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Institution

Humboldt University of Berlin

EducationBerlin, Germany
About: Humboldt University of Berlin is a education organization based out in Berlin, Germany. It is known for research contribution in the topics: Population & Transplantation. The organization has 33671 authors who have published 61781 publications receiving 1908102 citations. The organization is also known as: Humboldt-Universität zu Berlin & Universitas Humboldtiana Berolinensis.


Papers
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Journal ArticleDOI
TL;DR: Patients homozygous for CCR5Delta32 show longer survival of renal transplants than those with other genotypes, suggesting a pathophysiological role for C CR5 in transplant loss.

291 citations

Journal ArticleDOI
TL;DR: The DDA Reactions Catalyzed by Bases and Mechanism of the PDDA reaction 2058 and Conclusions 8.2.1.
Abstract: 2.1.3. Linker Bearing an Aromatic Ring 2053 2.2. Enynes and Diynes as Diene Component 2054 3. Photochemically Initiated DDA Reactions 2056 4. Mechanism of the DDA Reaction 2058 4.1. Mechanism of the Thermal DDA Reaction 2058 4.2. Mechanism of the PDDA reaction 2058 5. DDA Reactions Catalyzed by Bases 2058 6. Transition Metal-Catalyzed DDA reactions 2059 6.1. Rhodium and Platinum 2059 6.2. Palladium 2059 6.3. Gold 2061 7. Conclusions 2061 8. References 2062

291 citations

Journal ArticleDOI
TL;DR: In this paper, the efficacy of standard treatment with oral metronidazole in the eradication of the bacterial vaginosis biofilm was evaluated using an interventional follow-up study.

291 citations

Journal ArticleDOI
TL;DR: In this paper, the tree-level (disk) scattering amplitudes involving gauge, matter and moduli fields in IIB toroidal orbifold/orientifold backgrounds with D9-, D5- respectively D7-, D3-branes or via T-duality D6branes in type IIA compactifications were calculated.

290 citations

Journal ArticleDOI
Justin Albert1, E. Aliu, H. Anderhub2, P. Antoranz3, A. Armada, C. Baixeras4, Juan Abel Barrio3, H. Bartko5, Denis Bastieri6, Julia Becker7, W. Bednarek, K. Berger1, Ciro Bigongiari6, Adrian Biland2, R. K. Bock5, R. K. Bock6, Pol Bordas8, Valentí Bosch-Ramon8, Thomas Bretz1, I. Britvitch2, M. Camara3, E. Carmona5, Ashot Chilingarian9, J. A. Coarasa5, S. Commichau2, Jose Luis Contreras3, Juan Cortina, M. T. Costado10, V. Curtef7, V. Danielyan9, Francesco Dazzi6, A. De Angelis11, C. Delgado10, R. de los Reyes3, B. De Lotto11, E. Domingo-Santamaría, Daniela Dorner1, Michele Doro6, Manel Errando, Michela Fagiolini12, Daniel Ferenc13, E. Fernandez, R. Firpo, Jose Flix, M. V. Fonseca3, Ll. Font4, M. Fuchs5, Nicola Galante5, R. J. García-López10, M. Garczarczyk5, Markus Gaug6, Maria Giller, Florian Goebel5, D. Hakobyan9, Masaaki Hayashida5, T. Hengstebeck14, A. Herrero10, D. Höhne1, J. Hose5, C. C. Hsu5, P. Jacon, T. Jogler5, R. Kosyra5, D. Kranich2, R. Kritzer1, A. Laille13, Elina Lindfors, Saverio Lombardi6, Francesco Longo11, Jorge Andres Lopez Lopez, M. López3, E. Lorenz5, E. Lorenz2, P. Majumdar5, G. Maneva, K. Mannheim1, Oriana Mansutti11, Mosè Mariotti6, M. I. Martínez, Daniel Mazin5, C. Merck5, Mario Meucci12, M. Meyer1, Jose Miguel Miranda3, R. Mirzoyan5, S. Mizobuchi5, Abelardo Moralejo, Daniel Nieto3, K. Nilsson, Jelena Ninkovic5, E. Oña-Wilhelmi, N. Otte14, N. Otte5, I. Oya3, David Paneque5, M. Panniello10, Riccardo Paoletti12, J. M. Paredes8, M. Pasanen, D. Pascoli6, F. Pauss2, R. Pegna12, Massimo Persic15, Massimo Persic11, L. Peruzzo6, A. Piccioli12, M. Poller1, Elisa Prandini6, N. Puchades, A. Raymers9, Wolfgang Rhode7, Marc Ribó8, J. Rico, M. Rissi2, A. Robert4, S. Rügamer1, A. Saggion6, Alvaro Sanchez4, P. Sartori6, V. Scalzotto6, V. Scapin11, R. Schmitt1, T. Schweizer5, M. Shayduk5, M. Shayduk14, K. Shinozaki5, S. N. Shore16, N. Sidro, A. Sillanpää, Dorota Sobczyńska, Antonio Stamerra12, L. S. Stark2, L. O. Takalo, Petar Temnikov, D. Tescaro, Masahiro Teshima5, N. Tonello5, Diego F. Torres17, Nicola Turini12, H. Vankov, V. Vitale11, Robert Wagner5, Tadeusz Wibig, W. Wittek5, F. Zandanel6, Roberta Zanin, J. Zapatero4 
TL;DR: In this article, very high energy (VHE) gamma-ray observations of the Crab Nebula with the MAGIC telescope were reported, where the gamma spectrum can be described by a curved power law dF/dE = f(0)(E/300 GeV).
Abstract: We report about very high energy (VHE) gamma-ray observations of the Crab Nebula with the MAGIC telescope. The gamma-ray flux from the nebula was measured between 60 GeV and 9 TeV. The energy spectrum can be described by a curved power law dF/dE = f(0)(E/300 GeV)([a+b log)((E/300 GeV)])(10) with a flux normalization f(0) of (6.0 +/- 0.2(stat)) x 10(-10) cm(-2) s(-1) TeV-1, a = 2.31 +/- 0.06(stat), and b = 0.26 +/- 0.07(stat). The peak in the spectral energy distribution is estimated at 77 +/- 35 GeV. Within the observation time and the experimental resolution of the telescope, the gamma-ray emission is steady and pointlike. The emission's center of gravity coincides with the position of the pulsar. Pulsed gamma-ray emission from the pulsar could not be detected. We constrain the cutoff energy of the pulsed spectrum to be less than 27 GeV, assuming that the differential energy spectrum has an exponential cutoff. For a superexponential shape, the cutoff energy can be as high as 60 GeV.

290 citations


Authors

Showing all 34115 results

NameH-indexPapersCitations
Karl J. Friston2171267217169
Peer Bork206697245427
Raymond J. Dolan196919138540
Stefan Schreiber1781233138528
Andreas Pfeiffer1491756131080
Thomas Hebbeker1481984114004
Thomas Lohse1481237101631
Jean Bousquet145128896769
Hermann Kolanoski145127996152
Josh Moss139101989255
R. D. Kass1381920107907
W. Kozanecki138149899758
U. Mallik137162597439
C. Haber135150798014
Christophe Royon134145390249
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023208
2022747
20214,727
20204,083
20193,579
20183,143