13 February 2003 Probing the physics of high-z galaxies with the VLT
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This paper addresses the problem of measuring dynamical masses, metallicity, dust content and star formation rates of high redshift galaxies using large 8-10m class ground based telescopes and, in particular, the 8m VLT unit telescopes. The theoretical basis of the various methods and their limitations are also briefly reviewed.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Massimo Stiavelli, Massimo Stiavelli, } "Probing the physics of high-z galaxies with the VLT", Proc. SPIE 4834, Discoveries and Research Prospects from 6- to 10-Meter-Class Telescopes II, (13 February 2003); doi: 10.1117/12.457409; https://doi.org/10.1117/12.457409


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