Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-13T07:05:22.795Z Has data issue: false hasContentIssue false
  • English
  • Français

The Goddard High Resolution Spectrograph Status; Absorption lines in 3C 273

Published online by Cambridge University Press:  30 March 2016

John C. Brandt
John C. Brandt*
Affiliation:
Laboratory for Atmospheric and Space Physics University of Colorado

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.

The Goddard High Resolution Spectrograph (GHRS) is an ultraviolet spectrograph developed by the Goddard Space Flight Center and constructed by the Ball Aerospace Systems Group. The basic performance characteristics are given in Table 1. The detectors are Digicons with an approximately 500-diode linear array; the faceplate/photocathode combinations are LiF/CsI for Side 1 and MgF2/CsTe for Side 2. The two science apertures are 2x2 and 0.25 x 0.25 arc seconds square. The GHRS has several undispersed-light modes for target acquisition.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 467 - 470
Copyright
Copyright © Kluwer 1992