THE E-ELT DESIGN REFERENCE MISSION
DRM PROPOSALS
The following is the list of DRM proposals for the science cases chosen by the SWG for the DRM:
- Planets & Stars
- S3: From giant to terrestrial exoplanets: detection,
characterization and evolution
- Direct imaging of terrestrial and giant exoplanets (demo case; v1: 04 Mar 2008)
- Earth twins in the habitable zone of solar-type stars
- Rocky planets in the habitable zones of low-mass stars and brown dwarfs
- Physical properties of Earth-sized planets
- S9: Circumstellar disks
- Imaging the planet-forming regions of circumstellar disks (v1: 04 Mar 2008)
- Dynamics and chemical evolution of circumstellar disks (v1: 04 Mar 2008)
- S5: Young stellar clusters (incl. Galactic Centre)
- Characterizing the lowest mass freely floating objects in star forming regions (v2: 21 Apr 2008)
- The Centers of Massive Dense Young Clusters: deep ELT infrared imaging and 3D spectroscopy (v1: 16 Mar 2008)
- Giant-planet-mass objects in the Large Magellanic Cloud (v2: 21 Apr 2008)
- S3: From giant to terrestrial exoplanets: detection,
characterization and evolution
- Stars & Galaxies
- G4: Imaging and spectroscopy of resolved stellar
populations in galaxies
- The Resolved Stellar Populations of Elliptical Galaxies (demo case; v1: 04 Mar 2008)
- The Chemo-Dynamical Structure of Galaxies (v1: 04 Mar 2008)
- First Stars relics in the Milky-Way and satellites (v1: 04 Mar 2008)
- G9: Black holes / AGN
- A Survey of Black Holes in Different Environments (v1: 04 Mar 2008)
- G4: Imaging and spectroscopy of resolved stellar
populations in galaxies
- Galaxies & Cosmology
- C10: The physics of high redshift galaxies
- The Physics and Mass Assembly of Galaxies out to z ~ 6 (demo case; v1: 04 Mar 2008)
- High resolution imaging of high redshift galaxies (v1: 04 Mar 2008)
- ELT integrated spectroscopy of early-type galaxies at z > 1 (v1: 04 Mar 2008)
- C4: First light – the highest redshift galaxies
- First light – the highest redshift galaxies (v2: 22 Mar 2010)
- C7: Is the low-density intergalactic medium metal enriched?
- Is the low-density intergalactic medium at z ~ 2-3 metal enriched? (v1: 04 Mar 2008)
- C2: A dynamical measurement of the expansion history of the Universe
- C10: The physics of high redshift galaxies
The letter/number combinations refer to the science case designations in the SWG's first report.
E-ELT Science
What's New?
- 05 Dec 2014
Spending on first construction phase approved
Science Case
Project Science Team
Phase B (2006 – 2011)
- Science Working Group
- Design Reference Mission
- Design Reference Science Plan
- Tools: Imaging ETC / Spectroscopic ETC / Other software