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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

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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