Titlebook: Deep Fields; Proceedings of the E Stefano Cristiani,Alvio Renzini,Robert E. Williams Conference proceedings 2001 Springer-Verlag Berlin Hei

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https://doi.org/10.1007/978-1-4842-4366-4HDFs are prone to selection biases. These biases are extremely severe beyond . such that a meaningful interpretation of generic galaxy evolution is not possible. We can however extract well defined volume-limited samples at . < 1. The data are entirely consistent with passive/null-evolution for elli

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https://doi.org/10.1007/978-1-4842-4366-4mits (Ferguson et al. [11]). This is also the aim of the FORS Deep Field (FDF), which has about 5 times the field-size of the two Hubble Deep Fields together and, in addition, contains a relatively bright quasar of 18.5mag at . = 3.36 at its center. A full exploration of the FDF multicolor data requ

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Deep Fields978-3-540-45514-1Series ISSN 1431-2433 Series E-ISSN 1611-6143

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Stefano Cristiani,Alvio Renzini,Robert E. WilliamsThis is the first survey of deep field astronomy, based on the new instruments of ESO and STSCI

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Hans Jürgen Ohlbach,Norbert EisingerI give examples of stellar work that is done with data collected in the course of extragalactic surveys, including the Hamburg/ESO objective-prism survey. I list some considerations to be taken into account for future (stellar) surveys.

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