| PROPOSAL OVERVIEW | |
| Proposal Title | X-EDFF |
| Proposal Category | Cosmology, Extragalactic Deep Fields and Large Extragalactic Areas |
| Proposal Type | UNDEFINED |
| Proposal Id | 094121 |
| Number of Observations | 2 |
| Total exposure time (ks) | 3576 |
| PI DETAILS | |
| PI | Dr. Marguerite Pierre |
| Institute | CEA Paris-Saclay |
| Country | FRANCE |
| CO-INVESTIGATORS | ||
| Name | Country | |
| J. Brinchmann | PORTUGAL | |
| L. Chiappetti | ITALY | |
| J. Cuillandre | FRANCE | |
| S. Ettori | ITALY | |
| N. Hatch | UNITED KINGDOM | |
| H. Hoekstra | NETHERLANDS | |
| E. Koulouridis | GREECE | |
| M. Maturi | GERMANY | |
| S. Maurogordato | FRANCE | |
| Y. Mellier | FRANCE | |
| L. Moscardini | ITALY | |
| T. Nagano | JAPAN | |
| F. Pacaud | GERMANY | |
| E. Piconcelli | ITALY | |
| S. Pires | FRANCE | |
| E. Pouliasis | GREECE | |
| T. Schrabback | AUSTRIA | |
| Y. Toba | JAPAN | |
| I. Valtchanov | SPAIN | |
| C. Vignali | ITALY | |
| ABSTRACT | |
| The 10 deg2 Euclid Deep Fornax Field (EDFF) will be the foremost extragalactic medium-area deep field due to its unique multi-lambda coverage. We aim to provide the X-ray view by mapping the entire EDFF at 40ks depth for untold legacy value. The XMM data and associated surveys will enable major advances in the study of AGN and galaxy clusters, including: deep characterisation of Euclid clusters and their selection function; robust measures of cluster scaling relations to z=1.5 and the group regime; the study of rare clusters and AGN in a variety of environments; and revealing the link between AGN feedback and star formation to z>3. We will deliver a complete, validated multi-lambda legacy dataset that will greatly enhance the AGN and cluster science from the 15,000 deg2 Euclid Wide survey. | |
| 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 |