Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.stsci.edu/ftp/science/hdf/pipeline/scatteredlight.html
Дата изменения: Thu Feb 13 21:59:54 1997
Дата индексирования: Sun Dec 23 05:16:59 2007
Кодировка:
The Hubble Deep Field - scattered light subtraction

HDF Scattered Light Subtraction:


The HDF observations were carefully scheduled to minimize the effect of scattered light. Nevertheless, Scattered light from the bright earth produces a visible X pattern in about 25% of the HDF data frames. The attached figure shows the distribution of mean sky backgrounds actually obtained. The filled-in portion of the histograms indicates data where the scatttered light patern is visible to the eye. In most cases the higher background associated with the scattered light has only a very small effect on the resultant S/N for faint objects. However, the X pattern is not terribly pleasing to the eye, and may cause problems for some object detection algorithms.

A major difference between version 1 and version 2 of the data reduction was the treatment of scattered light. Details can be found below:

Copyright © 1997 The Association of Universities for Research in Astronomy, Inc. All Rights Reserved.


Harry Ferguson ferguson@stsci.edu 3/1/96