| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780051 | New Astronomy Reviews | 2006 | 7 Pages |
Abstract
Here is discussed various ways by which the cosmic microwave background (CMB) radiation can be use to measure the velocities of matter in the universe. We include some new statistical techniques for using the kinetic Sunyaev-Zel'dovich (kSZ) effect and integrated Sachs-Wolfe (ISW) effect to determine velocities by correlating wide area CMB maps with overlapping large-scale structure (LSS) surveys.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Albert Stebbins,