Colour Theory
Stochastic Gravitational Lensing and the Nature of Dark Matter Chuck Keeton Rutgers University Gravitational lens database -- .
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Physics at KIPAC Steven M. Kahn SLUO Annual Meeting 6 July 2004.
How do we transform between accelerated frames? Consider Newton’s first and second laws: m i is the measure of the inertia of an object – its resistance.
Deriving and fitting LogN-LogS distributions Andreas Zezas Harvard-Smithsonian Center for Astrophysics.
On the Distribution of Dark Matter in Clusters of Galaxies David J Sand Chandra Fellows Symposium 2005.
The Large Synoptic Survey Telescope Steven M. Kahn Presentation to the SLAC Program Review Committee - June 2, 2004.
Suzaku search for evidence of sterile neutrinos in the X-ray spectra of dwarf spheroidal galaxies Michael Loewenstein, Alexander Kusenko (UCLA), Peter.
THE DARK SIDE OF THE FORCE - THE DARK SIDE OF THE FORCE - Black Holes and Dark Matter Weldon J. Wilson Department of Physics & Engineering University of.
Microsoft DryadLINQ --Jinling Li. What’s DryadLINQ? A System for General-Purpose Distributed Data-Parallel Computing Using a High-Level Language. [1]
The Stellar Populations, Mass-to-Light Ratios and Dark Matter in Spiral Galaxies Roelof S. de Jong Steward Observatory Eric Bell Rob Kennicutt Rob Swaters.
![Microsoft DryadLINQ --Jinling Li. What’s DryadLINQ? A System for General-Purpose Distributed Data-Parallel Computing Using a High-Level Language. [1]](https://static.fdocuments.in/doc/330x215/56649e2d5503460f94b1ce42/microsoft-dryadlinq-jinling-li-whats-dryadlinq-a-system-for-general-purpose.jpg)
