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MS1512-cB58 is an z=2.73 galaxy whose apparent brightness is amplified by30–50X due to gravitationally lensing. The restframe far-UV spectrum of cB58 that was obtained by Keck-I/LRISis `one of the best ultraviolet spectra of a starburst galaxy obtained at any redshift' (Pettini et al. 2000). We have analyzed and modeled the spectrum of this galaxy in order to learn the properties of high-redshift...
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