Institution
Charles University in Prague
Education•Prague, 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.
Topics: Population, Large Hadron Collider, Czech, Magnetization, Transplantation
Papers published on a yearly basis
Papers
More filters
••
NanoString Technologies1, Ghent University2, Katholieke Universiteit Leuven3, Cornell University4, Memorial Sloan Kettering Cancer Center5, Ludwig Institute for Cancer Research6, Charles University in Prague7, Istituto Superiore di Sanità8, National Institutes of Health9, Institute of Cancer Research10, Merck & Co.11, University of Manchester12, University of California, San Diego13, Harvard University14, University of Navarra15, University of Pittsburgh16, McMaster University17, University of Tromsø18, Humanitas University19, University of Turin20, QIMR Berghofer Medical Research Institute21, Université de Montréal22, University of São Paulo23, University of Texas Southwestern Medical Center24, Yale University25
TL;DR: An updated operational definition of immunogenic cell death is provided, the key factors that dictate the ability of dying cells to drive an adaptive immune response are discussed, and experimental assays that are currently available for the assessment of ICD in vitro and in vivo are summarized.
Abstract: Cells succumbing to stress via regulated cell death (RCD) can initiate an adaptive immune response associated with immunological memory, provided they display sufficient antigenicity and adjuvanticity. Moreover, multiple intracellular and microenvironmental features determine the propensity of RCD to drive adaptive immunity. Here, we provide an updated operational definition of immunogenic cell death (ICD), discuss the key factors that dictate the ability of dying cells to drive an adaptive immune response, summarize experimental assays that are currently available for the assessment of ICD in vitro and in vivo, and formulate guidelines for their interpretation.
544 citations
••
TL;DR: Patients treated with the hybrid protocol, and especially those who responded poorly to prednisone, had higher EFS than most reported outcomes for treatment of infant ALL, and Delayed intensification of chemotherapy did not benefit patients.
539 citations
••
Max Planck Society1, Yerevan Physics Institute2, Durham University3, Centre national de la recherche scientifique4, University of Hamburg5, Université libre de Bruxelles6, Collège de France7, Humboldt University of Berlin8, University of Montpellier9, Tata Institute of Fundamental Research10, École Polytechnique11, Dublin Institute for Advanced Studies12, DSM13, Joseph Fourier University14, North-West University15, Washington University in St. Louis16, Ruhr University Bochum17, Iowa State University18, University of Sheffield19, Charles University in Prague20, University of Namibia21
TL;DR: A TeV γ-ray image of the SNR shows the spatially resolved remnant has a shell morphology similar to that seen in X-rays, which demonstrates that very-high-energy particles are accelerated there, consistent with current ideas of particle acceleration in young SNR shocks.
Abstract: A significant fraction of the energy density of the interstellar medium is in the form of high-energy charged particles (cosmic rays)1. The origin of these particles remains uncertain. Although it is generally accepted that the only sources capable of supplying the energy required to accelerate the bulk of Galactic cosmic rays are supernova explosions, and even though the mechanism of particle acceleration in expanding supernova remnant (SNR) shocks is thought to be well understood theoretically2,3, unequivocal evidence for the production of high-energy particles in supernova shells has proven remarkably hard to find. Here we report on observations of the SNR RX J1713.7 - 3946 (G347.3 - 0.5), which was discovered by ROSAT4 in the X-ray spectrum and later claimed as a source of high-energy γ-rays5,6 of TeV energies (1 TeV = 1012 eV). We present a TeV γ-ray image of the SNR: the spatially resolved remnant has a shell morphology similar to that seen in X-rays, which demonstrates that very-high-energy particles are accelerated there. The energy spectrum indicates efficient acceleration of charged particles to energies beyond 100 TeV, consistent with current ideas of particle acceleration in young SNR shocks.
537 citations
•
01 Aug 2012TL;DR: In this paper, the authors introduce the concept of space-time related to Schwarzchild and Taub-NUT space-times, and provide solutions for uniformly accelerating particles in the plane and pp-wave domain.
Abstract: Preface 1. Introduction 2. Basic tools and concepts 3. Minkowski space-time 4. de Sitter space-time 5. Anti-de Sitter space-time 6. Friedmann-Lemaitre-Robertson-Walker space-times 7. Electrovacuum and related background space-times 8. Schwarzchild space-time 9. Space-times related to Schwarzchild 10. Static axially symmetric space-times 11. Rotating black holes 12. Taub-NUT space-time 13. Stationary, axially symmetric space-times 14. Accelerating black holes 15. Further solutions for uniformly accelerating particles 16. Plebanski-Demianski solutions 17. Plane and pp-waves 18. Kundt solutions 19. Robinson-Trautman solutions 20. Impulsive waves 21. Colliding plane waves 22. A final miscellany Appendix A. 2-spaces of constant curvature Appendix B. 3-spaces of constant curvature References Index.
533 citations
••
U. Bhawandeep1, Vardan Khachatryan, Albert M. Sirunyan, Armen Tumasyan +2289 more•Institutions (147)
TL;DR: In this paper, the trigger system consists of two levels designed to select events of potential physics interest from a GHz (MHz) interaction rate of proton-proton (heavy ion) collisions.
Abstract: This paper describes the CMS trigger system and its performance during Run 1 of the LHC. The trigger system consists of two levels designed to select events of potential physics interest from a GHz (MHz) interaction rate of proton-proton (heavy ion) collisions. The first level of the trigger is implemented in hardware, and selects events containing detector signals consistent with an electron, photon, muon, tau lepton, jet, or missing transverse energy. A programmable menu of up to 128 object-based algorithms is used to select events for subsequent processing. The trigger thresholds are adjusted to the LHC instantaneous luminosity during data taking in order to restrict the output rate to 100 kHz, the upper limit imposed by the CMS readout electronics. The second level, implemented in software, further refines the purity of the output stream, selecting an average rate of 400 Hz for offline event storage. The objectives, strategy and performance of the trigger system during the LHC Run 1 are described.
532 citations
Authors
Showing all 32719 results
Name | H-index | Papers | Citations |
---|---|---|---|
Ronald C. Petersen | 178 | 1091 | 153067 |
P. Chang | 170 | 2154 | 151783 |
Vaclav Vrba | 141 | 1298 | 95671 |
Milos Lokajicek | 139 | 1511 | 98888 |
Christopher D. Manning | 138 | 499 | 147595 |
Yves Sirois | 137 | 1334 | 95714 |
Rupert Leitner | 136 | 1201 | 90597 |
Gerald M. Reaven | 133 | 799 | 80351 |
Roberto Sacchi | 132 | 1186 | 89012 |
S. Errede | 132 | 1481 | 98663 |
Mark Neubauer | 131 | 1252 | 89004 |
Peter Kodys | 131 | 1262 | 85267 |
Panos A Razis | 130 | 1287 | 90704 |
Vit Vorobel | 130 | 919 | 79444 |
Jehad Mousa | 130 | 1226 | 86564 |