Institution
University of Siena
Education•Siena, Italy•
About: University of Siena is a education organization based out in Siena, Italy. It is known for research contribution in the topics: Population & Cancer. The organization has 12179 authors who have published 33334 publications receiving 1008287 citations. The organization is also known as: Università degli studi di Siena & Universita degli studi di Siena.
Topics: Population, Cancer, Large Hadron Collider, Sperm, Oxidative stress
Papers published on a yearly basis
Papers
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TL;DR: The usage of protein CO groups as biomarkers of oxidative stress has some advantages in comparison with the measurement of other oxidation products because of the relative early formation and the relative stability of carbonylated proteins.
2,097 citations
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TL;DR: Improvements to this method are described, and an extension of SIENA is extended to a new method for cross-sectional (single time point) analysis, which provides easy manual review of their output by the automatic production of summary images.
1,932 citations
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TL;DR: European consensus for the management of patients with differentiated thyroid carcinoma of the follicular epithelium Furio Pacini, Martin Schlumberger, Henning Dralle, Rossella Elisei, Johannes W A Smit, Wilmar Wiersinga and the European Thyroid Cancer Taskforce Section of Endocrinology and Metabolism are presented.
Abstract: European consensus for the management of patients with differentiated thyroid carcinoma of the follicular epithelium Furio Pacini, Martin Schlumberger, Henning Dralle, Rossella Elisei, Johannes W A Smit, Wilmar Wiersinga and the European Thyroid Cancer Taskforce Section of Endocrinology and Metabolism, University of Siena, Via Bracci, 53100 Siena, Italy, Service de Medicine Nucleaire, Institut Gustave Roussy, Villejuif, France, Department of General, Visceral and Vascular Surgery, University of Halle, Germany, Department of Endocrinology, University of Pisa, Italy, Department of Endocrinology and Metabolic Disease, Leiden University Medical Center, The Netherlands and Department of Endocrinology and Metabolism, University of Amsterdam, The Netherlands
1,926 citations
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The Catholic University of America1, Royal Prince Alfred Hospital2, University of Toronto3, Centre for Addiction and Mental Health4, Università Campus Bio-Medico5, University of Eastern Finland6, Monash University7, Medical University of South Carolina8, Paris 12 Val de Marne University9, University of Regensburg10, University of Brescia11, University of Göttingen12, Beth Israel Deaconess Medical Center13, University of Siena14, University College London15, Copenhagen University Hospital16, Fukushima Medical University17, University of Tübingen18
TL;DR: These guidelines provide an up-date of previous IFCN report on “Non-invasive electrical and magnetic stimulation of the brain, spinal cord and roots: basic principles and procedures for routine clinical application” and include some recent extensions and developments.
1,850 citations
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TL;DR: This analysis expands upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation of state and have spins within the range observed in Galactic binary neutron stars.
Abstract: On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation of state and have spins within the range observed in Galactic binary neutron stars. Our analysis employs two methods: the use of equation-of-state-insensitive relations between various macroscopic properties of the neutron stars and the use of an efficient parametrization of the defining function pðρÞ of the equation of state itself. From the LIGO and Virgo data alone and the first method, we measure the two neutron star radii as R1 ¼ 10.8 þ2.0 −1.7 km for the heavier star and R2 ¼ 10.7 þ2.1 −1.5 km for the lighter star at the 90% credible level. If we additionally require that the equation of state supports neutron stars with masses larger than 1.97 M⊙ as required from electromagnetic observations and employ the equation-of-state parametrization, we further constrain R1 ¼ 11.9 þ1.4 −1.4 km and R2 ¼ 11.9 þ1.4 −1.4 km at the 90% credible level. Finally, we obtain constraints on pðρÞ at supranuclear densities, with pressure at twice nuclear saturation density measured at 3.5 þ2.7 −1.7 × 1034 dyn cm−2 at the 90% level.
1,595 citations
Authors
Showing all 12352 results
Name | H-index | Papers | Citations |
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Johan Auwerx | 158 | 653 | 95779 |
I. V. Gorelov | 139 | 1916 | 103133 |
Roberto Tenchini | 133 | 1390 | 94541 |
Francesco Fabozzi | 133 | 1561 | 93364 |
M. Davier | 132 | 1449 | 107642 |
Roberto Dell'Orso | 132 | 1412 | 92792 |
Rino Rappuoli | 132 | 816 | 64660 |
Teimuraz Lomtadze | 129 | 893 | 80314 |
Manas Maity | 129 | 1309 | 87465 |
Dezso Horvath | 128 | 1283 | 88111 |
Paolo Azzurri | 126 | 1058 | 81651 |
Vincenzo Di Marzo | 126 | 659 | 60240 |
Igor Katkov | 125 | 972 | 71845 |
Ying Lu | 123 | 708 | 62645 |
Thomas Schwarz | 123 | 701 | 54560 |