Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-06T01:07:57.576Z Has data issue: false hasContentIssue false
  • English
  • Français

Ground-based Gamma-ray Astronomy

Published online by Cambridge University Press:  25 April 2016

R.W. Clay  and
B.R. DawSOn
R.W. Clay
Affiliation:
Department of Physics and Mathematical Physics, University of Adelaide, GPO Box 498, Adelaide SA 5001
B.R. DawSOn
Affiliation:
Department of Physics and Mathematical Physics, University of Adelaide, GPO Box 498, Adelaide SA 5001
Get access Rights & Permissions [Opens in a new window]

Abstract

Ground-based gamma-ray astronomy has slowly developed over the past quarter of a century to a position now where a number of sources are known to produce gamma-rays in the energy range 1011eV to 1018eV. The observations are difficult, with exceptional signal to noise problems, but improved techniques are now allowing observers to proceed with confidence. In this paper the physical bases of the observations are emphasised to show the important issues in the field and the present state of the observations is indicated.

Type
Invited
Information
Publications of the Astronomical Society of Australia , Volume 10 , Issue 3 , 1993 , pp. 183 - 188
Copyright
Copyright © Astronomical Society of Australia 1993

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Allan, H.R., 1971, in Progress in Elementary Particle and Cosmic Ray Physics, North-Holland, Amsterdam, 10, 171.Google Scholar
Bowden, C.C.G., et al., 1990, AIP Conference Proceedings, American Institute of Physics, New York, 220,75.Google Scholar
Bird, D.J. and Clay, R.W., 1989, Proc. Astron. Soc. Aust., 8, 46.Google Scholar
Bird, D.J., Clay, R.W. and Edwards, P.G., 1989, Proc. Astron. Soc. Aust., 8, 159.CrossRefGoogle Scholar
Cassiday, G.L., et al., 1989, Phys. Rev. Lett., 62, 383.CrossRefGoogle Scholar
Ciampa, D., et al., 1989, Astrophys. J., 346, 151.Google Scholar
Clay, R.W., 1988, Aust. J. Phys. 41, 729.CrossRefGoogle Scholar
Clay, R.W., et al., 1992, Astron. Astrophys., 255, 167.Google Scholar
Gregory, A.G., Patterson, J.R. and Protheroe, R.J., 1987, J. Phys. G, 13, 543.Google Scholar
Greisen, K., 1966, Phys. Rev. Lett., 16, 748.CrossRefGoogle Scholar
Grindlay, J., et al., 1975, Astrophys. J., 201, 82.CrossRefGoogle Scholar
Hillas, A.M., 1984, Nature, 312, 50.CrossRefGoogle Scholar
Jelley, J.V., 1967, in Progress in Elementary Particle and Cosmic Ray Physics, North-Holland, Amsterdam, 9, 41.Google Scholar
Lawrence, M.A., Prosser, D.C. and Watson, A.A., 1989, Phys. Rev. Lett., 63,1121.Google Scholar
Meyhandan, R., et al., 1992, Astrophys. J. 391, 236.Google Scholar
Mufson, S.L., et al., 1990, Astrophys. J., 354, 116.Google Scholar
Nagle, D.E., Gaisser, T.K. and Protheroe, R.J., 1988, Ann. Rev. Nucl. Part. Sci., 38,609.CrossRefGoogle Scholar
Ong, R.A., 1990, Nucl. Phys. B. (Proc. Suppl.), 14A, 273.CrossRefGoogle Scholar
Protheroe, R.J., 1986, Mon. Not. R. astr. Soc., 221, 769.CrossRefGoogle Scholar
Roberts, M.D., et al., 1991, in Proc 22nd Int. Cosmic Ray Conf., 2, 645.Google Scholar
Samorski, M. and Stamm, W., 1983, Astrophys. J. Lett., 268, L17.Google Scholar
Smith, A.G.K. and Clay, R.W., 1990, Aust. J. Phys. 43,373.Google Scholar
Sinclair, D., 1989, Nucl. Instrum. Methods, A278, 583.Google Scholar
Sokolsky, P., Sommers, P. and Dawson, B.R., 1992, Extremely High Energy Cosmic Rays, Physics Reports, 217, 225.CrossRefGoogle Scholar
Teshima, M., et al., 1990, Phys. Rev. Lett. 64, 1628.Google Scholar
Vacanti, G., et al., 1991, Astrophys. J., 377, 467.Google Scholar
Vladimirsky, B.M., Stepanian, A.A. and Fomin, V.P., 1973, in Proc 13th Int. Cosmic Ray Conf., 1, 456.Google Scholar
Weekes, T.C., et al., 1989, Astrophys. J., 342, 379.Google Scholar
Weekes, T.C., 1991, in Proc 22nd Int. Cosmic Ray Conf, 5, 59.Google Scholar