Hostname: page-component-6bf8c574d5-r4mrb Total loading time: 0 Render date: 2025-03-07T07:58:47.678Z Has data issue: false hasContentIssue false
  • English
  • Français

Galaxy Clustering to B = 27M

Published online by Cambridge University Press:  26 July 2016

N. Roche ,
T. Shanks ,
N. Metcalfe  and
R. Fong
N. Roche
Affiliation:
Department of Physics, University of Durham, South Road, Durham DH1 3LE, U.K.
T. Shanks
Affiliation:
Department of Physics, University of Durham, South Road, Durham DH1 3LE, U.K.
N. Metcalfe
Affiliation:
Department of Physics, University of Durham, South Road, Durham DH1 3LE, U.K.
R. Fong
Affiliation:
Department of Physics, University of Durham, South Road, Durham DH1 3LE, U.K.

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 angular two-point correlation function, ω(θ), for galaxies can be used as a probe of their redshift distribution N(z) and, therefore, of galaxy luminosity evolution. Without redshift data, we can still observe the projection onto the two-dimensional sky of the three-dimensional clustering of galaxies. The autocorrelation of this projected distribution is described by ω(θ). Observations have indicated that ω(θ) follows a θ−0.8 power-law (Peebles 1980) and that the index of the power-law remains approximately constant to the faintest limits of photographic surveys (Jones, Shanks & Fong 1987).

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 635 - 643
Copyright
Copyright © Kluwer 1994 

References

Babul, A. and Rees, M.J., 1992. Mon. Not. R. astron. Soc., 255, 498.CrossRefGoogle Scholar
Bruzual, G., 1981. PhD thesis, University of California, Berkeley.Google Scholar
Broadhurst, T.J., Ellis, R.S. and Glazebrook, K., 1992. Nature, 355, 55.CrossRefGoogle Scholar
Cowie, L.L., Songaila, A. and Hu, E.M., 1991. Nature, 354, 460.CrossRefGoogle Scholar
Efstathiou, G., Bernstein, G., Katz, N., Tyson, J.A. and Guhathakurta, P., 1991. Astrophys. J., 380, L47.Google Scholar
Infante, L., 1990. PhD thesis, University of Victoria.Google Scholar
Jones, L.R., Shanks, T. and Fong, R., 1987. ‘High Redshift and Primeval Galaxies’, eds. Bergeron, J., Kunth, D., Rocca-Volmerange, B. and Tran Thanh Van, J., Editions Frontières, France, p. 29.Google Scholar
Koo, D.A. and Szalay, A., 1984. Astrophys. J., 282, 390.Google Scholar
Lilly, S.J., Cowie, L.L. and Gardner, J.P., 1991. Astrophys. J., 369, 79.Google Scholar
Melott, A.L., 1992. Astrophys. J., 393, L45.CrossRefGoogle Scholar
Metcalfe, N., Shanks, T. and Fong, R., 1991a. Gemini, 34, 12.Google Scholar
Metcalfe, N., Shanks, T., Fong, R. and Jones, L.R., 1991b. Mon. Not. R. astron. Soc., 249, 498.Google Scholar
Neuschaefer, L.W., 1992. PhD thesis, Arizona State University.Google Scholar
Peebles, P.J.E., 1980. ‘The Large-Scale Structure of the Universe’, Princeton University Press.Google Scholar
Phillipps, S., Fong, R., Ellis, R.S., Fall, S.M. and MacGillivray, H.T., 1978. Mon. Not. R. astron. Soc., 182, 673.Google Scholar
Rocca-Volmerange, B. and Guiderdoni, B., 1990. Mon. Not. R. astron. Soc., 247, 166.Google Scholar
Roche, N., Shanks, T., Metcalfe, N. and Fong, R., 1993. Mon. Not. R. astron. Soc., 263, 360.CrossRefGoogle Scholar
Stevenson, P.R.F., Shanks, T., Fong, R. and MacGillivray, H.T., 1985. Mon. Not. R. astron. Soc., 213, 953.Google Scholar
Tyson, J.A., 1988. Astron. J., 96, 1.CrossRefGoogle Scholar