Physical properties of lensed high-redshift galaxies

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

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pgqa.conf..439l&link_type=abstract

Probing Galaxies through Quasar Absorption Lines, IAU Colloquium Proceedings of the International Astronomical Union 199, held M

Astronomy and Astrophysics

Astronomy

Scientific paper

We report the results obtained from optical and near-infrared spectroscopy and also broad-band photometry of lensed low-luminosity galaxies (1.3≤ z≤ 2.3) located in the core of lensing clusters. The amplification factor allowed us to obtain the physical properties (sfr, abundance ratios, mass, age of the burst, dust contents, etc.) of star-forming galaxies, 1 to 2 magnitudes fainter than galaxies in a blank field, using the same indicators as in studies of low-redshift galaxies. A part of this study was concentrated on the dynamics of distant lensed galaxies using integral field spectroscopy (sinfoni/VLT science verification programme).

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