In-orbit Vignetting Calibrations of XMM-Newton Telescopes

We describe measurements of the mirror vignetting in the XMM-Newton Observatory made in-orbit, using observations of SNR G21.5-09 and SNR 3C58 with the EPIC imaging cameras. The instrument features that complicate these measurements are briefly described. We show the spatial and energy dependences of measured vignetting, outlining assumptions made in deriving the eventual agreement between simulation and measurement. Alternate methods to confirm these are described, including an assessment of source elongation with off-axis angle, the surface brightness distribution of the diffuse X-ray background, and the consistency of Coma cluster emission at different position angles. A synthesis of these measurements leads to a change in the XMM calibration data base, for the optical axis of two of the three telescopes, by in excess of 1 arcminute. This has a small but measureable effect on the assumed spectral responses of the cameras for on-axis targets.Comment: Accepted by Experimental Astronomy. 26 pages, 18 figure

Promoting Values Development Through Community Service: A Design

Human society has become technologically complex, resulting in heightened global interdependency. However, rather than observing an era of collaboration and cooperation, we have witnessed a rise in individual and societal egocentrism (Newman, 1985 )

Investigation of shock waves in the relativistic Riemann problem: A comparison of viscous fluid dynamics to kinetic theory

We solve the relativistic Riemann problem in viscous matter using the relativistic Boltzmann equation and the relativistic causal dissipative fluid-dynamical approach of Israel and Stewart. Comparisons between these two approaches clarify and point out the regime of validity of second-order fluid dynamics in relativistic shock phenomena. The transition from ideal to viscous shocks is demonstrated by varying the shear viscosity to entropy density ratio $\eta/s$. We also find that a good agreement between these two approaches requires a Knudsen number $Kn < 1/2$.Comment: Version as published in PRC 82, 024910 (2010); 16 pages, 16 figures, typos correcte

Configuration of a Smectic A Liquid Crystal Due to an Isolated Edge Dislocation

We discuss the static configuration of a smectic A liquid crystal subject to an edge dislocation under the assumption the the director and layer normal fields ( n and a , respectively) defining the smectic arrangement are not, in general, equivalent. After constructing the energy density for the smectic, we obtain exact solutions to the equilibrium equations which result from its minimisation at quadratic order in the variables which describe the distortion, and hence a complete description of the smectic configuration across the domain of the sample. We also examine the effect of relaxing the constraint n ≡ a for different values of the constants which characterise the response of the material to distortions, and compare these results with the "classical" case considered by previous authors, in which equivalence of n and a is enforced