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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
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Journal ArticleDOI
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

Journal ArticleDOI
Felix Aharonian1, A. G. Akhperjanian2, Klaus-Michael Aye3, A. R. Bazer-Bachi4, M. Beilicke5, Wystan Benbow1, David Berge1, P. Berghaus6, P. Berghaus7, Konrad Bernlöhr8, Konrad Bernlöhr1, O. Bolz1, Catherine Boisson4, C. Borgmeier8, F. Breitling8, A. M. Brown3, J. Bussons Gordo9, P. M. Chadwick3, V. R. Chitnis10, V. R. Chitnis4, L-M. Chounet11, R. Cornils5, Luigi Costamante1, B. Degrange11, A. Djannati-Ataï7, L. O'c. Drury12, Tulun Ergin8, P. Espigat7, F. Feinstein9, P. Fleury11, G. Fontaine11, Stefan Funk1, Y. A. Gallant9, B. Giebels11, Stefan Gillessen1, P. Goret13, Julien Guy6, Julien Guy4, C. Hadjichristidis3, M. Hauser, G. Heinzelmann5, Gilles Henri14, German Hermann1, Jim Hinton1, Werner Hofmann1, M. Holleran15, Dieter Horns1, O. C. de Jager15, I. Jung16, I. Jung1, B. Khélifi1, Nu. Komin8, A. Konopelko1, A. Konopelko8, I. J. Latham3, R. Le Gallou3, M. Lemoine11, A. Lemière7, N. Leroy11, Thomas Lohse8, A. Marcowith4, Conor Masterson1, T. J. L. McComb3, M. de Naurois6, M. de Naurois4, S. J. Nolan3, A. Noutsos3, K. J. Orford3, J. L. Osborne3, M. Ouchrif6, M. Ouchrif4, M. Panter1, Guy Pelletier14, S. Pita7, Martin Pohl17, Martin Pohl18, G. Pühlhofer1, Michael Punch7, B. C. Raubenheimer15, M. Raue5, J. Raux4, J. Raux6, S. M. Rayner3, I. Redondo19, I. Redondo11, A. Reimer17, Olaf Reimer17, J. Ripken5, M. Rivoal6, M. Rivoal4, L. Rob20, L. Rolland4, L. Rolland6, Gavin Rowell1, V. Sahakian2, L. Saugé14, S. Schlenker8, Reinhard Schlickeiser17, C. Schuster17, U. Schwanke8, M. Siewert17, Helene Sol4, R. Steenkamp21, C. Stegmann8, J.-P. Tavernet6, J.-P. Tavernet4, C. G. Théoret7, M. Tluczykont11, D. J. van der Walt15, G. Vasileiadis9, P. Vincent6, P. Vincent4, B. Visser15, Heinrich J. Völk1, Stefan Wagner 
04 Nov 2004-Nature
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

Book
01 Aug 2012
TL;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

Journal ArticleDOI
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

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
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023203
2022555
20214,841
20204,793
20194,421
20183,991