HIGH-z Lensed Galaxies

Computer Science

Scientific paper

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Scientific paper

This talk reviews the main results recently obtained on the identification and study of very high-z galaxies using lensing clusters as natural gravitational telescopes. We present the last results of a deep near-IR survey of lensing clusters aimed at constraining the abundance of star-forming galaxies at z~6-12. Photometric selection criteria of optical-dropouts were specifically tuned to target star-forming galaxies in this redshift domain. These data were used to constrain the luminosity function of z>6 photometric candidates, and to derive an upper limit for the UV SFR density. The results obtained in lensing fields will be discussed and compared to deep blank-field findings. We also summarize the present state of the spectroscopic follow-up of photometric candidates in lensing clusters using VLT ISAAC and FORS, and the future observations planned with EMIR/GTC.

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