[ ESO ] EIS-Deep 
HDF-South (STIS) Field 
Quicklook Release

 
 

Description
 
In the course of the HDF-South project at ESO EIS has carried out deep observations of the Hubble Deep Field South using the SUSI2 and SOFI instruments at the ESO NTT  and the WFI at the ESO 2.2m telescope. The EIS field called HDF2, which covers the field observed by the WFPC2 of the HST has been observed in 8 filters (U, B, V, R, I, J, H, K),  the field HDF1 (this page) covering the STIS field has been observed in the three SOFI filters J, H, K. Here you will find links to all released data sets. Please read the copyright notice. Details about the observations, data reduction and products will be presented in forthcoming papers. 

For comments or suggestions on the data release or the EIS web pages in general please use our feedback form

Please be aware that the FITS images are quite big. The SUSI frames are about 20 MB, the SOFI frames 5 MB. If you want to request all frames you could use the request form instead where you may request the complete data set.

 
News & Updates
 
This section keeps the history of the data release and major updates of this page in general 
Sep. 14, 1999 - first HDF1 quicklook release 
Aug. 23, 1999 - HDF1/HDF2/HDF3 pages splitted 
Dec. 7, 1998 - Worldwide release of HDF-South data

Warning: The infrared data given here were reduced using the Jitter program of the Eclipse image processing package. Recently, it has been reported that magnitudes computed using this program may be underestimated by about 0.15 mag at faint magnitudes. A re-analysis of these data will be carried out in the near future.

 
Data Products
 
 
The current quick-look release of newly observed R,I,J,H and K band data covers coadded images and associated weight maps only. Other data products will follow as soon as available.
Click on green buttons to retrieve data HDF1: STIS field
optical bands (SUSI2) infrared bands (SOFI)
R I J H K
Image Data 
(coadded)
FITS
Weights
 

Send comments to <eisadm@eso.org> 
Last update: Sep 14, 1999 
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