VLT/ISAAC images of quasar hosts at z = 1.5

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Scientific paper

Our present knowledge of quasar host galaxies is essentially limited to z < 1. Fundamental data come specifically from observations obtained using both Hubble Space Telescope (HST, e.g. Disney et al. 1995; Bahcall et al. 1997; Boyce et al. 1998; McLure et al. 1999) and ground-based 4-m-class telescopes (e.g. McLeod & Rieke 1994, 1995; Taylor et al. 1996; Kotilainen, Falomo & Scarpa 1998; Hutchings et al. 1999; Kotilainen & Falomo 2000; Percival et al. 2000).

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