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high resolution Milky Way dark matter halos simulated on NASA's Columbia and ORNL's Jaguar supercomputers |
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VL-2 publications
Clumps and streams in the local dark matter distributionDiemand J., Kuhlen M., Madau P., Zemp M., Moore B., Potter D., Stadel J., 2008, Nature, 454, 735-738, astro-ph/0805.1244
The dark matter annihilation signal from galactic substructure: Predictions for GLAST
Kuhlen M., Diemand J., Madau P. 2008, ApJ in press, astro-ph/0805.4416
VL-1 publications
Dark matter substructure and gamma-ray annihilation in the Milky Way haloDiemand, J., Kuhlen, M., & Madau, P. 2007, ApJ, 657, 262, astro-ph/0611370 pdf
Formation and evolution of galaxy dark matter halos and their substructure
Diemand, J., Kuhlen, M., & Madau, P. 2007, ApJ, 667, 859, astro-ph/0703337 pdf erratum pdf
Redefining the Missing Satellites Problem
Strigari, L. E., Bullock, J. S., Kaplinghat, M., Diemand, J., Kuhlen, M., & Madau, P. 2007, ApJ, 669, 676, astro-ph/0704.1817
The shapes, orientation, and alignment of Galactic dark matter subhalos
Kuhlen, M., Diemand, J., & Madau, P. 2007, ApJ, 671, 1135, astro-ph/0705.2037
Dark matter subhalos and dwarf satellites
Madau, P., Diemand, J., & Kuhlen, M. 2008, ApJ, 679, 1260, astro-ph/0802.2265
Infall caustics in dark matter halos?
Diemand, J., & Kuhlen, M. 2008, ApJ in press, astro-ph/0804.4185
publications using via lactea data
The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite ProblemSimon, J. D., & Geha, M. 2007, ApJ, 670, 313, astro-ph/0706.0516
The Most Dark Matter Dominated Galaxies: Predicted Gamma-ray Signals from the Faintest Milky Way Dwarfs
Strigari, L. et al. 2007, ApJ, 678, 614, astro-ph/0709.1510
Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function
Tollerud, E. et al. 2008, ApJ submitted, astro-ph/0806.4381
Spin-independent elastic WIMP scattering and the DAMA annual modulation signal
Fairbairn M., Schwetz T., 2008, hep-ph/0808.0704
... let us know about other papers which should be posted here ...
last updated: August 6, 2008, by J. Diemand
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