Mass, Gas and Galaxies in the Abell 901/902 Supercluster

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The dark matter signature on the sky Matter Distant galaxies Dark Matter We can use the ‘lensing’ signature of dark matter to tell us where is it and how much if it there is. Catherine Heymans LBL 22nd Jan 2008
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Page 1 and 2: Mass, Gas and Galaxies in the Abell
Page 3 and 4: Catherine Heymans LBL 22nd Jan 2008
Page 5 and 6: The Abell 901/902 Supercluster 30x3
Page 7 and 8: QE (%) λ / nm COMBO-17 Wolf et al
Page 9 and 10: Massive ellipticals live in cluster
Page 11 and 12: Ram pressure stripping: The turbule
Page 13 and 14: 1. Galaxy-cluster gas interactions
Page 15 and 16: Seeing the invisible Meghan Gray (U
Page 17: lensed background galaxy z = 1.55 l
Page 21 and 22: A901a In this analysis we use 60,00
Page 23 and 24: What about systematics? B E Lensing
Page 25 and 26: A901b: the most massive and X-ray r
Page 27 and 28: SW group M = 3.8 ± 0.5h −1 10 13
Page 29 and 30: Mass to stellar mass ratio Catherin
Page 31 and 32: Why Hubble? ground-based Catherine
Page 33 and 34: Future telescopes in space: a quick
Page 35 and 36: STAGES: Space Telescope A901/902 Ga
Page 37 and 38: Anatomy of a supercluster: a comple
Page 39 and 40: hidden supermassive black hole Step
Page 41 and 42: Blue Galaxies Step 3: connect galax
Page 43 and 44: What causes galaxy evolution in den

Mass, Gas and Galaxies in the Abell 901/902 Supercluster

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