Ofer Lahav

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Data 2dFGRS Neutrino mass from Cosmology WMAP+2dF+… WMAP+2dFnew SDSS+WMAP Ly-α + SDSS+ WMAP WMAP alone Authors Elgaroy et al. 02 Spergel et al. 03 Sanchez et al. 05 Tegmark et al. 04 Seljak et al. 04 Ichikawa et al. 04 All upper limits 95% CL, but different assumed priors ! Mν = Σ mi < 1.8 eV < 0.7 eV < 1.2 eV < 1.7 eV < 0.4 eV < 2.0 eV
Halo model for LSS Picture credit: Cooray & Sheth (2002)
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 14 and 15: The expected rms bulk motion h V 2
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 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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