Institution
University of Notre Dame
Education•Notre Dame, Indiana, United States•
About: University of Notre Dame is a education organization based out in Notre Dame, Indiana, United States. It is known for research contribution in the topics: Population & Context (language use). The organization has 22238 authors who have published 55201 publications receiving 2032925 citations. The organization is also known as: University of Notre Dame du Lac & University of Notre Dame, South Bend.
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TL;DR: Key aspects of microbial traits are reviewed and a synthesis of these studies reveals that, despite the promiscuity of HGT, microbial traits appear to be phylogenetically conserved, or not distributed randomly across the tree of life.
Abstract: A focus on the phenotypic characteristics of microorganisms-their traits-offers a path for interpreting the growing amount of microbiome data. We review key aspects of microbial traits, as well as approaches used to assay their phylogenetic distribution. Recent studies reveal that microbial traits are differentially conserved across the tree of life and appear to be conserved in a hierarchical fashion, possibly linked to their biochemical complexity. These results suggest a predictive framework whereby the genetic (or taxonomic) resolution of microbiome variation among samples provides information about the traits under selection. The organizational parallels seen among human and free-living microbiomes seem to support this idea. Developments in this framework may offer predictions not only for how microbial composition responds to changing environmental conditions, but also for how these changes may alter the health or functioning in human, engineered, and environmental systems.
584 citations
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TL;DR: In this paper the control of linear plants, where the sensor is connected to a linear controller/actuator via a network through a network is addressed, both, state and output feedback are considered and results are derived for both continuous and discrete plants.
584 citations
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TL;DR: The central objective of developing this typology was to develop a classification system that would be useful to researchers from various disciplinary perspectives such that the classification system might be used as a foundation for theory construction.
Abstract: Despite the growing popularity of virtual communities, there is no consensus among researchers regarding the appropriate definition or types of virtual communities. In this paper, a virtual community is defined as an aggregation of individuals or business partners who interact around a shared interest, where the interaction is at least partially supported and/or mediated by technology and guided by some protocols or norms. The central objective of developing this typology was to develop a classification system that would be useful to researchers from various disciplinary perspectives such that the classification system might be used as a foundation for theory construction. The proposed typology serves its intended purposes and is evaluated against criteria put forth by Hunt (1991). The proposed typology uses establishment type and relationship orientation as the key categorization variables, reconciling problems posed by other researchers who attempt to use attributes as categorization variables. It is simple, pragmatic for practitioners and useful for researchers seeking to develop an understanding of the virtual community phenomenon.
584 citations
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TL;DR: In this article, the authors study the panel DOLS estimator of a homogeneous cointegration vector for a balanced panel of N individuals observed over T time periods and find that the estimator is fully parametric, computationally convenient, and more precise than the single equation estimator.
Abstract: We study the panel DOLS estimator of a homogeneous cointegration vector for a balanced panel of N individuals observed over T time periods. Allowable heterogeneity across individuals include individual-specific time trends, individual-specific fixed effects and time-specific effects. The estimator is fully parametric, computationally convenient, and more precise than the single equation estimator. For fixed N as T approaches infinity, the estimator converges to a function of Brownian motions and the Wald statistic for testing a set of linear constraints has a limiting chi-square distribution. The estimator also has a Gaussian sequential limit distribution that is obtained first by letting T go to infinity then letting N go to infinity. In a series of Monte Carlo experiments, we find that the asymptotic distribution theory provides a reasonably close approximation to the exact finite sample distribution. We use panel dynamic OLS to estimate coefficients of the long-run money demand function from a panel of 19 countries with annual observations that span from 1957 to 1996. The estimated income elasticity is 1.08 (asymptotic s.e.=0.26) and the estimated interest rate semi-elasticity is -0.02 (asymptotic s.e.=0.01).
582 citations
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Carnegie Institution for Science1, University of California, Santa Cruz2, Carnegie Learning3, University of California, Berkeley4, Lawrence Berkeley National Laboratory5, Pennsylvania State University6, University of Copenhagen7, Johns Hopkins University8, Space Telescope Science Institute9, California Institute of Technology10, Diego Portales University11, Massachusetts Institute of Technology12, Joint Institute for Nuclear Astrophysics13, University of Notre Dame14, National Autonomous University of Mexico15, University of La Serena16, University of Victoria17, Herzberg Institute of Astrophysics18, Valparaiso University19, Texas A&M University20, Catholic University of the North21, Millennium Institute22, University of Sydney23
TL;DR: In this paper, the authors present ultraviolet, optical, and infrared light curves of SSS17a extending from 10.9 hours to 18 days post-merger, showing that the late-time light curve indicates that SSS 17a produced at least 0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
Abstract: On 17 August 2017, gravitational waves (GWs) were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB 170817A. An optical transient source, Swope Supernova Survey 17a (SSS17a), was subsequently identified as the counterpart of this event. We present ultraviolet, optical, and infrared light curves of SSS17a extending from 10.9 hours to 18 days postmerger. We constrain the radioactively powered transient resulting from the ejection of neutron-rich material. The fast rise of the light curves, subsequent decay, and rapid color evolution are consistent with multiple ejecta components of differing lanthanide abundance. The late-time light curve indicates that SSS17a produced at least ~0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
582 citations
Authors
Showing all 22586 results
Name | H-index | Papers | Citations |
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George Davey Smith | 224 | 2540 | 248373 |
David Miller | 203 | 2573 | 204840 |
Patrick O. Brown | 183 | 755 | 200985 |
Dorret I. Boomsma | 176 | 1507 | 136353 |
Chad A. Mirkin | 164 | 1078 | 134254 |
Darien Wood | 160 | 2174 | 136596 |
Wei Li | 158 | 1855 | 124748 |
Timothy C. Beers | 156 | 934 | 102581 |
Todd Adams | 154 | 1866 | 143110 |
Albert-László Barabási | 152 | 438 | 200119 |
T. J. Pearson | 150 | 895 | 126533 |
Amartya Sen | 149 | 689 | 141907 |
Christopher Hill | 144 | 1562 | 128098 |
Tim Adye | 143 | 1898 | 109010 |
Teruki Kamon | 142 | 2034 | 115633 |