scispace - formally typeset
Search or ask a question
Institution

Charles University in Prague

EducationPrague, Czechia
About: Charles University in Prague is a education organization based out in Prague, Czechia. It is known for research contribution in the topics: Population & Large Hadron Collider. The organization has 32392 authors who have published 74435 publications receiving 1804208 citations.


Papers
More filters
Journal ArticleDOI
TL;DR: Angiotensin-neprilysin inhibition prevents the clinical progression of surviving patients with heart failure more effectively than angiotens in-converting enzyme inhibition.
Abstract: Background—Clinical trials in heart failure have focused on the improvement in symptoms or decreases in the risk of death and other cardiovascular events. Little is known about the effect of drugs ...

532 citations

Proceedings ArticleDOI
04 Jun 2009
TL;DR: This shared task combines the shared tasks of the previous five years under a unique dependency-based formalism similar to the 2008 task and describes how the data sets were created and show their quantitative properties.
Abstract: For the 11th straight year, the Conference on Computational Natural Language Learning has been accompanied by a shared task whose purpose is to promote natural language processing applications and evaluate them in a standard setting. In 2009, the shared task was dedicated to the joint parsing of syntactic and semantic dependencies in multiple languages. This shared task combines the shared tasks of the previous five years under a unique dependency-based formalism similar to the 2008 task. In this paper, we define the shared task, describe how the data sets were created and show their quantitative properties, report the results and summarize the approaches of the participating systems.

531 citations

Journal ArticleDOI
TL;DR: Treatment with six cycles of BEACOPP(escalated) followed by PET-guided radiotherapy was more effective in terms of freedom from treatment failure and less toxic than eight cycles of the same chemotherapy regimen, and should be the treatment of choice for advanced stage Hodgkin's lymphoma.

528 citations

Journal ArticleDOI
TL;DR: This work mapped cis- and trans-regulatory control elements for expression of thousands of genes across the genome in the BXH/HXB panel of rat recombinant inbred strains and generated a data set of 73 candidate genes for hypertension that merit testing in human populations.
Abstract: Integration of genome-wide expression profiling with linkage analysis is a new approach to identifying genes underlying complex traits. We applied this approach to the regulation of gene expression in the BXH/HXB panel of rat recombinant inbred strains, one of the largest available rodent recombinant inbred panels and a leading resource for genetic analysis of the highly prevalent metabolic syndrome. In two tissues important to the pathogenesis of the metabolic syndrome, we mapped cis- and trans-regulatory control elements for expression of thousands of genes across the genome. Many of the most highly linked expression quantitative trait loci are regulated in cis, are inherited essentially as monogenic traits and are good candidate genes for previously mapped physiological quantitative trait loci in the rat. By comparative mapping we generated a data set of 73 candidate genes for hypertension that merit testing in human populations. Mining of this publicly available data set is expected to lead to new insights into the genes and regulatory pathways underlying the extensive range of metabolic and cardiovascular disease phenotypes that segregate in these recombinant inbred strains.

527 citations

Journal ArticleDOI
Felix Aharonian1, A. G. Akhperjanian2, A. R. Bazer-Bachi3, M. Beilicke4, Wystan Benbow1, David Berge1, Konrad Bernlöhr1, Konrad Bernlöhr5, Catherine Boisson3, O. Bolz1, V. Borrel3, Ilana M. Braun1, F. Breitling5, A. M. Brown6, P. M. Chadwick6, L.-M. Chounet7, R. Cornils4, Luigi Costamante1, B. Degrange7, Hugh Dickinson6, A. Djannati-Ataï8, L. O'c. Drury9, Guillaume Dubus7, Dimitrios Emmanoulopoulos, P. Espigat8, F. Feinstein10, G. Fontaine7, Y. Fuchs11, Stefan Funk1, Y. A. Gallant10, B. Giebels7, Stefan Gillessen1, J. F. Glicenstein12, P. Goret12, C. Hadjichristidis6, D. Hauser1, M. Hauser, G. Heinzelmann4, Gilles Henri11, G. Hermann1, Jim Hinton1, Werner Hofmann1, M. Holleran13, Dieter Horns1, A. Jacholkowska10, O. C. de Jager13, B. Khélifi1, Sven Klages1, Nu. Komin5, A. Konopelko5, I. J. Latham6, R. Le Gallou6, A. Lemiere8, M. Lemoine-Goumard7, N. Leroy7, Thomas Lohse5, A. Marcowith3, Jean Michel Martin3, O. Martineau-Huynh3, Conor Masterson1, T. J. L. McComb6, M. de Naurois3, S. J. Nolan6, A. Noutsos6, K. J. Orford6, J. L. Osborne6, M. Ouchrif3, M. Panter1, Guy Pelletier11, S. Pita8, G. Pühlhofer, Michael Punch8, B. C. Raubenheimer13, Martin Raue4, J. Raux3, S. M. Rayner6, A. Reimer14, Olaf Reimer14, J. Ripken4, L. Rob15, L. Rolland3, Gavin Rowell1, V. Sahakian2, L. Saugé11, S. Schlenker5, Reinhard Schlickeiser14, C. Schuster14, Ullrich Schwanke5, M. Siewert14, Helene Sol3, D. Spangler6, R. Steenkamp16, C. Stegmann5, J.-P. Tavernet3, Regis Terrier8, C. G. Théoret8, M. Tluczykont7, C. van Eldik1, G. Vasileiadis10, Christo Venter13, P. Vincent3, Heinrich J. Völk1, Stefan Wagner 
09 Feb 2006-Nature
TL;DR: In this paper, a very high-energy γ-ray emission from the Galactic Centre region has been measured using HESS, the High Energy Stereoscopic System recently constructed in Namibia, South West Africa.
Abstract: Events at the centre of our Galaxy are key to our understanding of high-energy processes in the Universe, since it contains examples of virtually every type of exotic object known to astronomers. The very-high-energy γ-ray emission from the Galactic Centre region has now been measured using HESS, the High Energy Stereoscopic System recently constructed in Namibia, South West Africa. HESS operates at energies above the regime accessible to satellite-based detectors, taking γ-ray astronomy into new territory. The results show that these clouds are glowing in very high energy γ-rays. The glow is caused by constant bombardment of the clouds by cosmic rays — probably protons and nuclei — produced close to the central black hole or in the expanding blast waves of supernova explosions. The source of Galactic cosmic rays (with energies up to 1015 eV) remains unclear, although it is widely believed that they originate in the shock waves of expanding supernova remnants1,2. At present the best way to investigate their acceleration and propagation is by observing the γ-rays produced when cosmic rays interact with interstellar gas3. Here we report observations of an extended region of very-high-energy (> 1011 eV) γ-ray emission correlated spatially with a complex of giant molecular clouds in the central 200 parsecs of the Milky Way. The hardness of the γ-ray spectrum and the conditions in those molecular clouds indicate that the cosmic rays giving rise to the γ-rays are likely to be protons and nuclei rather than electrons. The energy associated with the cosmic rays could have come from a single supernova explosion around 104 years ago.

527 citations


Authors

Showing all 32719 results

NameH-indexPapersCitations
Ronald C. Petersen1781091153067
P. Chang1702154151783
Vaclav Vrba141129895671
Milos Lokajicek139151198888
Christopher D. Manning138499147595
Yves Sirois137133495714
Rupert Leitner136120190597
Gerald M. Reaven13379980351
Roberto Sacchi132118689012
S. Errede132148198663
Mark Neubauer131125289004
Peter Kodys131126285267
Panos A Razis130128790704
Vit Vorobel13091979444
Jehad Mousa130122686564
Network Information
Related Institutions (5)
University of Milan
139.7K papers, 4.6M citations

90% related

Sapienza University of Rome
155.4K papers, 4.3M citations

90% related

University of Amsterdam
140.8K papers, 5.9M citations

89% related

University of Oxford
258.1K papers, 12.9M citations

89% related

Tel Aviv University
115.9K papers, 3.9M citations

89% related

Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023203
2022554
20214,838
20204,793
20194,421
20183,991