2008-5-20IVOA Interoperability Meeting, Trieste1 Mining data using MATLAB through AstroBox Chao LIU, Chenzhou CUI Presented by: Chenzhou CUI National Astronomical.
Edelweiss-II : status and first results A new generation of background-free bolometers for WIMP search X-F. Navick - CEA Saclay, IRFU, France LTD13 – Stanford.
" The Maximum Likelihood Problem and Fitting the Sagittarius Dwarf Tidal Stream " Matthew Newby Astronomy Seminar RPI Oct. 22, 2009 1.
Observational Constraints on Hot Gas Accretion Joel Bregman University of Michigan Collaborators: Mike Anderson, Xinyu Dai.
Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, [email protected] 1 Aldo Morselli INFN, Sezione di Roma 2 & Università.
One tenth solar_abundances_along_the_body_of-the_stream
Caltech Composite Inelastic Dark Matter
Experimental Searches for Dark Matter
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Our milky way
Combined Energy Spectra of Flux and Anisotropy Identifying Anisotropic Source Populations of Gamma-rays or Neutrinos Sheldon Campbell The Ohio State University.
Status of Top-Down Models for the Origin of Ultra-High Energy Cosmic Rays I. Observation of ultra-high energy cosmic rays before the Pierre Auger Observatory.
