For the production of movies for the Adler planetarium Chicago we were rerunning the Box 64 - 10909 simulation (dark matter only) on the pleiades computer of NAS Ames. For this special purpose 7200 outputs in equal distance delta_a_expn = 0.0001362 were stored. The movie shows the evolution of the Local Group in spherical projection. Credit: CLUES team and C. Henze, N. McCurdy, J. Primack Fast preview movie [avi, 1024x1024, 4.4 MB] Full resolution [mpg, 1024x1024, 134 MB] Lower quality [mp4, 1024x1024, 23 MB] Snapshot [jpg, 1024x1024, 109 KB]
	Same as above, but no spherical projection. At the end of evolution the camera zooms inward and the Local Group, Virgo Cluster and Fornax are labeled. Credit: CLUES team and C. Henze, N. McCurdy, J. Primack Fast preview movie [avi, 1024x1024, 9.3 MB] Full resolution [mp4, 1024x1024, 345 MB] Full resolution [webm, 1024x1024, 25 MB] Medium resolution [mp4, 640x640, 113 MB] Low resolution [mp4, 320x320, 29 MB] Snapshot [jpg, 1024x1024, 113 KB]
	Flight through the whole simulation box, WMAP5 (dark matter only, Box 64 - 10909. Visualized using pgplot. Credit: G. Yepes and the CLUES team [avi, 1520x1142, 17 MB]
	Evolution of Andromeda (center), Milky Way (upper right) and M33 (lower right) in a ~ 2 Mpc/h box (Box 64 - 186592), starting at redshift z=42. The colours represent the dark matter density. A similar movie for the gas density evolution can be found in the Gas-section. Visualized using PMViewer. Credit: K. Riebe and the CLUES team [avi, 1024x768, 27 MB]
	Evolution of Milky Way and Andromeda Galaxy (M31) in a 1.5 Mpc box (Box 64 - 10909). Visualized using pgplot. Credit: G. Yepes and the CLUES team [avi, 1520x1140, 19 MB]
	Evolution of M31 in a 250 kpc box (Box 64 - 10909). Visualized using pgplot. Credit: G. Yepes and the CLUES team [avi, 1520x1142, 19 MB]
	Evolution of the Milky Way in a 250 kpc box (Box 64 - 10909). Visualized using pgplot. Credit: G. Yepes and the CLUES team [avi, 1520x1142, 19 MB]
	A comparison between cold and warm dark matter, Box 64 - 186592. Visualized using PMViewer. Credit: A. Khalatyan and the CLUES team [avi, 720x576, 8.8 MB]
	Comparison between cold and warm dark matter for the three main halos of the Local Group, Box 64 - 186592. Visualized using PMViewer. Credit: A. Khalatyan and the CLUES team [avi, 640x480, 2.3 MB]
	Comparison of dark matter (left) and gas (right) density distribution of the Local Group at z=0 (Box 64 - 186592, 2048^3 particles effective resolution). Visualized using PMViewer. Credit: K. Riebe and the CLUES team [avi, 1220x610, 38 MB] [avi, 1024x512, 38 MB]
	A flight through the whole simulation box (dark matter distribution), Box 64 - 186592. Visualized using pgplot. Credit: G. Yepes and the CLUES team [avi, 1520x1142, 16 MB]