Volume 379, Number 2, November IV 2001
|Page(s)||740 - 754|
|Section||Numerical methods and codes|
|Published online||15 November 2001|
ESO imaging survey*
Deep public survey: Multi-color optical data for the Chandra Deep Field South
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany
2 Observatoire de la Côte d'Azur, BP 229, 06304 Nice Cedex 4, France
3 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching b. München, Germany
4 Universidade Estadual de Feira de Santana, Campus Universitário, Feira de Santana, BA, Brazil
5 Observatório Nacional, Rua Gen. José Cristino 77, Rio de Janerio, Brasil
Corresponding author: S. Arnouts, email@example.com
Accepted: 17 September 2001
This paper presents multi-passband optical data obtained from observations of the Chandra Deep Field South (CDF-S), located at , . The observations were conducted at the ESO/MPG 2.2 m telescope at La Silla using the Wide-Field Imager (WFI). This data set, taken over a period of one year, represents the first field to be completed by the ongoing Deep Public Survey (DPS) being carried out as a part of the ESO Imaging Survey (EIS) project. This paper describes the optical observations, the techniques employed for un-supervised pipeline processing and the general characteristics of the final data set. Image processing has been performed using multi-resolution image decomposition techniques adapted to the EIS pipeline. The automatic processing steps include standard de-bias and flat-field, automatic removal of satellite tracks, de-fringing/sky-subtraction, image stacking/mosaicking and astrometry. Stacking of dithered images is carried out using pixel-based astrometry which enables the efficient removal of cosmic rays and image defects, yielding remarkably clean final images. The final astrometric calibration is based on a pre-release of the GSC-II catalog and has an estimated intrinsic accuracy of 0.10 arcsec, with all passbands sharing the same solution. The paper includes data taken in six different filters (U'UBVRI). The data cover an area of about 0.25 square degrees reaching 5σ limiting magnitudes of , , , and 24.7 mag, as measured within a aperture. The optical data covers an area of ~0.1 square degrees for which moderately deep observations in two near-infrared bands are also available, reaching limiting magnitudes of and . The current optical/infrared data also fully encompass the region of the deep X-ray observations recently completed by the Chandra telescope. The optical data presented here, as well as the infrared data released earlier, are publicly available world-wide in the form of fully calibrated pixel and associated weight maps and source lists extracted in each passband. These data can be requested through the URL "http://www.eso.org/eis" .
Key words: catalogs / surveys / stars: general / galaxies: general
© ESO, 2001
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