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Institution

Washington State University

EducationPullman, Washington, United States
About: Washington State University is a education organization based out in Pullman, Washington, United States. It is known for research contribution in the topics: Population & Gene. The organization has 26947 authors who have published 57736 publications receiving 2341509 citations. The organization is also known as: WSU & Wazzu.


Papers
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Journal ArticleDOI
TL;DR: It is proposed that reactive Cys persulfides and S-polythiolation have critical regulatory functions in redox cell signaling and H2S may act primarily as a marker for the biologically active of persulfide species.
Abstract: Using methodology developed herein, it is found that reactive persulfides and polysulfides are formed endogenously from both small molecule species and proteins in high amounts in mammalian cells and tissues. These reactive sulfur species were biosynthesized by two major sulfurtransferases: cystathionine β-synthase and cystathionine γ-lyase. Quantitation of these species indicates that high concentrations of glutathione persulfide (perhydropersulfide >100 μM) and other cysteine persulfide and polysulfide derivatives in peptides/proteins were endogenously produced and maintained in the plasma, cells, and tissues of mammals (rodent and human). It is expected that persulfides are especially nucleophilic and reducing. This view was found to be the case, because they quickly react with H2O2 and a recently described biologically generated electrophile 8-nitroguanosine 3′,5′-cyclic monophosphate. These results indicate that persulfides are potentially important signaling/effector species, and because H2S can be generated from persulfide degradation, much of the reported biological activity associated with H2S may actually be that of persulfides. That is, H2S may act primarily as a marker for the biologically active of persulfide species.

688 citations

Journal ArticleDOI
TL;DR: In Taiwan, tourism and economic development reinforce each other, indicating a long-run equilibrium relationship and further a bi-directional causality between the two factors.

686 citations

Journal ArticleDOI
TL;DR: Although institutional investors have a preference for large capitalization stocks, over time they have shifted their preferences toward smaller, riskier securities as mentioned in this paper, and evidence also suggests that recent growth in institutional investment combined with this shift in preferences helps explain why markets in general and smaller stocks in particular, have exhibited greater firm-specific risk and liquidity.
Abstract: Although institutional investors have a preference for large capitalization stocks, over time they have shifted their preferences toward smaller, riskier securities. These changes in aggregate preferences have arisen primarily from changes in the preferences of each class of institution, rather than changes in the importance of different classes. Evidence also suggests that recent growth in institutional investment combined with this shift in preferences helps explain why markets in general, and smaller stocks in particular, have exhibited greater firm-specific risk and liquidity in recent years. Additional analyses suggest that institutional investors moved toward smaller securities because such securities offer "greener pastures." Copyright 2003, Oxford University Press.

685 citations

Journal ArticleDOI
Stefan Hild1, M. R. Abernathy1, Fausto Acernese2, Pau Amaro-Seoane3, Nils Andersson4, K. G. Arun5, Fabrizio Barone2, B. Barr1, M. Barsuglia, Mark Beker, N. Beveridge1, S. Birindelli6, Suvadeep Bose7, L. Bosi, S. Braccini8, C. Bradaschia8, Tomasz Bulik9, Enrico Calloni10, Giancarlo Cella8, E. Chassande Mottin, S. Chelkowski11, Andrea Chincarini, James S. Clark12, E. Coccia13, C. Colacino8, J. Colas, A. Cumming1, L. Cunningham1, E. Cuoco, S. L. Danilishin14, Karsten Danzmann3, R. De Salvo15, T. Dent12, R. De Rosa10, L. Di Fiore10, A. Di Virgilio8, M. Doets16, V. Fafone13, Paolo Falferi17, R. Flaminio, J. Franc, F. Frasconi8, Andreas Freise11, D. Friedrich18, Paul Fulda11, Jonathan R. Gair19, Gianluca Gemme, E. Genin, A. Gennai11, A. Giazotto8, Kostas Glampedakis20, Christian Gräf3, M. Granata, Hartmut Grote3, G. M. Guidi21, A. Gurkovsky14, G. D. Hammond1, Mark Hannam12, Jan Harms15, D. Heinert22, Martin Hendry1, Ik Siong Heng1, E. Hennes, J. H. Hough, Sascha Husa23, S. H. Huttner1, G. T. Jones12, F. Y. Khalili14, Keiko Kokeyama11, Kostas D. Kokkotas20, Badri Krishnan3, Tjonnie G. F. Li, M. Lorenzini, H. Lück3, Ettore Majorana, Ilya Mandel24, Vuk Mandic25, M. Mantovani8, I. W. Martin1, Christine Michel, Y. Minenkov13, N. Morgado, S. Mosca10, B. Mours26, Helge Müller-Ebhardt18, P. G. Murray1, Ronny Nawrodt22, Ronny Nawrodt1, John Nelson1, Richard O'Shaughnessy27, Christian D. Ott15, C. Palomba, Angela Delli Paoli, G. Parguez, A. Pasqualetti, R. Passaquieti28, R. Passaquieti8, D. Passuello8, Laurent Pinard, Wolfango Plastino29, Rosa Poggiani28, Rosa Poggiani8, P. Popolizio, Mirko Prato, M. Punturo, P. Puppo, D. S. Rabeling16, P. Rapagnani30, Jocelyn Read31, Tania Regimbau6, H. Rehbein3, S. Reid1, F. Ricci30, F. Richard, A. Rocchi, Sheila Rowan1, A. Rüdiger3, Lucía Santamaría15, Benoit Sassolas, Bangalore Suryanarayana Sathyaprakash12, Roman Schnabel3, C. Schwarz22, Paul Seidel22, Alicia M. Sintes23, Kentaro Somiya15, Fiona C. Speirits1, Kenneth A. Strain1, S. E. Strigin14, P. J. Sutton12, S. P. Tarabrin18, Andre Thüring3, J. F. J. van den Brand16, M. van Veggel1, C. Van Den Broeck, Alberto Vecchio11, John Veitch12, F. Vetrano21, A. Viceré21, S. P. Vyatchanin14, Benno Willke3, Graham Woan1, Kazuhiro Yamamoto 
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Abstract: Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.

682 citations

Journal ArticleDOI
TL;DR: This document is a summary statement of the outcome from he meeting: “Bisphenol A: An Examination of the Relevance of cological, In vitro and Laboratory Animal Studies for Assessng Risks to Human Health” sponsored by both the NIEHS and IDCR at NIH/DHHS.

681 citations


Authors

Showing all 27183 results

NameH-indexPapersCitations
Anil K. Jain1831016192151
Martin Karplus163831138492
Herbert A. Simon157745194597
Suvadeep Bose154960129071
Rajesh Kumar1494439140830
Kevin Murphy146728120475
Jonathan D. G. Jones12941780908
Douglas E. Soltis12761267161
Peter W. Kalivas12342852445
Chris Somerville12228445742
Pamela S. Soltis12054361080
Yuehe Lin11864155399
Howard I. Maibach116182160765
Jizhong Zhou11576648708
Farshid Guilak11048041327
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202398
2022344
20212,786
20202,783
20192,691
20182,370