Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2025-01-06T02:18:59.781Z Has data issue: false hasContentIssue false
  • English
  • Français

Techniques for improving the sensitivity of proportional counters used in X-ray astronomy

Published online by Cambridge University Press:  14 August 2015

P. W. Sanford ,
A. M. Cruise  and
J. L. Culhane
P. W. Sanford
Affiliation:
Mullard Space Science Laboratory, University College of London, London, England
A. M. Cruise
Affiliation:
Mullard Space Science Laboratory, University College of London, London, England
J. L. Culhane
Affiliation:
Mullard Space Science Laboratory, University College of London, London, England

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 discovery and measurement of cosmic X-ray sources has almost invariably been performed with proportional counters which have large window areas. In the energy range from 1 to 50 keV, proportional counters have advantages over other types of detectors; they provide energy resolution and they can be made relatively easily with very large window areas.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 35 - 40
Copyright
Copyright © Reidel 1970 

References

[1] Mathieson and Sanford: 1963, Proc. Inst. Symp. Nuclear Electronics, Paris p. 65 Google Scholar
[2] University College London Proposal for the ESRO TD1 Satellite.Google Scholar