Abstract
Future studies of: (1) galaxy property relationships, (2) environmental dependencies, and (3) the merger rate and accretion histories will require: (a) large solid angle (with large area/boundary ratio), (b) multi-band imaging, (c) high signal-to-noise and high resolution imaging, and (d) spectroscopy. All of these things will be provided by the next generation of wide-field surveys.
Original language | English (US) |
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Pages (from-to) | 379-386 |
Number of pages | 8 |
Journal | New Astronomy Reviews |
Volume | 49 |
Issue number | 7-9 |
DOIs | |
State | Published - Nov 2005 |
Keywords
- Galaxies: evolution
- Galaxies: formation
- Galaxies: structure
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science