Stability of Cool Cores during Galaxy Cluster Growth: A Joint Chandra/SPT Analysis of 67 Galaxy Clusters along a Common Evolutionary Track Spanning 9 Gyr
We present the results of a joint analysis of $Chandra$ X-ray and South Pole Telescope (SPT) SZ observations targeting the first sample of galaxy clusters at $0.3 < z < 1.3$, selected to be the progenitors of well-studied nearby clusters based on their expected accretion rate. We develop a...
Main Authors: | Ruppin, F, McDonald, M, Bleem, LE, Allen, SW, Benson, BA, Calzadilla, M, Khullar, G, Floyd, B |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | English |
Published: |
American Astronomical Society
2022
|
Online Access: | https://hdl.handle.net/1721.1/142177 |
Similar Items
-
Deep XMM–Newton observations of the most distant SPT-SZ galaxy cluster
by: Mantz, Adam B, et al.
Published: (2021) -
Deep XMM–Newton observations of the most distant SPT-SZ galaxy cluster
by: Mantz, Adam B, et al.
Published: (2022) -
A Detailed Study of the Most Relaxed SPT-selected Galaxy Clusters: Properties of the Cool Core and Central Galaxy
by: McDonald, M, et al.
Published: (2021) -
A Detailed Study of the Most Relaxed SPT-selected Galaxy Clusters: Properties of the Cool Core and Central Galaxy
by: McDonald, Michael A., et al.
Published: (2022) -
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2
by: Bulbul, Esra, et al.
Published: (2021)