PPT-The GALEX Ultraviolet Virgo Cluster Survey (

GUViCS IV The role of the cluster environment on galaxy evolution Speaker Xinkai Chen Sample Sample Extended Source Catalogue of Voyer14 recessional velocity lt 3500kms1 Virgo cluster region. Patrick Ogle and the NED . Team. IPAC, California Institute of Technology. NASA Extragalactic Database (NED). A fusion of multi-wavelength extragalactic data from journal articles and large catalogs. dense cloud decoupling & evidence for magnetic binding in the ISM. Jeff Kenney (Yale). Anne Abramson. Hector Bravo-Alfaro. Jacqueline van . Gorkom. partially . strips large spirals in Virgo-like . ENVIRONMENT. . The High Performance Computing environment consists of high-end systems used for executing complex number crunching applications for research it has two such machines and they are,. . VG. So we want a color magnitude diagram for AGN so that by looking at the color of an AGN we can get its luminosity. But AGN have no fusion, why would we expect a color-magnitude relation?. The gas that accretes onto the black hole is still hot and so must follow the Blackbody Radiation law. . CCPM. What is the CCPM?. A self-assessment of cluster performance against the 6 core cluster functions and Accountability to Affected populations:. support service delivery . inform the HC/HCT's strategic decision-making . Ultraviolet (UV) light falls in the range of the EM spectrum between visible light and X-rays. UV . light, which comes from the sun, is invisible to the human eye. .. It . makes black-light posters glow, and is responsible for summer tans — and sunburns. Neutron number (N). Proton number (Z). University of York. (Replace with institution name) . Nuclear physics in stars. The CNO cycle – catalysts for stars. HotCNO. . Where do heavy elements come from?. Kepler, . Ticho. Brahe, . Copernicus. Galileo, Newton. Einstein, . Eötvos. Amaldi. & the . resonating. . antennas. The era of . interferometers. : . . GEO600 & VIRGO in EU. . LIGO in USA, TAMA in Japan. European Gravitational Observatory. EGO. “Raison d'être”, origin, structure . & future perspectives. Federico Ferrini . – EGO Director. Welcome to. The Einstein Telescope. Design Study Presentation. Lazar Kirchev. March 26. th. , 2013. photo: Werner Kunz. , http://www.flickr.com/photos/werkunz/5748357415. /. Agenda. Virgo server background. Virgo distributions. Web Admin Console. Enabling enterprise applications in Virgo. Fornax and Virgo Clusters Gas Dynamics Merger History and Elemental EnrichmentR Kraft1Y Su1T Fish21A Sheardown2E Roediger21W Forman1C Jones1P Nulsen1E Churazov3 S Randall1 EBulbul11Smithsonian Astrop Special Meeting on 1. st. April 2015 @ 10AM. UNHCR Kabul Office. Cluster Coordination Performance Monitoring. What is the CCPM?. A self-assessment of cluster performance against the 6 core cluster functions and Accountability to Affected populations:. radiaton. , through different types of filters. . UV & . Sunblock. Measuring and comparing the level of ultraviolet radiation, through different types of filters.. Objective. The purpose of this activity is to study the level of ultraviolet radiation resulting from the intervention of a sunlight beam through different types of filters, creating a hypothesis and proceeding to test it using the . . CS APC. Virgo and LIGO in the . next. . decade. Data . takings. . alternated. to upgrades, . pushing. . current. infrastructure to . limits. Program . until. . ~ 2030 . CS APC. 2. Einstein .