Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
Proposal Category
Groups of Galaxies, Clusters of Galaxies and Superclusters
Proposal Type
LARGE PROGRAM
Proposal Id
069366
Number of Observations
25
Total exposure time (ks)
745
PI Details
PI
Dr monique arnaud
Institute
CEA - Service d'Astrophysique
Country
FRANCE
Co-Investigators
Name
Country
n. Aghanim
FRANCE
g. Pratt
FRANCE
j. Democles
FRANCE
e. Pointecouteau
FRANCE
p. Mazzotta
UNITED STATES
j. Bartlett
FRANCE
I. Bikmaev
RUSSIA
H. Boehringer
GERMANY
S. Borgani
ITALY
P. Carvalho
UNITED KINGDOM
E. Churazov
GERMANY
H. Dahle
NORWAY
M. Douspis
FRANCE
S. Fromenteau
FRANCE
G. Hurier
FRANCE
C. LI
CHINA
J. Melin
FRANCE
J. Rubino Martin
SPAIN
R. Sunayev
GERMANY
S. White
GERMANY
Abstract
We propose to gather spatially resolved spectroscopy of a sample of 33 massive (M_{500}>5e+14 solar masses) clusters detected blindly by Planck and confirmed to-day to be in the redshift range 0.5
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)
