Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field

Details Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field

2002-08-07

arxiv.org/abs/astro-ph/0208159v2

Astronomy and Astrophysics

Astrophysics

12 pages, 10 figures, to be presented at "Astronomical Telescopes & Instrumentation", SPIE 2002; corrected authors list

Scientific paper

10.1117/12.457011

The Capodimonte Deep Field (OACDF) is a multi-colour imaging survey on two 0.5x0.5 square degree fields performed in the BVRI bands and in six medium-band filters (700 - 900 nm) with the Wide Field Imager (WFI) at the ESO 2.2 m telescope at La Silla, Chile. In this contribution the adopted strategies for the OACDF data reduction are discussed. Preliminary scientific results of the survey are also presented.

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