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Institution

University of Valencia

EducationValencia, Spain
About: University of Valencia is a education organization based out in Valencia, Spain. It is known for research contribution in the topics: Population & Neutrino. The organization has 27096 authors who have published 65669 publications receiving 1765689 citations. The organization is also known as: Universitat de València & UV.


Papers
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Journal ArticleDOI
TL;DR: This work estimated population in 195 locations by single year of age and single calendar year from 1950 to 2017 with standardised and replicable methods and used the cohort-component method of population projection, with inputs of fertility, mortality, population, and migration data.

287 citations

Journal ArticleDOI
TL;DR: A European perspective on the best way to play an active role in implementing into clinical practice the key principle of radiation protection that: 'each patient should get the right imaging exam, at the right time, with the right radiation dose'.
Abstract: The benefits of cardiac imaging are immense, and modern medicine requires the extensive and versatile use of a variety of cardiac imaging techniques. Cardiologists are responsible for a large part of the radiation exposures every person gets per year from all medical sources. Therefore, they have a particular responsibility to avoid unjustified and non-optimized use of radiation, but sometimes are imperfectly aware of the radiological dose of the examination they prescribe or practice. This position paper aims to summarize the current knowledge on radiation effective doses (and risks) related to cardiac imaging procedures. We have reviewed the literature on radiation doses, which can range from the equivalent of 1-60 milliSievert (mSv) around a reference dose average of 15 mSv (corresponding to 750 chest X-rays) for a percutaneous coronary intervention, a cardiac radiofrequency ablation, a multidetector coronary angiography, or a myocardial perfusion imaging scintigraphy. We provide a European perspective on the best way to play an active role in implementing into clinical practice the key principle of radiation protection that: 'each patient should get the right imaging exam, at the right time, with the right radiation dose'.

287 citations

Journal ArticleDOI
TL;DR: The major taphonomic processes that control insect preservation in carbonate rocks (limestones, travertines and nodules) are biological: insect size and wingspan, degree of decomposition, presence of microbial mats, predation and scavenging; environmental: water surface tension, water temperature, density and salinity, current activity; and diagenetic: authigenic mineralisation, flattening, deformation, carbonisation as discussed by the authors.

287 citations

Journal ArticleDOI
10 Sep 1999-Science
TL;DR: The effects of clonal interference were measured in the asexual RNA virus vesicular stomatitis virus; rates and average effects of beneficial mutations were quantified.
Abstract: In asexual populations, beneficial mutations that occur in different lineages compete with one another. This phenomenon, known as clonal interference, ensures that those beneficial mutations that do achieve fixation are of large effect. Clonal interference also increases the time between fixations, thereby slowing the adaptation of asexual populations. The effects of clonal interference were measured in the asexual RNA virus vesicular stomatitis virus; rates and average effects of beneficial mutations were quantified.

287 citations

Journal ArticleDOI
TL;DR: Using a collapsar progenitor model of MacFadyen & Woosley, the propagation of an axisymmetric jet through a collapsing rotating massive star with the GENESIS multidimensional relativistic hydrodynamic code is simulated.
Abstract: We have studied the relativistie beamed outflow proposed to occur in the collapsar model of gamma-ray bursts. A jet forms as a consequence of an assumed energy deposition of ~ 1050 - 1051 erg/s within a 30° cone around the rotation axis of the progenitor star. The generated jet flow is strongly beamed ( ≲ few degrees) and reaches the surface of the stellar progenitor (r ≈ 31010 cm) intact. At break-out the maximum Lorentz factor of the jet flow is about 33. Simulations have been performed with the GENESIS multi-dimensional relativistie hydrodynamic code.

286 citations


Authors

Showing all 27402 results

NameH-indexPapersCitations
H. S. Chen1792401178529
Alvaro Pascual-Leone16596998251
Sabino Matarrese155775123278
Subir Sarkar1491542144614
Carlos Escobar148118495346
Marco Costa1461458105096
Carmen García139150396925
Javier Cuevas1381689103604
M. I. Martínez134125179885
Marco Aurelio Diaz134101593580
Avelino Corma134104989095
Kevin Lannon133165295436
Marina Cobal132107885437
Mogens Dam131110983717
Marcel Vos13199385194
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20251
2023140
2022487
20214,747
20204,696
20193,996