| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9827971 | New Astronomy Reviews | 2005 | 8 Pages |
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.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
David W. Hogg,