The EIS Pre-FLAMES Survey: observations of selected stellar fields

Details The EIS Pre-FLAMES Survey: observations of selected stellar fields The EIS Pre-FLAMES Survey: observations of selected stellar fields

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001msngr.105...25z&link_type=abstract

The Messenger, No. 105, p. 25 - 31 (September 2001)

Physics

1

Imaging Surveys

Scientific paper

The primary goal of the ESO Imaging Survey (EIS) project is to produce data sets matching the foreseen scientific goals and requirements of different VLT instruments (e.g. Renzini and da Costa 1997) and to publicly release them prior to the commissioning and first year of operation of these instruments. With this goal in mind, for the past two years EIS has been carrying out the Deep Public Survey (DPS), an optical/infrared deep survey of high-galactic latitude fields, and the Pre-Flames (PF) Survey, a B V I survey of selected stellar fields, to provide suitable samples for VIMOS and FLAMES (Fibre Large Array Multi-Element Spectrograph, Pasquini et al. 2000), respectively.

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