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.
Weak Gravitational Lensing and Cluster Counts Alexandre Refregier (CEA Saclay) Collaborators: Jason Rhodes (Caltech) Richard Massey (Cambridge) David Bacon.
Weak Gravitational Lensing by Large-Scale Structure Alexandre Refregier (Cambridge) Collaborators: Richard Ellis (Caltech) David Bacon (Cambridge) Richard.
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.
