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

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Scientific Drivers for ESO Future VLT/VLTI Instrumentation978-3-662-43215-0Series ISSN 1431-2433 Series E-ISSN 1611-6143

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Conference proceedings 2002nd more complex astrophysical data sets. A modern instrument represents a very significant investment in cash, human resources and time. Such a meeting gives us a precious yardstick to evaluate the competitiveness of 1st-generation instruments and associated current and forthcoming proposals for 1st

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1431-2433 r larger and more complex astrophysical data sets. A modern instrument represents a very significant investment in cash, human resources and time. Such a meeting gives us a precious yardstick to evaluate the competitiveness of 1st-generation instruments and associated current and forthcoming proposa

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Galaxy Evolution from Deep Multicolor Surveys: The VLT Perspectiveger than current. For the VLT to be competitive in the long term, and to match the expected performances of VIMOS, I emphasize the need for efficient VLT imagers in the U-B and K bands with field of view of the order of 10’ × 10’.

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The Physics of Gamma-Ray Burst Afterglows and the Nature of Their Host GalaxiesSAX, their distant extra-galactic nature was definitely established in 1997. We discuss the history and current status of the study of gamma-ray burst afterglows, and future VLT observations that can significantly advance the field.

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