The Cosmic Flows project : voyage to the Great Attractor - LUTH

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Constraint simulations using peculiar velocities in <strong>the</strong> Initial Conditions: WF + <strong>the</strong> back in time machine RZA
SGY [Mpc/h] 160 140 120 100 80 60 40 20 0 GA Test re-‐simulaGons at z=0, box 160 Mpc/h Doumler et al. Accepted MNRAS 2012 COMA LSC 30 60 0 20 40 60 80 100 120 140 160 SGX [Mpc/h] Original simulation full box PP log(δ+1) BOX160 2.5 Y [Mpc/h] Y [Mpc/h] 100 90 80 70 60 50 40 30 100 90 80 70 60 50 40 30 2 1.5 1 0.5 0 40 50 60 70 80 90 100 110 C30_10_II_A -0.5 (with RZA) Original simulation X [Mpc/h] 40 50 60 70 80 90 100 110 X [Mpc/h] Y [Mpc/h] Y [Mpc/h] 100 90 80 70 60 50 40 30 100 90 80 70 60 50 40 30 C30_10_I_A (without RZA) 40 50 60 70 80 90 100 110 Re-simulation X [Mpc/h] no RZA E60_10_II_A (with RZA) Re-simulation with a CF1 mock Re-simulation with a CF2 mock 40 50 60 70 80 90 100 110 X [Mpc/h] 2 1.5 1 0.5 0 2 1.5 1 0.5 0
Page 1 and 2: The Cosmic Flows project : voyage t
Page 3 and 4: The large scale cosmic flows constr
Page 5 and 6: 2004 : Advent of the new giant radi
Page 7: 2008 : Cosmicflows-‐1 2012 : Co
Page 10 and 11: Results from cosmicflows-‐1 in
Page 18 and 19: CLUES 2 A simulation of the Local U
Page 20: Preliminary results (yesterday) Com
Page 23 and 24: CLUES Structure Formation with cold
Page 25 and 26: Status of Current observaGonal surv
Page 27 and 28: Preliminary results from cosmicflow
Page 29 and 30: Future surveys and simulaGons 2015
Page 31: Thank you hope you will take home s

The Cosmic Flows project : voyage to the Great Attractor - LUTH

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