Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..385h&link_type=abstract
Astrophysics and Space Science, v. 284, Issue 2, p. 385-388 (2003).
Astronomy and Astrophysics
Astrophysics
1
Catalogs, Galaxies: Fundamental Parameters, Galaxies: Photometry
Scientific paper
The FORS Deep Field project is a multi-colour, multi-object spectroscopical investigation of a ˜ 7′ × ′' region near the south galactic pole based mostly on observations carried out with the FORS instruments attached to the VLT telescopes. It includes the QSO Q 0103-260 (z = 3.36). The goal of this study is to improve our understanding of the formation and evolution of galaxies in the young Universe. In this contribution, the photometric observations are presented. In particular, a combined B and I selected UBgRIJKs photometric catalog of 8753 objects in the FDF is presented and its content is briefly described. The formal 50% completeness limits for point sources, derived from the coadded images, are 25.64, 27.69, 26.86, 26.68, 26.37, 23.60 and 21.57in U, B, g, R, I, J and Ks, respectively.
Appenzeller Immo
FDF-Team
Gabasch Armin
Heidt Jochen
Jäger Klaus
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