scispace - formally typeset
Search or ask a question
Institution

University of Siena

EducationSiena, 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.


Papers
More filters
Journal ArticleDOI
TL;DR: A number of correlative pathological and MRI studies have helped to define in vivo the pathological substrates of MS in focal lesions and normal-appearing white matter, not only in the brain, but also in the spinal cord.
Abstract: Pathological evaluation is the gold standard for identifying processes related to multiple sclerosis that explain disease manifestations, and for guiding the development of new treatments. However, there are limitations to the techniques used, including the small number of donors available, samples often representing uncommon cases, and impossibility of follow-up. Correlative studies have demonstrated that MRI is sensitive to the different pathological substrates of multiple sclerosis (inflammation, demyelination, and neuro-axonal loss). The role of MRI in evaluating other pathological processes, such as leptomeningeal involvement, central vein and rim of lesions, microstructural abnormalities, iron accumulation, and recovery mechanisms, has been investigated. Although techniques used for quantifying pathological processes in different regions of the CNS have advanced diagnosis and monitoring of disease course and treatment of multiple sclerosis, new perspectives and questions have emerged, including how different pathological processes interact over the disease course and when remyelination might occur. Addressing these questions will require longitudinal studies using MRI in large cohorts of patients with different phenotypes.

441 citations

Journal ArticleDOI
TL;DR: On behalf of all coauthors of the safety paper, they apologize to the scientific community, and provide a revised 13-item screening questionnaire, which should replace the previous one.

439 citations

Journal ArticleDOI
TL;DR: The fundamental concepts of speckle‐tracking echocardiography are described, how to obtain strain measurements using this technique is illustrated, and their recognized and developing clinical applications are discussed.
Abstract: Speckle-tracking echocardiography has recently emerged as a quantitative ultrasound technique for accurately evaluating myocardial function by analyzing the motion of speckles identified on routine 2-dimensional sonograms. It provides non-Doppler, angle-independent, and objective quantification of myocardial deformation and left ventricular systolic and diastolic dynamics. By tracking the displacement of the speckles during the cardiac cycle, strain and the strain rate can be rapidly measured offline after adequate image acquisition. Data regarding the feasibility, accuracy, and clinical applications of speckle-tracking echocardiography are rapidly accumulating. This review describes the fundamental concepts of speckle-tracking echocardiography, illustrates how to obtain strain measurements using this technique, and discusses their recognized and developing clinical applications.

433 citations

Journal ArticleDOI
Justin Albert1, E. Aliu, H. Anderhub, P. Antoranz2, A. Armada, M. Asensio2, C. Baixeras3, Juan Abel Barrio2, M. Bartelt4, H. Bartko5, Denis Bastieri6, S. R. Bavikadi7, W. Bednarek8, K. Berger1, Ciro Bigongiari6, Adrian Biland, E. Bisesi7, R. K. Bock5, Pol Bordas9, Valentí Bosch-Ramon9, Thomas Bretz1, I. Britvitch, M. Camara2, E. Carmona5, Ashot Chilingarian10, Stefano Ciprini, J. A. Coarasa5, S. Commichau, Jose Luis Contreras2, Juan Cortina, V. Curtef4, V. Danielyan10, Francesco Dazzi6, A. De Angelis7, R. de los Reyes2, B. De Lotto7, E. Domingo-Santamaría, Daniela Dorner1, Michele Doro6, Manel Errando, Michela Fagiolini11, Daniel Ferenc12, E. Fernandez, R. Firpo, Jose Flix, M. V. Fonseca2, Ll. Font3, M. Fuchs5, Nicola Galante11, M. Garczarczyk5, Markus Gaug6, Maria Giller8, Florian Goebel5, D. Hakobyan10, Masaaki Hayashida5, T. Hengstebeck13, D. Höhne1, J. Hose5, C. C. Hsu5, Paula Gina Isar5, P. Jacon8, O. Kalekin13, R. Kosyra5, D. Kranich1, D. Kranich12, M. Laatiaoui5, A. Laille12, T. Lenisa7, P. Liebing5, Elina Lindfors, S. Lombardi6, Francesco Longo14, Josue J. Lopez, M. López2, E. Lorenz5, F. Lucarelli2, P. Majumdar5, G. Maneva, K. Mannheim1, Oriana Mansutti7, Mosè Mariotti6, M. I. Martínez, K. Mase5, Daniel Mazin5, C. Merck5, Mario Meucci11, M. Meyer1, Jose Miguel Miranda2, R. Mirzoyan5, S. Mizobuchi5, Abelardo Moralejo, K. Nilsson, E. Oña-Wilhelmi, R. Orduña3, N. Otte5, I. Oya2, David Paneque5, Riccardo Paoletti11, Josep M. Paredes9, M. Pasanen, D. Pascoli6, F. Pauss, N. Pavel13, R. Pegna11, Massimo Persic, L. Peruzzo6, A. Piccioli11, M. Poller1, Guy G. Pooley15, Elisa Prandini6, A. Raymers10, Wolfgang Rhode4, Marc Ribó9, J. Rico, B. Riegel1, M. Rissi, A. Robert3, Gustavo E. Romero16, S. Rügamer1, A. Saggion6, Alvaro Sanchez3, P. Sartori6, V. Scalzotto6, V. Scapin6, R. Schmitt1, T. Schweizer13, M. Shayduk13, K. Shinozaki5, Steven N. Shore17, N. Sidro, A. Sillanpää, Dorota Sobczyńska8, Antonio Stamerra11, L. S. Stark, L. O. Takalo, Petar Temnikov, D. Tescaro, Masahiro Teshima5, N. Tonello5, A. Torres3, Diego F. Torres18, Nicola Turini11, H. Vankov, V. Vitale7, Robert Wagner5, Tadeusz Wibig8, W. Wittek5, R. Zanin6, J. Zapatero3 
23 Jun 2006-Science
TL;DR: The detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303 is reported, which suggests that the emission is periodic.
Abstract: Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sources of cosmic rays and can be used to elucidate the physics of relativistic jets. We report the detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303. Six orbital cycles were recorded. Several detections occur at a similar orbital phase, which suggests that the emission is periodic. The strongest gamma-ray emission is not observed when the two stars are closest to one another, implying a strong orbital modulation of the emission or absorption processes.

433 citations


Authors

Showing all 12352 results

NameH-indexPapersCitations
Johan Auwerx15865395779
I. V. Gorelov1391916103133
Roberto Tenchini133139094541
Francesco Fabozzi133156193364
M. Davier1321449107642
Roberto Dell'Orso132141292792
Rino Rappuoli13281664660
Teimuraz Lomtadze12989380314
Manas Maity129130987465
Dezso Horvath128128388111
Paolo Azzurri126105881651
Vincenzo Di Marzo12665960240
Igor Katkov12597271845
Ying Lu12370862645
Thomas Schwarz12370154560
Network Information
Related Institutions (5)
University of Florence
79.5K papers, 2.3M citations

97% related

Sapienza University of Rome
155.4K papers, 4.3M citations

96% related

University of Padua
114.8K papers, 3.6M citations

95% related

University of Bologna
115.1K papers, 3.4M citations

95% related

University of Milan
139.7K papers, 4.6M citations

95% related

Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202391
2022221
20211,870
20201,979
20191,639
20181,523