Weak Gravitational Lensing

More documents

Recommendations

Info

Shear-Shear Comparison: Most Consistent Subset Subset : 21 < Mag < 24.5 1.8 拻 < Size < 3.2 拻 RMS = 0.1 Slope = 0.97
Noise From the Ground and Space Noise in mass maps of the COSMOS field from the ground (left; Subaru) and space (right; HST). The ground-based map is noisier and produces ‘false positives.’ Precision lensing measurements must be done from space! From Kasliwal, Massey, Ellis, Miyazaki, and Rhodes, 2007
Page 1 and 2: Weak Gravitational Lensing Jason Rh
Page 3 and 4: Weak Gravitational Lensing Weak len
Page 5 and 6: Why Not Space? • Single facility-
Page 7 and 8: Bullet Cluster Purple is dark matte
Page 9 and 10: Abel 901/902Supercluster •Weak le
Page 11 and 12: 3-D dark matter distribution z=0.7
Page 13: Shear-Shear Comparison : All Matche
Page 17 and 18: JDEM • NASA/DOE Joint Dark Energy
Page 19 and 20: Final Questions •What aspects of

Weak Gravitational Lensing

Create successful ePaper yourself

Delete template?

Save as template?