Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-12T11:50:07.205Z Has data issue: false hasContentIssue false

The Uses of a VLT for Complementing Observations with Radio and Space Telescopes

Published online by Cambridge University Press:  12 April 2016

Donald N.B. Hall*
Affiliation:
Space Telescope Science Institute, Baltimore, U.S.A.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is now evident that major advances in observational sensitivity in other regions of the electromagnetic spectrum invariably lead to heavy demand for complementary observations with existing large (3- to 5-meter) optical/infrared (O/IR) telescopes, and that such observations are often essential to the interpretation and understanding of phenomena revealed by the former. The Einstein X-ray mission, the International Ultraviolet Explorer (IUE), the Very Large Array (VLA) and the recent Infrared Astronomical Satellite (IRAS) are all clear demonstrations of this effect.

Type
V. Astronomical Programs For A Very Large Telescope
Copyright
Copyright © ESO 1984