Wide-Field Spectroscopy pp 267-275 | Cite as
The Canada France Redshift Survey
Conference paper
Abstract
The properties of field galaxies are investigated based on a sample of ∼ 600 galaxies from z=0.05 to z=1.3. The strongest evolutionary features are found in the luminosity function of the blue galaxies, in the emission line properties and in the disk
surface brightness. It is argued that the star formation rate was higher in the past than today but other mechanisms (such as evolution of the opacity) are also likely contributing to the observed evolution.
Keywords
High Redshift Luminosity Function Star Formation Rate Starburst Galaxy Galaxy Population
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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References
- Benn, C,R., Rowan-Robinson, M., McMahon, R.G., Broadhurst, T.J., Lawrence, A., 1993, MNRAS, 263, 98.Google Scholar
- Broadhurst, T.J., Ellis, R.S., Shanks, T., 1988, MNRAS, 235, 827ADSGoogle Scholar
- Bruzual, G. and Charlot, S. 1993, ApJ, 405, 538.(BC93)ADSCrossRefGoogle Scholar
- Bruzual, G. and Charlot, S. 1995, preprint.Google Scholar
- Bruzual, G. and Charlot, S. 1996, in preparation.Google Scholar
- Colless, M.M., Ellis, R., Taylor, K., Hook, R.N., 1990, MNRAS, 244, 408ADSGoogle Scholar
- Cowie, Hu and Songalai, 1995, Nature, 377, 603.ADSCrossRefGoogle Scholar
- Crampton, D., Le Fèvre, O., Lilly, S. 1995, ApJ, 455, 96 (CFRS V)ADSCrossRefGoogle Scholar
- Davis, M., Peebles, P.J.E., 1983, ApJ, 267, 465ADSCrossRefGoogle Scholar
- Fisher, B.F., Davis, M., Strauss, M., Yahil., A., Huchra, J., 1994, MNRAS, 266, 50.ADSGoogle Scholar
- Fomalont, E.B., Windhorst, R., Kristian, J.A., Kellerman, K., 1991, AJ, 102, 1258ADSCrossRefGoogle Scholar
- Gallagher, Bushouse, Hunter, 1989, AJ, 97, 700ADSCrossRefGoogle Scholar
- Hammer, F., Crampton, D., Le Fèvre, O., Lilly, S., 1995a, ApJ, 455, 88 (CFRS IV)ADSCrossRefGoogle Scholar
- Hammer, F., Crampton, D., Lilly, S., Le Fèvre, O., Kenett, T., 1995b, MNRAS, 276, 1085 (CFRS VII)ADSGoogle Scholar
- Hammer, F., Flores, H., Lilly, S., Crampton, D., Le Fèvre, O., Rola, C., Mallen, G., Schade, D., Tresse, L., 1996, ApJ, submitted (CFRS XIV )Google Scholar
- Kennicutt, 1992, ApJ, 388, 310ADSCrossRefGoogle Scholar
- Le Fèvre, O., Crampton, D., Lilly, S., Hammer, F., Tresse, L., 1995, ApJ, 455, 60 (CFRS II)ADSCrossRefGoogle Scholar
- Lilly, S., Le Fèvre, O., Crampton, D., Hammer, F., Tresse, L., 1995a, ApJ, 455, 50 (CFRS I)ADSCrossRefGoogle Scholar
- Lilly, S., Hammer, F., Le Fèvre, O., Crampton, D., 1995b, ApJ, 455, 75 (CFRS III)ADSCrossRefGoogle Scholar
- Lilly, S., Tresse, L., Hammer, F., Crampton, D., 1995c, ApJ (CFRS VI )Google Scholar
- Lilly, S., Le Fèvre, 0., Hammer, F., Crampton, D., 1996, ApJ, 460, L1ADSCrossRefGoogle Scholar
- Schade, D., Lilly, S., Crampton, D., Hammer, F., Le Fèvre, O., Tresse, L., 1995, ApJL, 451, Ll (CFRS IX )ADSCrossRefGoogle Scholar
- Tresse, L., Rola, C., Hammer, F., Stasinska, G., Le Fèvre, O., Lilly, S., Crampton, D., 1995, MNRAS, in press (CFRS XII).Google Scholar
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