Ofer Lahav

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The expected rms bulk motion h V 2 (R *) i / Ω m 1.2 s dk P(k) W 2 (kR*) almost independent of the Cosmological Constant (<strong>Lahav</strong>, Lilje, Primack & Rees 91) Or Dark Energy (Wang & Steinhardt 98) In low density CDM smaller amplitude (σ 8 Ω m 0.6 ), larger coherence length (smaller Ω m h) than in SCDM
Wiener Filter 2MRS velocity field (CMB frame) Erdogdu et al.
Page 1 and 2: Large Scale Structure at Low Redshi
Page 3 and 4: LSS at low z • 2MRS/6dF The LG di
Page 6 and 7: 2MASS Galactic chart F
Page 8 and 9: 2MASS and follow-ups • 2MASS: 1.5
Page 10 and 11: Dipole - weighting schemes by Numbe
Page 12 and 13: Kocevski, Mullis & Ebeling, astro-p
Page 16 and 17: The revival of peculiar velocities
Page 18 and 19: 7 Abell clusters 77 groups (>8) 20
Page 20 and 21: From 2dF+CMB (6 parameter fit): Col
Page 22 and 23: Brief History of ‘Hot Dark Matter
Page 24 and 25: Data 2dFGRS Neutrino mass from Cosm
Page 26 and 27: The halo model - the ‘new biasing
Page 28 and 29: Correlation Function per Type dP /
Page 30 and 31: Imaging CFHTLS Supernovae SDSS Spec
Page 32 and 33: Input: magnitudes ANNz Collister &
Page 34 and 35: DES + VISTA griz+YJHKs filters 10σ
Page 36: Conclusions - in the Trio’s own w

Ofer Lahav

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