In order to probe the formation of these relations, we require a complete analysis of both galaxies and their environments. This can only be achieved using the highly complete spectroscopic samples required to identify cluster, group, pair, filament and void structures as well as the galaxies that reside within them. DEVILS will achieve this by combining a deep, highly complete (>95%), magnitude limited (Y-mag<21.2) spectroscopic sample with extensive multi-wavelength imaging across a broad range of wavelengths. The survey is designed to detect M∗z=0 (1010.7M⊙) galaxies to z = 1, major merger satellites of M∗z=0 galaxies to z = 0.7, and 1013M⊙ groups to z = 0.7. DEVILS will probe the evolution of dark matter and the impact of environment on galaxy evolution over an extensive ∼ 8Gyr baseline. This unique survey will also provide a diverse legacy resource for galaxy evolution science. DEVILS will open up new avenues of discovery, focusing on two key science projects:
- The influence of environment in regulating galaxy evolution at 0.3 < z < 0.8
- The evolution of the dark matter distribution using the most massive groups and clusters
DEVILS Target Fields
Name |
Common Name |
RA
|
Dec
|
RA
|
Dec
|
Observable (AAT) |
Input Band |
Input Depth |
Input Survey |
---|---|---|---|---|---|---|---|---|---|
D02 | XMM-LSS | 35.4975 | -4.825 | 02:21:59 | -04:49:30 | Sept-Dec | VISTA-Y | Y<21.2 | VIDEO |
D03 | ECDFS | 53.65 | -28.1 | 03:34:36 | -28:06:00 | Sept-Jan | VISTA-Y | Y<21.2 | VIDEO |
D10 | COSMOS | 150.1 | 2.1 | 10:00:24 | 02:06:00 | Jan-April | VISTA-Y | Y<21.2 | UltraVISTA |