Physical properties of lensed high-redshift galaxies
Por:
Lemoine-Busserolle M., Contini T., Pello R., Le Borgne J.-F., Kneib J.-P., Richard J., Kissler-Patig M., Sanchez S.F.
Publicada:
1 ene 2005
Resumen:
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). © 2005 International Astronomical Union 10.1017/S1743921305003017.
Filiaciones:
Lemoine-Busserolle M.:
Institute of Astronomy, Madingley Road, CB3 OHA, Cambridge, United Kingdom
Contini T.:
LAOMP, 14 Avenue E. Belin, F-31400 Toulouse, France
Pello R.:
LAOMP, 14 Avenue E. Belin, F-31400 Toulouse, France
Le Borgne J.-F.:
LAOMP, 14 Avenue E. Belin, F-31400 Toulouse, France
Kneib J.-P.:
LAOMP, 14 Avenue E. Belin, F-31400 Toulouse, France
Richard J.:
LAOMP, 14 Avenue E. Belin, F-31400 Toulouse, France
Kissler-Patig M.:
ESO, Karl-Schwarzschild-Str.2, 85748 Garching, Germany
Sanchez S.F.:
CAHA, C/Jesus Durban Remon 2-2, E-04004 Almeria, Spain
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