Hostname: page-component-745bb68f8f-mzp66 Total loading time: 0 Render date: 2025-01-09T09:09:18.372Z Has data issue: false hasContentIssue false
  • English
  • Français

Modeling Faint Galaxy Counts

Published online by Cambridge University Press:  08 February 2017

B. Guiderdoni  and
B. Rocca-Volmerange
B. Guiderdoni
Affiliation:
1Institut d'Astrophysique de Paris 98 bis Boulevard Arago F–75014 Paris France
B. Rocca-Volmerange
Affiliation:
1Institut d'Astrophysique de Paris 98 bis Boulevard Arago F–75014 Paris France 2Laboratoire René Bernas Bât 108 Université Paris XI F–91405, Orsay France

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.

In this paper, we summarize the results of an analysis of faint galaxy counts presented in Guiderdoni and Rocca-Volmerange (1989). We choose to restrict our analysis here to the examination of pure luminosity evolution.

Type
IV. Extragalactic Background Radiation and Cosmology
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 365 - 366
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Dube, R. R., Wickes, W. C., and Wilkinson, D. T. 1979, Ap. J., 232, 333.CrossRefGoogle Scholar
Guiderdoni, B. and Rocca-Volmerange, B. 1987, Astron. Astrophys., 186, 1.Google Scholar
Guiderdoni, B. and Rocca-Volmerange, B. 1989, Astron. Astrophys., in press.Google Scholar
Matsumoto, T. Akiba, M. and Murakami, H. 1988, Ap. J., 332, 575.Google Scholar
Paresce, F. and Jakobsen, P. 1980, Nature, 288, 119.CrossRefGoogle Scholar
Rocca-Volmerange, B. and Guiderdoni, B. 1988, Astron. Astrophys. Suppl. Series, 75, 93.Google Scholar
Toller, G. N. 1983, Ap. J. Letters, 266, L79.Google Scholar