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The UTIC Hard X-ray Balloon-borne Platform

Published online by Cambridge University Press:  25 April 2016

J. G. Greenhill ,
D. J. Watts ,
M. W. Emery ,
A. B. Giles ,
K. B. Fenton  and
S. C. Ashton
J. G. Greenhill
Affiliation:
Department of Physics, University of Tasmania
D. J. Watts
Affiliation:
Department of Physics, University of Tasmania
M. W. Emery
Affiliation:
Department of Physics, University of Tasmania
A. B. Giles
Affiliation:
Department of Physics, University of Tasmania
K. B. Fenton
Affiliation:
Department of Physics, University of Tasmania
S. C. Ashton
Affiliation:
Department of Physics, University of Tasmania
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Extract

Most of the recent advances in X-ray astronomy have resulted from satellite observations in the low energy (< 20 keV) range. The Einstein X-ray Observatory in particular has been responsible for a dramatic increase in our knowledge of the X-ray sky, in that all major classes of astronomical objects have been detected.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 460 - 465
Copyright
Copyright © Astronomical Society of Australia 1982

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