TY - JOUR A1 - Romoli, Carlo A1 - Chakraborty, Nachiketa A1 - Dorner, Daniela A1 - Taylor, Andrew A1 - Blank, Michael T1 - Flux Distribution of Gamma-Ray Emission in Blazars: The Example of Mrk 501 JF - Galaxies N2 - Flux distribution is an important tool to understand the variability processes in activegalactic nuclei. We now have available a great deal of observational evidences pointing towards thepresence of log-normal components in the high energy light curves, and different models have beenproposed to explain these data. Here, we collect some of the recent developments on this topic usingthe well-known blazar Mrk 501 as example of complex and interesting aspects coming from its fluxdistribution in different energy ranges and at different timescales. The observational data we refer toare those collected in a complementary manner by Fermi-LAT over multiple years, and by the FirstG-APD Cherenkov Telescope (FACT) telescope and the H.E.S.S. array in correspondence of the brightflare of June 2014 KW - gamma rays KW - very high energy KW - active galactic nuclei KW - Markarian 501 KW - monitoring KW - flux distributions Y1 - 2018 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-197580 SN - 2075-4434 VL - 6 IS - 4 ER - TY - JOUR A1 - Schumann, Sarah A1 - Eberlein, Uta A1 - Muhtadi, Razan A1 - Lassmann, Michael A1 - Scherthan, Harry T1 - DNA damage in leukocytes after internal ex-vivo irradiation of blood with the α-emitter Ra-223 JF - Scientific Reports N2 - Irradiation with high linear energy transfer α-emitters, like the clinically used Ra-223 dichloride, severely damages cells and induces complex DNA damage including closely spaced double-strand breaks (DSBs). As the hematopoietic system is an organ-at-risk for the treatment, knowledge about Ra-223-induced DNA damage in blood leukocytes is highly desirable. Therefore, 36 blood samples from six healthy volunteers were exposed ex-vivo (in solution) to different concentrations of Ra-223. Absorbed doses to the blood were calculated assuming local energy deposition of all α- and β-particles of the decay, ranging from 0 to 142 mGy. γ-H2AX + 53BP1 co-staining and analysis was performed in leukocytes isolated from the irradiated blood samples. For DNA damage quantification, leukocyte samples were screened for occurrence of α-induced DNA damage tracks and small γ-H2AX + 53BP1 DSB foci. This revealed a linear relationship between the frequency of α-induced γ-H2AX damage tracks and the absorbed dose to the blood, while the frequency of small γ-H2AX + 53BP1 DSB foci indicative of β-irradiation was similar to baseline values, being in agreement with a negligible β-contribution (3.7%) to the total absorbed dose to the blood. Our calibration curve will contribute to the biodosimetry of Ra-223-treated patients and early after incorporation of α-emitters. KW - alpha particles KW - blood KW - DNA Breaks KW - double-stranded KW - gamma rays KW - healthy volunteers KW - humans KW - leukocytes KW - radiation effects KW - radium Y1 - 2018 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-175596 VL - 8 IS - 2286 ER - TY - THES A1 - Summa, Alexander T1 - Modelling high-energy observables of supernova explosions T1 - Modellierung hochenergetischer Beobachtungsgrößen von Supernova-Explosionen N2 - In this work, high-energy observables arising during different phases of SN explosions are studied with respect to their potential for allowing conclusions on suggested explosion scenarios and physical mechanisms that are thought to influence the evolution of SNe in a major way. The focus on selected observables at keV and MeV energies is motivated by the appearance of large degeneracies that can even be found for disparate scenarios in many wavelength regimes. Since the discussed emission in the high-energy regime is directly linked to nuclear processes being usually very distinct for different suggested physical models, the signatures at keV and MeV energies allow for meaningful comparisons of simulations with observations. N2 - In der vorliegenden Arbeit werden Hochenergie-Beobachtungsgrößen, die während verschiedener Phasen von Supernova-Explosionen entstehen, hinsichtlich der Möglichkeit von Rückschlüssen auf vorgeschlagene Explosionsszenarien und physikalische Mechanismen, welche einen wichtigen Einfluss auf die Entwicklung dieser Explosionen ausüben, untersucht. Die Schwerpunktsetzung auf Beobachtungsgrößen im keV- und MeV-Energiebereich ist dabei durch die großen Ähnlichkeiten begründet, die grundverschiedene Szenarien in ihrer Emission in vielen Wellenlängenbereichen zeigen. Da die diskutierten Beobachtungsgrößen im Hochenergie-Bereich direkt mit nuklearen Prozessen verknüpft sind, die bei unterschiedlichen physikalischen Modellen sehr charakteristisch ausgeprägt sein können, eignen sich gerade die vorgestellten Signaturen im keV- und MeV-Bereich für aussagekräftige Vergleiche von Simulationen und Beobachtungen. KW - Supernova KW - Hochenergieastronomie KW - supernovae KW - nucleosynthesis KW - gamma rays KW - X-rays KW - cosmic rays KW - Nukleosynthese KW - Gammastrahlung KW - Röntgenstrahlung KW - Kosmische Strahlung Y1 - 2014 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-94608 ER -