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pro vyhledávání: '"KIRSCH, m"'
A large-volume Time Projection Chamber (TPC) is the main tracking and particle identification (PID) detector of the ALICE experiment at the CERN LHC. PID in the TPC is performed via specific energy-loss measurements (dE/dx), which are derived from th
Externí odkaz:
http://arxiv.org/abs/2312.13781
Publikováno v:
In Journal de Traumatologie du Sport June 2023 40(2):99-103
Publikováno v:
In Gondwana Research June 2022 106:191-210
Publikováno v:
In Experimental Thermal and Fluid Science April 2019 102:152-162
Autor:
Martin-Carrillo, A., Kirsch, M. G. F., Caballero, I., Freyberg, M. J., Ibarra, A., Kendziorra, E., Lammers, U., Mukerjee, K., Schönherr, G., Stuhlinger, M., Saxton, R. D., Staubert, R., Suchy, S., Wellbrock, A., Webb, N., Guainazzi, M.
Reliable timing calibration is essential for the accurate comparison of XMM-Newton light curves with those from other observatories, to ultimately use them to derive precise physical quantities. The XMM-Newton timing calibration is based on pulsar an
Externí odkaz:
http://arxiv.org/abs/1204.0978
Autor:
Duro, R., Dauser, T., Wilms, J., Pottschmidt, K., Nowak, M. A., Fritz, S., Kendziorra, E., Kirsch, M. G. F., Reynolds, C. S., Staubert, R.
We present the analysis of the broadened, flourescent iron Kalpha line in simultaneous XMM-Newton and RXTE data from the black hole Cygnus X-1. The XMM-Newton data were taken in a modified version of the timing mode of the EPIC-pn camera. In this mod
Externí odkaz:
http://arxiv.org/abs/1108.1157
Autor:
Miceli, M., Bocchino, F., Iakubovskyi, D., Orlando, S., Telezhinsky, I., Kirsch, M. G. F., Petruk, O., Dubner, G., Castelletti, G.
Efficient particle acceleration can modify the structure of supernova remnants. In this context we present the results of the combined analysis of the XMM-Newton EPIC archive observations of SN 1006. We aim at describing the spatial distribution of t
Externí odkaz:
http://arxiv.org/abs/0903.3392
Autor:
Petruk, O., Dubner, G., Castelletti, G., Bocchino, F., Iakubovskyi, D., Kirsch, M. G. F., Miceli, M., Orlando, S., Telezhinsky, I.
A number of important processes taking place around strong shocks in supernova remnants (SNRs) depend on the shock obliquity. The measured synchrotron flux is a function of the aspect angle between interstellar magnetic field (ISMF) and the line of s
Externí odkaz:
http://arxiv.org/abs/0811.2319
Autor:
Actis, O., Erdmann, M., Fischer, R., Hinzmann, A., Kirsch, M., Klimkovich, T., Müller, G., Plum, M., Steggemann, J.
VISPA is a novel development environment for high energy physics analyses, based on a combination of graphical and textual steering. The primary aim of VISPA is to support physicists in prototyping, performing, and verifying a data analysis of any co
Externí odkaz:
http://arxiv.org/abs/0810.3609
We present a procedure for reconstructing particle cascades from event data measured in a high energy physics experiment. For evaluating the hypothesis of a specific physics process causing the observed data, all possible reconstruction versions of t
Externí odkaz:
http://arxiv.org/abs/0801.1302