Slide 1Cosmological Magnetic Fields Angela V. Olinto University of Chicago Slide 2 Cosmological Fields? Were there Magnetic Fields before recombination? Slide 3 Cosmological…

Slide 1Some Secular Drivers of Galaxy Evolution (A brief, selective overview) NGC 2841, SDSS image Curt Struck Iowa State Univ., USA For the 5 th KIAS Workshop on Cosmology…

1. Design, Development, & Deployment of Wisconsin DNR Map ServicesJeff Shaw, John Laedlein, Jerry Sullivan Wisconsin Department of Natural ResourcesBureau of Technology…

1. EXTREME IMAGE OPTIMIZATIONS: WEBP AND JPEG XRIdo Safruti, Akamai [email protected] ForwardTM©2013 Akamai 2. Images make up 61% of Page Byteshttp://httparchive.org/interesting.php#bytesperpage…

1. When using charcoal and white conte on gray paper, do not blend the two. Allow the white conte to define lighter values, let the gray of the paper be a value, and use…

Slide 1P.Tisserand Rencontres du Vietnam 2006 1 Final results on galactic dark matter from the EROS-2 microlensing survey ~ 850 000 images processed - 55 million stars monitored…

Slide 1 CDM cusps in LSB galaxies by means of stellar kinematics A.Pizzella, E.M.Corsini, F. Bertola Università di Padova And J. Magorrian, M. Sarzi University of Oxford…

Slide 1 Susan CartwrightOur Evolving Universe1 Galaxy evolution n Why do galaxies come in such a wide variety of shapes and sizes? n How are they formed? n How do they evolve?…

Σπειροειδείς γαλαξίες Spiral Galaxies Compared to ellipticals, the spirals cover a distinctly smaller range in absolute magnitude (and mass). They are…

PNe as mass tracers Dark-to-luminous properties of early-type galaxies Nicola R. Napolitano Kapteyn Institute Groningen (NL) ESO workshop: PNe beyond the Milky Way. Garching…