Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-19T22:51:05.576Z Has data issue: false hasContentIssue false
  • English
  • Français

The Berkeley-AAO Distant Supernova Search

Published online by Cambridge University Press:  25 April 2016

W. J. Couch ,
S. Perlmutter ,
H. J. M. Newburg ,
C. Pennypacker ,
G. Goldhaber ,
R. Muller  and
B. J. Boyle
W. J. Couch
Affiliation:
School of Physics, University of NSW, PO Box 1 Kensington, NSW 2033
S. Perlmutter
Affiliation:
Lawrence Berkeley Laboratory and Department of Physics, University of California, Berkeley
H. J. M. Newburg
Affiliation:
Lawrence Berkeley Laboratory and Department of Physics, University of California, Berkeley
C. Pennypacker
Affiliation:
Lawrence Berkeley Laboratory and Department of Physics, University of California, Berkeley
G. Goldhaber
Affiliation:
Lawrence Berkeley Laboratory and Department of Physics, University of California, Berkeley
R. Muller
Affiliation:
Lawrence Berkeley Laboratory and Department of Physics, University of California, Berkeley
B. J. Boyle
Affiliation:
Institute of Astronomy, Cambridge
Get access Rights & Permissions [Opens in a new window]

Abstract

A search for Type Ia supernovae at cosmological distances is being undertaken in an attempt to exploit their standard candle property to constrain the mass density of the universe. We describe the rationale for such a program, the observational approach and strategy taken, and the progress made to date. The science that is being generated by the project in additional to supernova detection is also discussed briefly.

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 2 , 1991 , pp. 261 - 265
Copyright
Copyright © Astronomical Society of Australia 1991

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

Boyle, B. J., Shanks, T. and Peterson, B. A., 1988, Mon. Not. R. Astr. Soc., 235, 935.CrossRefGoogle Scholar
Colgate, S. A., 1979, Astrophys. J., 232, 404.Google Scholar
Dresslier, A., 1980, Astrophys. J., 236, 351.CrossRefGoogle Scholar
Evans, R., van den Bergh, S. and McClure, R. D., 1989, Astrophys. J., 345, 752.CrossRefGoogle Scholar
Guth, A., 1980, Phys. Rev., D23, 374.Google Scholar
Kawano, L., Schramm, D. and Steigman, G., 1988, Astrophys. J., 327, 750.Google Scholar
Koo, D. C. and Kron, R. G., 1988, Astrophys. J., 325, 92.Google Scholar
Leibundgut, B., 1988, Ph.D. Thesis, University of Basel.Google Scholar
Miller, G. and Branch, D., 1991, preprint.Google Scholar
Muller, R. A., Newburg, H. J. M., Pennypacker, C. R., Perlmutter, S., Sasseen, T. and Smith, C., 1991, preprint.Google Scholar
Nomoto, K. and Shigeyama, T., 1989, in Particle Astrophysics: Forefront Experimental Issues, Norman, E. B. (ed). World Scientific, Singapore, p 198.Google Scholar
Nørgaard-Nielsen, H. U., Hansen, L., Jørgensen, H. E., Salamanca, A. A., Effis, R. S. and Couch, W. J., 1989, Nature, 339, 523.Google Scholar
Pence, W. D., 1976, Astrophys. J., 203, 39.Google Scholar
Peterson, B. A., Ellis, R. S., Efstathiou, G., Shanks, T., Bean, A. J., Fong, R., and Zen-Long, Z., 1986, Mon. Not. R. Astr. Soc., 221, 233.CrossRefGoogle Scholar
Porter, A. C. and Filippenko, A. V., 1987, Astron. J., 93, 1372.Google Scholar
Rowan-Robinson, M. et al., 1990, Mon. Not. R. Astr. Soc., 247, 1.Google Scholar
Schlechter, P., 1976, Astrophys. J., 203, 297.CrossRefGoogle Scholar
Schramm, D., 1989, in Particle Astrophysics: Forefront Experimental Issues, Norman, E. B. (ed). World Scientific, Singapore, p. 3.Google Scholar
Shanks, T., Stevenson, P. R. F., Fong, R. and MacGUlivray, H., 1984, Mon. Not. R. Astr. Soc., 206, 767.Google Scholar
Tyson, J. A. and Seitzer, P., 1988, Astrophys. J., 335, 552.Google Scholar
van den Bergh, S. and Tammann, G. A., 1991, Annu. Rev. Astron. Astrophys., in press.Google Scholar
Woosley, S. E. and Weaver, T. A., 1986, Annu. Rev. Astron. Astrophys., 24, 205.Google Scholar