Properties of high-z galaxies as seen through lensing clusters
Astrophysics
2009-10-31 v1
Abstract
We discuss the first results obtained on the study of a sample of high-z galaxies (2 < z < 7), using the gravitational amplification effect in the core of lensing clusters. Sources are located close to the critical lines in clusters with well constrained mass distributions, and selected through photometric redshifts, computed on a large wavelength domain, and lens inversion techniques.
Keywords
Cite
@article{arxiv.astro-ph/9910467,
title = {Properties of high-z galaxies as seen through lensing clusters},
author = {R. Pello and J-P. Kneib and J-F. Le Borgne and B. Fort and Y. Mellier and M. Bolzonella and L. Campusano and M. Dantel-Fort and J-M. Miralles},
journal= {arXiv preprint arXiv:astro-ph/9910467},
year = {2009}
}
Comments
5 pages, 3 figures, Conference Proceedings of the "Clustering at High Redshift" Conference, June 29 to July 2, 1999, Marseille (France)