Constraints on the Optical Depth of Galaxy Groups and Clusters
Future data from galaxy redshift surveys, combined with high-resolutions maps of the cosmic microwave background, will enable measurements of the pairwise kinematic Sunyaev-Zel'dovich (kSZ) signal with unprecedented statistical significance. This signal probes the matter-velocity correlation fu...
Main Authors: | Flender, Samuel (Author), Nagai, Daisuke (Author), McDonald, Michael A. (Contributor) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2017-06-05T17:57:20Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
by: McDonald, Michael, et al.
Published: (2020) -
REVISED MASS-TO-LIGHT RATIOS FOR NEARBY GALAXY GROUPS AND CLUSTERS
by: Shan, Yutong, et al.
Published: (2015) -
The Evolution of AGN Activity in Brightest Cluster Galaxies
by: McDonald, Michael
Published: (2022) -
OPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY
by: Bautz, Marshall W., et al.
Published: (2015) -
Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
by: Renneby, Malin, et al.
Published: (2022)