Properties of high-z galaxies as seen through lensing clusters

B. Fort (IAP); Japan); J-F. Le Borgne (OMP); J-M. Miralles (Astronomical Institute; J-P. Kneib (OMP); L. Campusano (U. de Chile); M. Bolzonella (Istituto di Fisica Cosmica; M. Dantel-Fort (Obs Paris); OMP); R. Pello (OMP)

arxiv: astro-ph/9910467 · v1 · submitted 1999-10-26 · 🌌 astro-ph

Properties of high-z galaxies as seen through lensing clusters

R. Pello (OMP) , J-P. Kneib (OMP) , J-F. Le Borgne (OMP) , B. Fort (IAP) , Y. Mellier (IAP) , M. Bolzonella (Istituto di Fisica Cosmica , OMP) , L. Campusano (U. de Chile)

show 4 more authors

M. Dantel-Fort (Obs Paris) J-M. Miralles (Astronomical Institute Sendai Japan)

This is my paper

classification 🌌 astro-ph

keywords clustersgalaxieshigh-zlensingamplificationclosecomputedconstrained

0 comments

read the original 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.

This paper has not been read by Pith yet.

Properties of high-z galaxies as seen through lensing clusters

discussion (0)