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These are called . active. . galaxies. .. . Act...
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super-massive black hole . occupation fraction. E...
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Build-up of the red sequence of galaxies thr...
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around Abell 370, . a galaxy cluster at z = 0.37....
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metallicity. gradients . in disk galaxies from ....
. Ste. llar. . P. opulations . at intermediate ...
In this session we will continue our examination ...
diffuse X-ray emission – a survey of highly i...
The Evolution of the Tully-Fisher Relation Since ...
A ‘finger’ of the Universe’s dark-matter sk...
0. Topic: . Multiwavelength. observations. Conce...
Division of Particle and Astrophysical Science, N...
. Why Spiral Arms?. Why not just an undisturbed ...
Hubble Expansion and the Big Bang . The fact that...
COSMIC HISTORY. t = 0. :. . The Big Bang. How do...
Oleg . Gnedin. (University of Michigan. ). g. rad...
. Loners. Interactions were once . believed to...
Harrison B. Prosper. Florida State University. YS...
Spiral Structure. . The Astronomical Context. By...
megaparsecs. away be moving with respect to us, ...
D.S. . Hajdukovic. GBAR Collaboration Meeting. 18...
Physicist and communicator at CERN. The dark side...
STARLIGHT. in 1, 2 & 3D . Lesson #1. : . Go...
References:. COBE web site. WMAP web site. ...
Q. . Daniel . Wang . University . of . Massachuse...
HECTOR project scientist. Australian Astronomical...
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G. . Fabbiano. Harvard-Smithsonian Center for Ast...
the . Antarctic 10-m THz Telescope. NAKAI . Naoma...
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the Reduced Shear, . the . Pixelation. Effect, ....
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