XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Completing and Ensuring Major Impact from the XMM-SERVS Survey
Proposal Category Cosmology, Extragalactic Deep Fields and Large Extragalactic Areas
Proposal Type UNDEFINED
Proposal Id 082038
Number of Observations 2
Total exposure time (ks) 3444

PI DETAILS
PI Prof William Brandt
Institute Pennsylvania State University
Country UNITED STATES

CO-INVESTIGATORS
Name Country
C. Chen UNITED STATES
B. Luo CHINA
F. Vito UNITED STATES
G. Yang UNITED STATES
J. Aird UNITED KINGDOM
D. Alexander UNITED KINGDOM
M. Banerji UNITED KINGDOM
F. Bauer CHILE
K. Chow AUSTRALIA
M. Cirasuolo UNITED KINGDOM
A. Comastri ITALY
A. Del Moro GERMANY
G. Garmire UNITED STATES
R. Gilli ITALY
M. Huynh AUSTRALIA
M. Jarvis UNITED KINGDOM
M. Lacy UNITED STATES
B. Lehmer UNITED STATES
J. Mullaney UNITED KINGDOM
R. Norris AUSTRALIA

ABSTRACT
We propose to complete our 12 deg^2 survey at 50 ks depth of three legacy sky regions: the SERVS areas of W-CDF-S, ELAIS-S1, and XMM-LSS. XMM-LSS won a 1.3 Ms AO-15 allocation. W-CDF-S and ELAIS-S1 coverage is now integrally required so that XMM-SERVS can dramatically advance studies of SMBH growth across the full range of cosmic environments, links between SMBH accretion and host-galaxy properties, groups/clusters at z = 0.1-2, protoclusters, and other topics. XMM-SERVS will allow outstanding studies of the newly detected 9000 AGNs and 760 X-ray groups/clusters by powerfully leveraging its superior radio-to-UV coverage, and its fields will have extraordinary legacy value as MOONS massive spectroscopy fields, DES/LSST deep-drilling fields, and prime ALMA fields.

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