Physical properties of low-luminosity high-redshift lensed galaxies

Details Physical properties of low-luminosity high-redshift lensed galaxies Physical properties of low-luminosity high-redshift lensed galaxies

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329p..39l&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We report the results obtained from NIR ISAAC/VLT and optical FORS/VLT spectroscopy of lensed low-luminosity 1.3 ≤ z ≤ 2.3 galaxies located in the core of the lensing clusters AC114, CL2244-02, and A370. The amplification factor allowed to obtain, for the first time, physical properties (SFR, abundance ratios, mass, age of the burst, dust content, etc) of star-forming galaxies, 1 to 2 magnitudes fainter than in previous studies of Lyman Break Galaxies at z ˜ 3.

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