AAS Meeting #193 - Austin, Texas, January 1999
Session 75. Hubble Deep Field South and North
Display, Friday, January 8, 1999, 9:20am-6:30pm, Exhibit Hall 1

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[75.06] The Hubble Deep Field South: Flanking Fields

R.A. Lucas, S. A. Baum, S. Casertano, D. de Mello, M. Dickinson, H. C. Ferguson, A. S. Fruchter, R. Gonzalez-Lopezlira, I. Heyer, J. Mack, R. Makidon, C. L. Martin, M. Mutchler, E. Smith, M. Stiavelli, H. I. Teplitz, M. S. Wiggs, R. Williams, D. Zurek (STScI), T.M. Brown, J. P. Gardner (GSFC), M. E. Kaiser (JHU), R. N. Hook (ESO/ST-ECF)

Due to the availability of the STIS and NICMOS instruments at the time of the observations, the Hubble Deep Field - South Flanking Fields are more complex and varied than those of the Hubble Deep Field - North. In addition to the WFPC2 Flanking Fields, there are parallel observations in STIS and NICMOS for each, and there are also a series of STIS observations of the NICMOS deep field, and associated WFPC2 and NICMOS parallels as well. In this paper, we will present the data and describe the data reduction process used for the HDF-S Flanking Fields.

If you would like more information about this abstract, please follow the link to http://www.stsci.edu/ftp/science/hdf/hdfsouth/hdfs.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

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