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A z = 2.72 Galaxy Gravitationally Lensed by the Cluster MS 1512+36: Reconstruction and Near-infrared Spectroscopy
2001
Symposium - International astronomical union
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Using archival HST/WFPC2 optical data and near-infrared VLT/ISAAC spectroscopy, the properties of the Lyman-break galaxy cB58 are analyzed. Thez= 0.37 galaxy cluster MS1512+36 lenses it into strongly magnified arcs with ample substructure. The data enables an accurate reconstruction of the source, yielding milliarcseconds resolution; an unparalleled view of the central kpc of thez= 2.72 starburst galaxy.
doi:10.1017/s0074180900220846
fatcat:lmi6h43c7fc4fpo2bjldl4wldi