, we can now directly determine stellar masses for a statistically significant sample of stars in the old open clusters NGC 6791 and 6819. The aim of this work is to constrain the integrated RGB mass-loss by comparing the average mass of stars in the red clump (RC) with that of stars in the low-luminosity portion of the RGB [i.e. stars with L L(RC)]. Stellar masses were determined by combining the available seismic parameters νmax and �ν with additional photometric constraints and with independent distance estimates. We measured the masses of 40 stars on the RGB and 19 in the RC of the old metal-rich cluster NGC 6791. We find that the difference between the average mass of RGB and RC stars is small, but significant [� M = 0.09 ± 0.03 (random) ±0.04 (systematic)
339 citations
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University of Washington1, University of Cambridge2, University of Leicester3, University of Lübeck4, University of Copenhagen5, University of Wisconsin–Milwaukee6, University of Michigan7, Montreal Heart Institute8, University of Oxford9, Broad Institute10, Samsung Medical Center11, University of Amsterdam12, Queen Mary University of London13, University of Göttingen14, University of Dundee15, University of Verona16, Vanderbilt University17, University of Kiel18, University of Bonn19, University of Basel20, Norwegian University of Science and Technology21, Umeå University22, University of Duisburg-Essen23, Technische Universität München24, University of Tartu25, Lund University26, University of Ottawa27, King Abdulaziz University28, Merck & Co.29, Ohio State University30, National Institutes of Health31, Johns Hopkins University32, Harvard University33, University of Insubria34, University of Glasgow35, Leiden University36, Queen's University Belfast37, Pierre-and-Marie-Curie University38, Wellcome Trust Sanger Institute39, University of Leeds40, Duke University41, University of Pennsylvania42
TL;DR: It was found that carriers of loss-of-function mutations in ANGPTL4 had triglyceride levels that were lower than those among noncarriers; these mutations were also associated with protection from coronary artery disease.
Abstract: BACKGROUND The discovery of low-frequency coding variants affecting the risk of coronary artery disease has facilitated the identification of therapeutic targets. METHODS Through DNA genotyping, we ...
339 citations
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TL;DR: The main objective of this work was to compare the structural and chemical characteristics of the isolated fractions and test models describing DOM reactivity toward metal ions, and showed significant structural differences between the three isolated fractions.
Abstract: Humic substances typically constitute 40-60% of the dissolved organic matter (DOM) in surface waters. However, little information is available regarding the metal binding properties of the nonhumic hydrophilic portion of the DOM. In this study, humic and nonhumic DOM samples were isolated from the South Platte River (Colorado, DOC = 2.6 mg x L(-1), SUVA254 = 2.4 L/mg x m) using a two-column array of XAD-8 and XAD-4 resins. The three major isolated fractions of DOM, which accounted for 57% of the bulk DOM,were characterized using a variety of analytical tools. Proton and copper binding properties were studied for each fraction. The main objective of this work was to compare the structural and chemical characteristics of the isolated fractions and test models describing DOM reactivity toward metal ions. The characterization work showed significant structural differences between the three isolated fractions of DOM. The hydrophobic acid fraction (i.e., humic substances isolated from the XAD-8 resin) gave the largest C/H, C/O, and C/N ratios and aromatic carbon content among the three isolated fractions. The transphilic acid (TPHA) fraction ("transphilic" meaning fraction of intermediate polarity isolated from the XAD-4 resin) was found to incorporate the highest proportion of polysaccharides, whereas the transphilic neutral (TPHN) fraction was almost entirely proteinaceous. The gradual increase of the charge with pH for the three DOM fractions is most likely caused by a large distribution of proton affinity constants for the carboxylic groups, as well as a second type of group more generally considered to be phenolic. In the case of the DOM fraction enriched in proteinaceous material (i.e., TPHN fraction), the results showed that the amino groups are responsible for the charge reversal. For low copper concentrations, nitrogen-containing functional groups similar to those of amino acids are likely to be involved in complexation, in agreement with previously published data.
338 citations
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TL;DR: IL-17, like other cytokines, appears to be a pleiotropic cytokine with possible protumor or antitumor effects on tumor development, which often depends on the immunogenicity of tumor models.
338 citations
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TL;DR: In this paper, a new method for analyzing directed and elliptic flow in heavy-ion collisions is presented, which separates the contribution of flow to azimuthal correlations from contributions due to other effects.
Abstract: We present a new method for analyzing directed and elliptic flow in heavy-ion collisions. Unlike standard methods, it separates the contribution of flow to azimuthal correlations from contributions due to other effects. The separation relies on a cumulant expansion of multiparticle azimuthal correlations, and includes corrections for detector inefficiencies. This new method allows the measurement of the flow of identified particles in narrow phase-space regions, and can be used in every regime, from intermediate to ultrarelativistic energies.
338 citations
Authors
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Name | H-index | Papers | Citations |
---|---|---|---|
Zhong Lin Wang | 245 | 2529 | 259003 |
Guido Kroemer | 236 | 1404 | 246571 |
Krzysztof Matyjaszewski | 169 | 1431 | 128585 |
J. E. Brau | 162 | 1949 | 157675 |
E. Hivon | 147 | 403 | 118440 |
Kazuhiko Hara | 141 | 1956 | 107697 |
Simon Prunet | 141 | 434 | 96314 |
H. J. McCracken | 140 | 579 | 71091 |
G. Calderini | 139 | 1734 | 102408 |
Stefano Giagu | 139 | 1651 | 101569 |
Jean-Paul Kneib | 138 | 805 | 89287 |
G. Marchiori | 137 | 1590 | 94277 |
J. Ocariz | 136 | 1562 | 95905 |
Jean-Marie Tarascon | 136 | 853 | 137673 |
Alexis Brice | 135 | 870 | 83466 |