XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Studying the Progenitors of Our Favorite Clusters at z>1
Proposal Category Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters
Proposal Type LARGE PROGRAM
Proposal Id 86264
Number of Observations 16
Total exposure time (ks) 447

PI DETAILS
PI Dr Adam Mantz
Institute Stanford University
Country UNITED STATES

CO-INVESTIGATORS
Name Country
M. McDonald UNITED STATES
S. Allen UNITED STATES
G. Morris UNITED STATES
R. Canning UNITED STATES
E. Noordeh UNITED STATES
M. Brodwin UNITED STATES
A. Stanford UNITED STATES

ABSTRACT
Surveys in the 2020s, notably the CMB-S4 program and Athena, will reveal galaxy clusters at high redshifts, all the way back to z~3, when they first formed. Unveiling the properties (density, temperature, entropy, metallicity) and evolution of the intracluster medium and the galaxy-halo connection in these early-forming systems will be among the primary science goals of both Athena and any Chandra successor. While many of the most exciting questions about the initial formation of galaxy clusters must wait for next-generation X-ray missions, we can lay an important foundation now by extending studies of statistical cluster samples into the z>1 regime.

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