PROPOSAL OVERVIEW | |
Proposal Title | eROSITA & XMM-Newton Legacy High Redshift Cluster Survey |
Proposal Category | Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters |
Proposal Type | LARGE PROGRAM |
Proposal Id | 090447 |
Number of Observations | 17 |
Total exposure time (ks) | 1000 |
PI DETAILS | |
PI | Dr. Esra Bulbul |
Institute | MPE |
Country | GERMANY |
CO-INVESTIGATORS | ||
Name | Country | |
V. Ghirardini | GERMANY | |
A. Liu | GERMANY | |
T. Reiprich | GERMANY | |
E. Bahar | GERMANY | |
J. Sanders | GERMANY | |
F. Pacaud | GERMANY | |
K. Migkas | GERMANY | |
M. Ramos Ceja | GERMANY | |
J. Comparat | GERMANY | |
S. Shereeram | GERMANY | |
M. Brueggen | GERMANY | |
T. Pasini | GERMANY | |
T. Schrabback | GERMANY | |
J. Ider-Chitham | GERMANY | |
M. Klein | GERMANY | |
K. Dolag | GERMANY | |
S. Riccardo | GERMANY | |
J. Joshi | GERMANY | |
A. Veronica | GERMANY | |
P. Nandra | GERMANY |
ABSTRACT | |
We propose 880ks XMM-Newton observations of the most massive, bright, high-redshift galaxy clusters in the Universe detected in the first All-Sky Survey. The XMM-Newton data will enable detailed studies of the density and temperature structure of the intracluster medium (ICM) in these clusters of galaxies. Precise ICM mass measurements and temperature information will enhance the pioneering eROSITA studies of the evolution of baryons in their deep potential wells by constraining the properties of this crucial massive cluster population. Furthermore, by combining the eROSITA data with the proposed XMM-Newton follow-up observations, we will constrain the detailed structure formation process as a function of mass, redshift, and environment as well as understanding the (an-)isotropy of the Universe. |
PAPERS |
- CLASS 1: | papers that present specific XMM-Newton observations |
- CLASS 2: | papers that refer to published XMM-Newton results with complementary observations, follow-up analysis, or theoretical analysis |
- CLASS 3: | further deliveries which resulted from the program and which are made available to the community (e.g. source catalogues, processed images or spectra in public data base) |
- CLASS 4: | comments and suggestions from PI |