XMM-Newton Large Programme Details



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
Authors marked in red are (co-)investigators in the proposal

Classification of papers are:
- 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


There are no papers associated to this proposal