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Technical Report: The Fastest Relativistic Jets from Quasars and Active Galactic Nuclei
Authors:B Glenn Piner
Institution:Department of Physics and Astronomy , Whittier College , Whittier, CA, USA
Abstract:This workshop was held to gather scientists interested in exploiting beamlines I06 and I10 of the Surface and Interfaces Village at Diamond Light Source from June 10–11, 2009. Sarnjeet Dhesi introduced the meeting with a short explanation of the village structure at Diamond. This village includes the Nanoscience beamline (I06), catering for soft X-rays for Photo-Emission Electron Microscopy (PEEM) and X-ray Magnetic Circular and Linear Dichroism (XMCD and XMLD), and the Beam Line for Advanced Dichroism Experiments (BLADE, beamline I10), which is a polarized soft X-ray beam for XMCD, XMLD, and soft X-ray diffraction. I06 has been operational for over two years, while I10 is scheduled to come on-line in late 2010. In addition, there are two surface science beamlines (I07 and I09) in the village dedicated to surface diffraction and X-ray standing waves.
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