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Titlebook: Scientific Drivers for ESO Future VLT/VLTI Instrumentation; Proceedings of the E Jacqueline Bergeron,Guy Monnet Conference proceedings 2002

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Faint Object Spectroscopy and GRBs: The Need for a Spectroscopic Laboratory at the VLTAcquiring high quality spectra of Gamma-ray Burst afterglows is an observational challenge, as they are transient phenomena at initially unknown redshift. The implications for a spectrograph which can match this challenge are discussed here.
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High Redshift Ellipticals: Prospects for the VLTThe results and the present limits of the observations of high-. ellipticals are discussed in the framework of VLT imminent and future instruments.
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ESO Astrophysics Symposiahttp://image.papertrans.cn/s/image/862738.jpg
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Introduction to Meeting: Towards VLT/VLTI 2nd Generation Instruments ultimately fabricate and operate new advanced capabilities at Parana!. In particular, its scientific input is crucial to define the needs to be filled with present and upgraded 1st Generation instruments, 2nd Generation instruments and Visitor instruments.
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