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 |
- 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 |